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Int. J. Mol. Sci. 2012, 13(10), 12773-12856; doi:10.3390/ijms131012773
Published: 8 October 2012
Abstract
: The increasing importance of studies on soft matter and their impact on new technologies, including those associated with nanotechnology, has brought intermolecular and surface forces to the forefront of physics and materials science, for these are the prevailing forces in micro and nanosystems. With experimental methods such as the atomic force spectroscopy (AFS), it is now possible to measure these forces accurately, in addition to providing information on local material properties such as elasticity, hardness and adhesion. This review provides the theoretical and experimental background of AFS, adhesion forces, intermolecular interactions and surface forces in air, vacuum and in solution.1. Introduction
The integral form of interaction forces between surfaces of macroscopic bodies through a third medium (e.g., vacuum and vapor) are named surfaces forces, while those that work to hold two bodies in contact are named adhesive forces. If a process between two bodies is perfectly elastic, that is, no energy dissipates during their interaction, the adhesive and surface forces are equal in magnitude [1]. Understanding intermolecular interactions is key to achieving control of materials at the molecular level, which is essential for various areas of physics and for nanotechnology. While the properties of widely used materials such as metals and inorganic semiconductors are governed by covalent or metallic bonding, in soft matter van der Waals (vdW) interactions play a prominent role, though their associated energies are much smaller than covalent or even H-bonds. In most systems involving surfaces and colloidal phenomena, intermolecular (or interatomic) forces are crucial, which act between discrete, nonbonded atoms or molecules over distances significantly greater than molecular bond dimensions [2]. Intermolecular forces are, therefore, nondirectional, nonstoichiometric, and long-range forces [3]. The vdW forces arise from interaction between uncharged atoms or molecules, leading not only to such phenomena as the cohesion of condensed phases and physical adsorption of gases, but also to a universal force of attraction between macroscopic bodies [3,4]. The existence of this force is demonstrated by the adherence of any particles of microscopic size to one another in the absence of special forces of repulsion, as in aggregation of fine powders and coagulation in colloidal dispersions [5].
vdW forces are crucial in a host of phenomena such as adhesion [6], surface tension [7], nanostructured films [8], nanostructures [9,10], nanosystems [11], physical adsorption [12] and wettability [13], and affect the properties of gases, liquids, thin films and the structure of condensed macromolecules [14–16]. They are also relevant in determining film thickness in wetting [17] and surface melting problems [18], interactions involving polymer surfaces [14,19], in free standing films in soap bubbles [20], and in the flocculation and deflocculation of colloidal systems [21]. Direct information of vdW forces became possible in the 1970’s with the surface force apparatus (SFA) [22,23] to explore their magnitude and distance dependence. However, this technique is restricted because it requires smooth, semitransparent, macroscopic surfaces as part of the experimental set-up, which limits the materials that can be examined.
A significant advance was achieved with the atomic force microscopy (AFM) [24–26] which made it possible to observe and manipulate molecular and atomic level features (i.e., measurement and manipulation of vdW forces), in addition to having a well-defined tip-sample geometry with a higher force resolution [27]. Another major application of AFM is force spectroscopy [28,29] where the AFM tip is extended towards and retracted from the surface, and the deflection of the cantilever is monitored as a function of the piezoelectric displacement. AFS has been used to measure nanoscale contacts, atomic bonding, vdW and Casimir forces, dissolution forces in liquids, single molecule stretching and rupture forces [8,28,30,31]. It is ideally suited for short and long-range interactions as well as to study adhesion between solid surfaces, including those bearing deposited polyelectrolytes [32,33]. The forces relevant to AFM are ultimately of electromagnetic origin, but distinct intermolecular, surface and macroscopic effects give rise to interactions with different dependencies. In the absence of external fields, the dominant forces are vdW interactions, short-range repulsive interactions and adhesion forces. Following Butt [28] and Ducker et al. [30], vdW forces between AFM tips and surfaces have been calculated and measured by many researchers [34–39] based on the interaction between a spherical or conical tip and various types of samples.
The aim of this paper is to provide a review of vdW interactions and adhesion forces, including fundamental models and possible applications with AFM. The paper is organized as follows. The basic concepts involved in vdW interactions and use of the Hamaker constant are introduced in Sections 2 and 3, respectively. The main uses of AFS are discussed in Section 4. Section 5 is dedicated to theoretical models and experimental results for vdW and adhesion forces in vacuum, in air and in solution, where the measurements using pull-on and pull-off forces are treated separately. Section 6 closes the paper with final remarks.
2. Van der Waals Interactions
2.1. vdW Interactions between Molecules in Vacuum
In chemistry and physics, the name vdW force is sometimes used as a synonym for the totality of non-covalent forces (also known as intermolecular forces). These forces, which act between stable molecules, are weak compared to those appearing in chemical bonding [40]. All atoms and molecules, even in an inert gas such as helium and argon, exhibit weak, short-range attractions due to vdW forces. Friction, surface tension, viscosity, adhesion and cohesion, are also related to vdW forces [41,42]. These phenomena arise from the fluctuations in the electric dipole moments of molecules which become correlated as the molecules come closer together, giving rise to an attractive force [43]. In 1893, Johannes D. van der Waals (1837–1923) [44] developed a thermodynamic theory of capillarity to explain the behavior of liquids, after having introduced unspecific forces for gas molecules. He established the minimization of free energy as the criterion for equilibrium in a liquid-gas system and applied this to surface tensions, introducing the long-range vdW forces as resulting from dipole and quadrupolar interactions between molecules that make up gases, liquids or solids [45]. vdW forces are the general name given to a set of forces characterized by the same power dependence on distance, having the dipole moment and the atomic polarizability as the important parameters [46]. They include three forces of different origins [47], all proportional to 1/r^{6}, where r is the distance between the atoms or molecules.
The first contribution is due to electrostatic interactions between charges (in molecular ions), dipoles (for polar molecules), quadrupoles (all molecules with symmetry lower than cubic), and permanent multipoles. It is also referred to as Keesom force, named after Willem Hendrik Keesom [48]. Often, these forces occur between two molecules with permanent dipoles, i.e., they originate from the attraction between permanent dipoles as in the molecules of Figure 1a, and are temperature dependent. Such molecules are called polar, e.g., water, which has a dipole moment of 1.85 Debye (1D = 3.336 × 10^{−30} C/m). These permanent dipoles occur when 2 atoms in a molecule have substantially different electronegativity (Figure 1d). Thus, Keesom forces depend on the electronegativity of an atom [49], and more electronegative atoms have a δ^{−} charge. Note that usually the dipole-dipole interaction between two atoms is zero, because atoms rarely carry a permanent dipole. Atoms in an S-state (a spherically symmetric state), such as the H-atom and noble gas atoms, do not carry any multipole and for such systems this force is absent.
The second contribution is the induction (also known as polarization) or Debye force [50], arising from interactions between rotating permanent dipoles and from the polarizability of atoms and molecules (induced dipoles). These induced dipoles occur when one molecule with a permanent dipole repels another molecule’s electrons. A molecule with permanent dipole can induce a dipole in a similar neighboring molecule and cause mutual attraction, as depicted in Figure 1b. Debye forces cannot occur between atoms. The forces between induced and permanent dipoles are not as temperature dependent as Keesom interactions because the induced dipole is free to shift and rotate around the non-polar molecule. The Debye induction effects and Keesom orientation effects are referred to as polar interactions.
The third and dominant contribution is the dispersion or London force (fluctuating dipole-induced dipole) [51], due to the non-zero instantaneous dipole moments of all atoms and molecules. Such polarization can be induced either by a polar molecule or by the repulsion of negatively charged electron clouds in non-polar molecules (Figure 1c). Thus, London interactions are caused by random fluctuations in electron density in an electron cloud. Figure 1d shows that the electron rich side, possessing a δ^{−} charge, and the electron deficient side (with a δ^{+} charge) attract and repel neighboring dipoles. An atom with a large number of electrons will have a greater associated London force than a smaller atom. The dispersion (London) force is the most important component because all materials are polarizable, whereas Keesom and Debye forces require permanent dipoles. The London interaction is universal and is present in atom-atom interactions as well. For various reasons, London interactions (dispersion) have been considered relevant for interactions between macroscopic bodies in condensed systems. Hamaker developed the theory of vdW between macroscopic bodies in 1937 and showed that the additivity of these interactions renders them considerably more long-range, as will be seen in Section 3.
The interaction free energies of these 3 types of forces can be written in a single equation, which describes the total vdW contribution to the free energy of interaction between two small particles 1 and 2:
where C_{ind}, C_{orient}, and C_{disp} are the coefficients due to induction, orientation and dispersion, respectively. This equation together with a repulsive [52], very short-ranged potential due to the overlap between the electron clouds of atoms describes the interaction between isolated molecules in vacuum.
The constant C_{vdW} (C^{(6)}) in Equation 2.1 is given by [53]:
and thus:
in which α_{1} and α_{2} are the electronic polarizabilities of the molecules, μ_{1} and μ_{2} are the dipole moments, ɛ_{0} is the vacuum permittivity (8.854 × 10^{−12} C^{2}J^{−1}m^{−1}), k_{B} is the Boltzmann constant (1.381 × 10^{−23} JK^{−1}), T is the temperature, hν_{1} and hν_{2} are the first ionization potentials of the molecules (ν_{1}, ν_{2} are ionization frequencies (Hz)) and h is the Planck constant (6.626 × 10^{−34} Js). The first term (ν = 0) contains the Keesom and Debye energies, valid for interactions between polar molecules and named polar or entropic contribution [54–56]. The second term (ν > 0) is referred to as dispersion (London) contribution and acts between all molecules [57]. This expression yields good agreement with experimental data, with C_{12} being close to the average of C_{11} and C_{22} for dissimilar molecules 1 and 2. However, this empirical law does not apply to water, which is highly polarized [53].
The total vdW interaction free energy of two molecules 1 and 2 in free space or air, where ɛ = 1, is therefore:
The interaction (Keesom forces) between molecules with permanent dipole moments (polar molecules) (first term) also contain dipole-quadrupole interactions, but these contributions are usually much weaker. The quadrupolar contribution to the atom-surface vdW interaction was discussed by Jiang et al. [58,59] and by Hutson et al. [60]. When molecular constituents of a gas (N_{2}, O_{2} or H_{2}) have no dipole-allowed vibration-rotation transitions, no absorption is seen using conventional spectroscopic techniques [61,62]. However, long-path-length infrared spectroscopy can reveal weak features in the neighborhood of the fundamental vibration of the uncomplexed molecule [63]. The spectra of N_{2}-Ar molecule near fundamental vibration of N_{2} can also present absorption bands [64]. This phenomenon occurs because the complex contains a small dipole moment induced by the electron cloud distortion and molecular quadrupole induction effects [62]. Power and Thirunamachandran [65] concluded that the internal structures of the interacting systems need to be considered to obtain the complete form of vdW forces in terms of the multipole polarizabilities. The retarded vdW forces involving electric quadrupole polarizabilities have also been investigated in detail [66,67].
The vdW dipole-dipole interaction potential can be calculated using the London’s formula (Equation 2.1). The dipole-quadrupole vdW potential and dipole-quadrupole coefficients have been estimated by Mayer [68] using a revised formula by Margenau [69]. The intervening matrix elements appearing in the Margenau formula were expressed by Mayer in terms of polarizabilities, thus obtaining [69–71]:
where C^{(8)} denotes the dipole-quadrupole constant and is described in terms of dispersion coefficients (C^{(6)}). For more details see Khandelwal et al. [71]. Using Equation 2.5, Porsev and Derevianko [72] calculated vdW coefficients C^{(6)} and C^{(8)} of alkaline-earth metal dimers for the interaction of two like atoms in the ground state with high accuracy. This expression is easily extended to include quadrupole-quadrupole dispersion energies as [65]:
The main problem of Equation 2.1 is that it is incomplete, since it neglects quadrupolar polarizations and such effects make an important contribution to C^{(6)}. This may be seen most easily by considering the case of a solid A composed of distinct polarizable atoms B. If dielectric screening (local field) effects are neglected, the atom-surface potential may be written as a sum over long-range atom-atom potential [60]:
Thus, vdW forces between atoms without permanent dipoles may be described as resulting from the interactions of multipoles associated with quantum transitions of the atoms. When the atoms are far apart, the dipole interaction is the only appreciable one. But at short distances, higher dipoles, usually neglected, must be considered [69]. For more details on the role of quadrupole forces in vdW attractions, see relevant papers [58–60,73]. Pauling and Beach [74] calculated the vdW interaction energy of two hydrogen atoms at large internuclear distances using a linear variation function. The authors use 26 terms for the dipole-dipole interaction, 17 for the dipole-quadrupole interaction and 26 for the quadrupole-quadrupole interaction. The interaction energy was given as:
where $\rho =\frac{r}{{a}_{o}}$.
Summarizing, almost all intermolecular forces have four major contributions. There is always a repulsive part, prohibiting the collapse of molecular complexes, and an attractive part. The repulsive part is mainly due to the typical quantum mechanical effect of intermolecular electron exchange. The attractive part consists of three distinct contributions, namely Keesom, Debye and London. It is noteworthy that in some texts the vdW force means the totality of forces (including repulsion), in others it means all the attractive forces, while still in some other cases the term vdW is used solely as a synonym for the London force.
2.2. vdW between Molecules in a Medium
The vdW force can be calculated also for atoms or molecules of dielectric constant ɛ_{1} and ɛ_{2} in a medium of dielectric constant ɛ_{3}. McLachlan [75] presented a generalized theory for vdW forces between infinite media 1 and 2 separated by a medium 3, in which α was the excess polarizability of the molecules. For a small spherical molecule 1 of radius α in a medium 3, the excess polarizability is given approximately by [23,76]:
where ɛ_{1} and ɛ_{2} are the dielectric constants of media 1 and 2, respectively, and ρ is the number of atoms per unit volume.
Inserting Equation 2.3 into Equation 2.2, the entropic (ν = 0) and the dispersion (ν > 0) terms become:
and
in which ɛ_{1}(0), ɛ_{2}(0), and ɛ_{3}(0) are the static dielectric constants of the three media, and ɛ_{1}(iv), ɛ_{2}(iv), and ɛ_{3}(iv) are the dielectric constants of the three media at the imaginary frequencies iv = 2iπk_{B}T/h. If the dielectric medium has one strong absorption peak at the frequency ν_{e} (mean absorption frequency in the ultraviolet region), which is usually different from the frequency ν of the isolated molecule, ɛ_{1}(v) can be written as ɛ (v) = 1 + (n^{2} − 1)/[1 − (v/v_{e})^{2}], so that:
where n is the refractive index, approximately equal to $\sqrt{\varepsilon ({\nu}_{\nu is})}$, where v_{vis} = 5 × 10^{14} s^{−1}. Substituting into Equation 2.7, we obtain:
where n_{1}, n_{2} and n_{3} are the refractive indices for media with molecules 1 and 2 and for the medium 3, respectively. For simplicity, it is assumed that all three media have the same absorption frequency v_{e}.
The total vdW interaction free energy of two identical molecules 1 in medium 3 is therefore:
which is strictly valid only for r >> a, where a is the radius of the molecule.
Some features of the vdW forces are noteworthy:
The vdW force is anisotropic, similarly to the polarizabilities of the majority of molecules, i.e., they have different values for different molecular directions (except for ideal spherical particles);
The orienting effects of the anisotropic dispersion forces are usually less important than other forces such as dipole-dipole interactions;
The vdW force is non-additive. The force between two molecules is affected by molecules nearby, which behave like a medium, and is important for large particles interacting with a surface;
The vdW force is much reduced in a solvent medium.
Retardation effects should be considered to account for the speed with which particles interact (limited to the speed light), especially in media where the speed of light is much smaller than in vacuum [53].
3. Interactions between Surfaces and the Hamaker Constant
The expressions 2.1 through 2.11 are used for interactions between molecules and atoms isolated. For estimating vdW interactions between surfaces, measurements can be performed using an AFM (Figure 2) or theoretical models may be used. In general, there are two approaches to calculating the vdW interaction between two bodies as a function of their separation distance [77]. The first one, referred to as the Hamaker approach [78], determines the vdW interaction of two macroscopic bodies by carrying out the so-called Hamaker-type integration of all the intermolecular interactions. The second approach, based on the Lifshitz theory [79], is more rigorous and gives the vdW interaction energy as a function of macroscopic electrodynamic properties of the interacting media, such as their dielectric permittivities and refractive indices. It should be noted that, regardless of the approach employed, the only difference is in the way the Hamaker constant is determined.
The most direct way to investigate vdW interactions is simply to position two bodies together and measure the force of attraction as a function of the distance between them, as we shall discuss in Section 4. Interactions between surfaces in AFM or SFA may be modeled by summing the attractive and repulsive potential pairs over all interacting atoms. The potential energy is then:
where ξ is the binding energy (well depth), r_{0} is approximately the equilibrium distance between bound atoms (r_{o} = 2^{⅙}σ, with σ being the diameter of one of the atoms) and r is the interatomic distance. For clarity, the potential can also be expressed as:
The tip-surface interactions are normally modeled as schematically shown in Figure 2a [80]. The AFM tip is represented by a conical macroscopic tip of angle ϕ with a sphere of radius R at the end, according to the pyramidal shape determined with scanning electron microscopy (SEM) (Figure 2b) [81]. The atomistic nano-tip is embedded at the base of the sphere.
A simple sum for all the atoms of the tip and sample is a good approximation for repulsive forces. However, the vdW interaction is non-additive; i.e., the interaction of two bodies is affected by the presence of other bodies, and a simple sum of the pair-wise interactions is usually greater than the actual force between the macro bodies [39]. The degree of non-additivity may depend on the density of the medium, i.e., for rarefied media it is possible to assume additive forces [82]. An additive approximation based on the local geometry, material properties and structure of the tip [83] is used in many practical applications, including atomistic simulations for AFM [84], because the full tip contains billions of atoms.
The original work by London [85] focused on the attractions of induced electrical dipoles in individual atoms and molecules. Sokolov [84] generalized this for the forces between spherical particles as a function of particle size and separation, by summing all dipolar interactions of the atoms and molecules of a solid or liquid. He was able to apply this analysis for particles in a fluid, thus introducing constants (now known as Hamaker constants), which provide scales for the vdW forces between particles of various shapes with intervening media. Hamaker used the following approximations: (1) the total interaction is obtained by the pair-wise summation of the individual contributions (additivity); (2) the summation can be replaced by an integration over the volumes of the interacting bodies assuming that each atom occupied a specific volume, with a density ρ (continuous medium); (3) ρ and C (interaction constant defined by London and specific to the identity of the interacting atoms) should be uniform over the volume of the bodies (homogeneous material properties).
The non-retarded energy of interaction between two particles 1 and 2, of volumes V_{1} and V_{2} containing ρ_{1} and ρ_{2} atoms per milliliter is:
where C_{L} is the non-retarded microscopic constant (London constant), i.e., the second term in Equation 2.2, C_{ν}_{>0}. The vdW force is
vdW forces have been obtained by combining Equation 3.3 with Equation 3.4 for bodies of regular geometric form [78]. For example, for two spheres of radii R_{1} and R_{2}, ${F}_{vdW}=\frac{AR}{12{D}^{2}}$ (see Section 5), where A is the Hamaker’s coefficient (or constant), being equal to [78]:
The Hamaker constant depends on C_{L}, a microscopic property of two interacting atoms, then ultimately depending on the strength of the interaction between bodies and the medium surrounding them. It has dimension of energy.
In Equation 3.5, many-body effects of an intervening liquid medium and retardation effects for large distances were ignored. To overcome this problem, Lifshitz [79] presented an approach with multi-body interaction where the polarizability, α, and the first ionization potential in the Hamaker equations were replaced by the static and frequency-dependent dielectric constant, ɛ_{r}, and refractive index, n [86]. Within Lifshitz’ derivation, the Hamaker constant for interaction of medium 1 and 2 across medium 3 (immersion medium) is:
Inserting Equation 2.9 into Equation 3.6, the Hamaker constant may be expressed in terms of dielectric constants, ɛ_{r}, and refractive index, n_{r}, taking into account the approximation of Ninham and Parsegian [20] and Hough and White [87]:
The first term of Equation 3.7 includes Debye and Keesom forces and the second term is the dispersion contribution. In polar condensed media, especially in the presence of electrolytes, the dispersion contribution is normally the only significant term.
For the “symmetric case” of two identical phases (ɛ_{1} = ɛ_{2} and n_{1} = n_{2}) interacting across medium 3, Equation 3.7 reduces to the simple expression:
The non-retarded Hamaker constant comprises non-dispersion or entropic contribution (A_{ν=0}) and dispersion (A_{ν>0}) components, such that A = A_{ν=0} + A_{ν>0}. For identical particles, the Lifshitz continuum theory can be used to estimate the integral parts:
The term k_{B}T defines the interaction as being primarily entropic in nature with a maximum value of $\frac{3}{4}({k}_{B}T)$, since $\left\{\frac{\left({\varepsilon}_{1}-{\varepsilon}_{3}\right)}{\left({\varepsilon}_{1}+{\varepsilon}_{3}\right)}\right\}\le 1$. At T = 300 K, k_{B}T ≈ 3 × 10^{−23} J, which is an order of magnitude less than the dispersion contribution. The actual difference between the two terms (dispersion and electrostatic) will be reduced by mathematical cancellations in the second (dispersion) term in Equation 3.7, but only rarely will the electrostatic contribution constitute the dominant factor in the total interaction.
Thus, for interactions between two hydrocarbon phases across a water film, the Hamaker constant is ${A}_{\nu >0}=\frac{3\left(6.63\times {10}^{-34}\right)\left(3\times {10}^{15}\right)}{16\sqrt{2}}\frac{{\left({1.41}^{2}-{1.33}^{2}\right)}^{2}}{{\left({1.41}^{2}+{1.33}^{2}\right)}^{3/2}}\approx 0.17\times {10}^{-20}\text{J}$, where both of these liquids have roughly the same absorption frequency ν_{e} ≈ 3.0 × 10^{15} s^{−1} [23], h = 6.63× 10^{15} Js and n_{1}, n_{2}, are the refractive indices of water and hydrocarbon, respectively. Concerning the zero-frequency contribution, water has a high static dielectric constant ɛ_{1} = 80, while hydrocarbons have a dielectric constant ɛ_{1} ≈ 2 [23]. The large difference between ɛ_{1} and ɛ_{2} leads to a large zero-frequency contribution to the Hamaker constant of ${A}_{\nu =0}=\frac{3}{4}\left(1.381\times {10}^{23}\right)\left(300\right){\left(\frac{80-2}{80+2}\right)}^{2}\approx 0.28\times {10}^{-20}\text{J}$, giving A_{total} ≈ 0.45 × 10^{−20} J.
For interactions between conducting bodies such as metals, Equation 3.7 cannot be applied, since their static dielectric constant ɛ is infinite (the dielectric permittivity of a metal is given approximately by ɛ(ν) = 1 − ν_{e}^{2}/ν^{2}). For two metals in vacuum, the Hamaker constant is [23]: $A\cong \frac{3}{8\sqrt{2}}h\frac{{\nu}_{e1}{\nu}_{e2}}{{\nu}_{e1}+{\nu}_{e2}}\cong {4.10}^{-19}\text{J}$, in which ν_{e1} and ν_{e2} are the plasma frequencies of the free electron gas, typically in the range (3–5) × 10^{15} s^{−1}.
The equations above exhibit some important features:
The vdW force between two identical bodies in a medium is always attractive (A is positive), whereas the force between two different bodies may be attractive or repulsive. If ɛ_{3} and n_{3} are intermediate between ɛ_{1} and ɛ_{2} and n_{1} and n_{2}, respectively, A is negative (repulsive). Hamaker noted this [78], which was supported by Derjaguin [88], while Visser [89] established the precise conditions necessary for repulsive vdW-London forces. Fowkes [90] was the first to indicate a few possible examples of such repulsions, and van Oss et al. [91] demonstrated the existence of many such systems;
The vdW force between any two condensed bodies in vacuum or in air (ɛ_{3} = 1 and n_{3} = 1) is always attractive (A is always positive);
If ɛ_{3} and n_{3} equal the dielectric constant and index of refraction of either of the two bodies, A vanishes;
The polar term cannot be larger than (3/4) k_{B}T;
Since hν >> k_{B}T, as for interactions in free space, the dispersion force contribution (ν > 0) is usually greater than the dipolar contribution (ν = 0);
The vdW force is much reduced in a solvent medium.
In other words, vdW forces can be attractive, repulsive or zero. The judicious choice of the medium in which an atomic force spectroscopy (AFS) experiment is carried out helps control the vdW forces between tip and sample. For non-conducting (non-metallic) solids and liquids interacting in vacuum or air (ɛ_{3} = n_{3} = 1) the Hamaker constant is typically in the range A = (5–10) × 10^{−20} J, while for interactions in a liquid medium such as water, the Hamaker constant is typically one order of magnitude smaller, in the range A = (0.5–1.5) × 10^{−20} J. For example, A~0.8 × 10^{−20} J is used for lipid bilayers [23], and is estimated as A~(1.0–1.5) × 10^{−20} J for proteins interacting in water or salt solutions, being slightly lower in high salt concentrations [92]. Hamaker constants for materials commonly used in AFS are listed in ref. [93]. Usual AFM tips are made of silicon nitride or silicon, one common substrate is mica and the colloidal probes are usually silica spheres.
In Figure 3, one example of an experimental attractive force curve for a diamond tip against a graphite surface is shown, together with an attempt of fitting the curve with a vdW force (curve A) using a reasonable value of A [94]. To obtain the best fit for a sphere on flat geometry, it is necessary to postulate an unreasonably large value of AR [95]. Even then, the fit is very poor, the prediction being too short-range. One suggestion is to consider more complex types of long-range interactions, which depend on a change in material properties of the near-surface region, giving increased attraction at small separations, as we will see later.
There are two possibilities to obtain the Hamaker constant: measuring the dielectric function for all frequencies or measuring the attraction force for a known geometry directly. To measure the dielectric function, use may be made of spectroscopic methods such as electron energy loss spectroscopy, absorption in the UV-vis. range, infrared and microwave spectroscopy [96]. A method to quantitatively evaluate the Hamaker constant using the jump-into-contact effect in AFM was developed by Das et al. [97]. They found that the jump-to-contact (see more details in Section 4) of the cantilever in the atomic force microscope is caused by an inherent instability in the motion of the AFM cantilever. The Hamaker constant was determined from the cantilever deflection at the jump-to-contact using the force constant of the cantilever and the tip radius of curvature, all of which can be obtained with AFM measurements. This method is applicable only to surfaces that have vdW interaction as the tip-sample interaction. Another interesting method consists in calculating the work of adhesion and then relating it to the Hamaker constant through [98]:
Where β and n depend on the geometry of the system and can be calculated from the force laws listed in Table 1.
The equations for surface interactions previously mentioned were derived for the situation in which the interacting units were separated by a vacuum. Special features appear when the measurements are performed under ambient conditions because both the tip and the sample surface may be coated with a thin water film. vdW interactions are affected by adsorbed layers of a dielectric material, with the Hamaker constant depending on the permittivity of the adsorbed layers. The effective Hamaker constant A_{iki}_{′} for two surfaces i and i′ with adsorbed layers j and j′ of thickness t and t′, across medium k can be evaluated using [103] (see Figure 4):
where, for this case, j = j′ (water).
Burnham et al. [94] suggested an expression for an effective Hamaker constant, based on a simple situation where a dry gas k separates two identical solids i that are both coated with layer j with thickness t:
Thus, for reasonably small values of t/D, A = (A_{jkj} − 2A_{ijk} + A_{iji}) + (A_{ijk} − A_{iji})(6t/D).
On the basis of reasonable values of t and of the constant term in Equation 3.13, Burnham et al. [94] obtained the fitting shown in Figure 3 (curve (b)). Considering the surface layer (Equation 3.13) the best fitting was obtained.
The terms in Equation 3.12 can be found by combining relations, which is frequently done for obtaining approximate values for unknown Hamaker constants in terms of known ones. Considering A_{ikj} from Equation 3.12 as the non-retarded Hamaker constant for media i and j interacting across medium k[23]:
where A_{ii}, A_{kk}, and A_{jj} are the Hamaker constant of the AFM tip, the medium and water, respectively. As an illustration of the above relations let us consider a system comprising silicon (i), air (or vacuum) (k), and water (j), for which Equation 3.14 would predict: ${A}_{ikj}\approx \left(\sqrt{18.65}-\sqrt{0}\right)\left(\sqrt{3.7}-\sqrt{0}\right)\times {10}^{-20}=8.3\times {10}^{-20}\text{J}$. When two surfaces of component i are separated by a medium of component k, i.e., i = j, the effective Hamaker constant is approximated by:
where A_{ii} is the Hamaker constant for component i in a vacuum, and A_{kk} is the corresponding constant for component k. As the Hamaker constants for i and k become similar, the effective Hamaker constant tends toward zero, and the free energy of attraction between the two surfaces is also reduced to zero. As discussed in Section 5, such a reduction in attractive forces due to an intervening medium provides one way to successfully prevent spontaneous joining of surfaces [2].
The Supplementary Material of this Review lists Hamaker constants for AFM studies, including values of a variety of conditions under which the force curves were measured, in some cases attaching colloidal spheres of different materials to AFM cantilevers. It should be stressed that Hamaker constants for many practical systems are still unknown, for they may be difficult to determine [104].
4. Introduction to Atomic Force Spectroscopy (AFS)
AFM can be used to determine the dependence of the interaction on the probe-sample distance at a given location [105], in the so-called atomic force spectroscopy (AFS). AFS may be performed in two ways: local force spectroscopy (LFS) and force imaging spectroscopy (FIS). In LFS, the force curve is determined at a particular location on the sample surface, as shown schematically in Figure 5. Force curves are plots of the deflection of the cantilever (force) versus the extension of the piezoelectric scanner (sample displacement); if the cantilever spring constant is known, then the force can be calculated or measured. These curves can be used to measure the vertical force that the tip applies to the sample surface and to study the surface properties of the sample, including the elastic deformation of soft samples. They can also be used to monitor the unfolding of protein molecules as the latter are pulled from the sample surface by the AFM tip.
In the diagram of Figure 5 is shown a typical F vs. D curve obtained with a soft cantilever on a hard sample. Segment a–d represents the first half cycle (approach curve) while segment d–h is the second half cycle (withdrawal curve) of the curve. These cycles can be divided roughly into three regions: the contact line, the non-contact region and the zero line. The zero line is obtained when the tip is far from the sample and the cantilever deflection is close to zero. For measurements in a liquid, this line gives information on the viscosity of the liquid [106]. When the sample is pressed against the tip, the corresponding cantilever deflection plot is referred to as the contact line, which can provide information on sample stiffness. The most interesting regions of the force curve are two non-contact regions, containing the jump-to-contact (JTC) and the jump-off-contact (JOC). The non-contact region in the approach curve provides information about attractive (vdW or Coulomb force) or repulsive forces (vdW in some liquids, double-layer, hydration and steric force) before contact; this discontinuity occurs when the gradient of the tip-sample force exceeds the spring constant of the cantilever. The maximum forward deflection of the cantilever multiplied by the effective spring constant of the cantilever is the pull-on force [94]. The non-contact region in the withdrawal curve contains the jump-off-contact, a discontinuity that occurs when the cantilever’s spring constant is greater than the gradient of the tip-sample adhesion forces. The maximum backward deflection of the cantilever multiplied by the effective spring constant of the cantilever is the pull-off force [94].
At the start of the cycle (point a) a large distance separates the tip and the sample, there is no interaction and the cantilever remains in a non-interacting equilibrium state. As separation decreases, in a–b the tip is brought into contact with the sample at a constant speed until it reaches a point close to the sample surface (point b). Once the total force gradient acting on the tip exceeds the stiffness of the cantilever, the tip jumps to contact (JTC) with the sample surface (b–c). JTC is often due to capillary forces from the moisture layer that covers the tip and the sample surface. In (c–d), the tip and sample are in contact and deflections are dominated by mutual electronic repulsions between overlapping molecular orbitals of the tip and sample atoms. The shape of segment (c–d) indicates whether the sample is deforming in response to the force from the cantilever. The slope of the curve in the contact region is a function of the elastic modulus and geometries of the tip and sample [29].
Segment (d–e) represents the opposite movement to segment (c–d), with the tip being withdrawn. If both segments are straight and parallel to each other, there is no additional information content. If they are not parallel, the hysteresis gives information on plastic deformation of the sample [26,29]. In segment (d–f) the sample is being retracted and adhesion or bonds formed during contact with the surface cause the tip to adhere to the sample. As the sample continues retracting, the spring force of the cantilever overcomes the adhesion forces and the cantilever pulls off sharply (f–g). In this segment, several long and short-ranged forces become effective (see Table 2) [43,107,108]. The force at point f is the total adhesive force between the tip and the sample. In segment (g–h) the cantilever is moved upwards to its undeflected or noncontact position. The adhesive force can be measured through deflections of a spring, according to Hooke’s law:
where the cantilever deflection δ_{c} is determined by the acting force F and the spring constant of the cantilever, k_{c}. Although cantilevers have a spring constant defined by the manufacturer, it is important to calibrate the system, as there have been cases where the actual spring constant was one order of magnitude off the nominal value. A number of methods for determining the spring constant have been proposed [109–112]. In the calibration, one has to measure the resonant frequency of the cantilever before and after addition of a small mass onto the tip [109]. Moreover, one has to determine the unloaded resonant frequency using the cantilever’s density and dimensions [110,113], or through thermal fluctuations of the cantilever [114,115].
In summary, using AFS makes it possible to obtain the following information: (i) the magnitude of the long-range attractive and adhesive forces [29,81]; (ii) estimation of the point of tip-sample contact; (iii) the tip-sample contact area; and (iv) the elastic modulus and plasticity of thin and thick films [116,117].
In force imaging spectroscopy (FIS), force curves are recorded at a large number of sample surface locations [118]. Figure 6 shows Young’s modulus maps obtained from nanomechanical mapping measurements for poly(styrene-b-ethylene-co-butylene-b-styrene) (SEBS) samples having different compositions [119]. The characteristic phase-separated morphologies consisting of high and low Young’s modulus regions are clearly exhibited. The contrasts in the maps reflect the variations in Z-travel needed to damp the amplitude of the interacting probe to a trigger level chosen by an operator. In the Young’s modulus maps, the light green areas with higher Young’s moduli are considered to be hard PS blocks, while the red areas with lower Young’s moduli are considered to be soft PEB blocks. Such experiments allow precise identification of surface locations occupied by different blocks and offer experimental data for nanomechanical models for extracting quantitative data.
The FIS mode can be used to measure adhesion [120], hardness, or deformability of samples and vdW interactions. Maps of interaction can be produced also by measuring the vertical displacement of the sample–driven by the piezoscanner–and the deflection of the cantilever with respect to its position at rest on several points of the surface. Force curves are digitally acquired at 100 or more points equally spaced from each other over the sample surface scanned area. By way of illustration, Figure 7 shows an adhesion map with islands of repulsive forces with diameter varying from 100 to 470 Å (average size = 306 ± 109 Å) in a matrix with attractive forces. These islands are made of protonated, semi-crystalline PANI. The result presented by AFS is in surprisingly good agreement with the value (200 to 300 Å) estimated by Zuo et al. [121] based on ac conductivity measurements. These charged domains provided new evidence for the formation of conducting islands [121–123].
Leite et al. [81] measured the variability in adhesion due to contamination and surface roughness using adhesion maps from the distribution of the measured forces. In addition to identifying regions contaminated by either organic compounds or adsorbed water, it was possible to estimate the adhesion force in air and water. The experimental results were in good agreement with theoretical calculations, where the adhesion forces in air and water were mostly associated with capillary and vdW forces, respectively. A small long-range repulsive force was observed in water due to the overlapping electrical double-layers formed on both the tip and sample surfaces.
Tapping mode AFM (Intermittent Contact-AFM) has also been used to map tip-surface interactions [124,125]. In this mode, the cantilever is oscillated at its resonant frequency at a position just above the surface, so that the tip is only in contact with the surface for a very short time. A feedback loop ensures that the amplitude of the cantilever oscillation remains almost constant. It is possible to measure the phase difference between the driving oscillation and the detected cantilever oscillation, generating a phase difference map. An increase in the phase difference arises from a stronger tip-sample interaction, creating contrast in the phase map [126]. There are still, however, problems associated with the methods for determining tip-sample interactions, and the nature of interactions leading to image contrast is under debate [127]. Kitamura and Iwatsuki [128] analyzed the use of noncontact atomic force microscopy to detect variations in surface composition, i.e., to detect a ‘spectroscopic image’ of the sample. The authors showed that long-range forces depend on the composition of the AFM tip and of the sample. They demonstrated how vdW forces may be utilized for AFM spectroscopy. vdW interactions have been detected for samples under high vacuum conditions [129–131].
5. Measuring and Calculating van der Waals and Adhesion Forces
The interactions between two surfaces depend on whether the system is in vacuum, in air or ambient conditions or in a liquid. In vacuum, there are long-range vdW and electrostatic (Coulombic) forces, while at smaller surface separations–corresponding to molecular contact (D ~ 0.1–0.2 nm)—there are additional forces such as covalent, hydrogen and metallic bonding forces. All of these forces determine the adhesion between bodies of different geometries, the surface and interfacial energies of planar surfaces, and the strengths of materials, grain boundaries, cracks, and other adhesive junctions [21]. When exposed to a vapor, e.g., atmospheric air, two solid surfaces in or close to contact may have a surface layer of chemisorbed or physisorbed molecules, or a capillary condensed liquid bridge between them [132,133]. Each of these effects can drastically modify adhesion. The adhesion force usually decreases, but in the case of capillary condensation, the additional Laplace pressure between the surfaces may cause the adhesion to be stronger than in an inert gas or vacuum. The force between two surfaces totally immersed in a liquid is again different from that in vacuum or air. The vdW attraction is generally reduced, but other forces come into play, which can qualitatively change both the range and even the sign of the interaction, as discussed in Section 3. The attractive forces depend on the surfaces characteristics, being stronger for two hydrophobic surfaces interacting in water and weaker for two hydrophilic surfaces. In addition, the force may no longer be purely attractive; it can be repulsive, or the force can change sign at some finite surface separation.
Because the factors mentioned above are important for determining the strength of vdW interactions and adhesion in different systems, we shall consider them in separate subsections, also distinguishing between measurements of pull-on (approach curve) or pull-off forces (withdrawal curve).
5.1. Interactions in Vacuum
5.1.1. Attractive Forces (pull-on forces)
The attractive forces or pull-on forces, F_{pull-on}, in vacuum, can comprise two components: the non-electrostatic, F_{ne}, and the electrostatic forces, F_{e}:
where F_{ne} comprise the vdW forces (F_{vdW}). Thus, the pull-on force in vacuum is given by:
5.1.1.1. Electrostatic Forces (F_{e})
The electrostatic forces come basically from the effect of electric fields on electrical charges [134]. The measurement of these Coulomb forces can be useful to investigate the tip shape and its influence on surface roughness and mechanical deformation at contact [29,134,135]. To describe these concepts, several analytical models exist in the literature, which are based on three assumptions [134]:
Surfaces are smooth, and the surface topography is not taken into account;
The materials are conductive with charge uniformly distributed, only on the surface, and the electric field is normal to the surface;
There is no charge between contacting objects.
5.1.1.1.1. Plane–Plane Model
This model gives the electrostatic pressure and requires the electrostatic force given by [134,136]:
where ε_{0} is the free space permittivity, V is the potential difference, A is the area of contact and z is the separation distance (gap). Additionally, very small distances between objects are used when the contact is estimated for flat surfaces.
5.1.1.1.2. Sphere–Plane Model
The sphere models have been developed for more complex shapes and larger separation distances. These models give an approximation of the electrostatic forces for the contact between a conductive sphere and a conductive plane, thus simulating the case of an AFM tip and the sample. For all separation distances a general expression has been developed [98,134,137]:
where ε_{0} is the free space permittivity, R is sphere radius (m), V is the potential difference, L is the length of the tip (m) and z is the separation distance (gap).
5.1.1.1.3. Uniformly Charged Line Models (Conical Tip Models)
The principle consists in replacing the equipotential conducting surfaces by the equivalent image charges. The main hypothesis is that the cone may be approximated by a charged line of constant charge density λ_{0} given by Hao et al. [138] for a small aperture angle (θ≤π/9) as:
The resulting force is [93]:
in which L ≤ z ≤ R. This model fits well the experimentally measured forces at large tip-sample separations.
5.1.1.1.4. The Asymptotic Model
The principle is to decompose a conical tip into infinitesimal surfaces [137]. The contribution of the apex and the spherical tip are evaluated separately and then added to get the total force, which is given by:
where ${k}^{2}=\frac{1}{{\left\{\text{ln}\left[\text{tan}\left(\frac{\theta}{2}\right)\right]\right\}}^{2}}$.
5.1.1.1.5. The Hyperboloid Model (Hyperboloid Tip Model)
In this model the tip is represented by hyperboles bounded by a maximum distance r_{max} from the axis. The expression is derived by solving the Laplace equation in a prolate spheroidal coordinate system and by treating the tip-sample geometry as two confocal hyperboloids [139,140].
in which ${\eta}_{tip}=\sqrt{z/z+R}$ and r_{max} is the cut-off radius introduced to avoid divergence.
5.1.1.1.6. The Cylindrical Model
This model differs from the previous one for being two-dimensional and not axisymmetrical. Using the analytical model for the cylinder–plane contact described by Smythe [141], the electrostatic force is given by [134]:
where ε_{0} and ε_{R} are the permittivity of free space and the relative permittivity of the environment, respectively and λ is the wavelength.
5.1.1.2. van der Waals Forces (F_{vdw})
The first attempts to measure vdW interactions began in the 1950’s with [88] and [142] for optically flat, polished glass plates in a vacuum. Experiments were performed with separations, D, between 500–2000 nm [142] and 500–950 nm [143]. Measurements between a sphere and a plate were made for separations of 100–700 nm [99] and 94–500 nm [143]. The separations between surfaces used in these experiments are beyond the range over which non-retarded vdW interactions dominate, usually of the order of 10 nm [78]. Thus, the values obtained are for retarded interactions, or in the transition regime between the two. The measurement of non-retarded vdW interactions required substantial improvements in sample smoothness and control of separations, obtained only with sophisticated equipment.
The first inter-surface force measurement at separations of the order of 1–10 nm was conducted by [47], using crossed cylindrical surfaces of cleaved mica, separated by air. A piezoelectric crystal was used to control the separation precisely. This mechanism was adapted to measure the surface forces between crossed mica cylinders in aqueous solutions [22], now named the surface force apparatus (SFA). The forces between mica surfaces were measured from 1–100 nn in aqueous KNO_{3} solutions at pH 6. With AFM force curves have been obtained for various materials separated by vacuum or liquids [98,144–146].
An analytical expression for the force curve (pull-on force) may employ the derivation of Hao et al. [138]. The cantilever-sample system can be described by means of a potential w_{tot}, which is the sum of three potentials: w_{tot} = w_{cs}(D) + w_{c}(δ_{c}) + w_{s}(δ_{s}). Here w_{cs}(D) is the interaction potential between the tip and sample (D is the sample-tip distance), e.g., the Lennard-Jones potential, w_{c}(δ_{c}) is Hooke’s elastic potential of the cantilever (w_{c}(δ_{c}) = ½ k_{c}δ_{c}^{2}) and w_{s}(δ_{s}) is the potential that describes the sample deformation according to Hooke’s law (w_{s}(δ_{s}) = ½ k_{s}δ_{s} ^{2}), where k_{c}, k_{s}, δ_{c}, and δ_{s} are the cantilever and sample spring constants, the deflection of the cantilever and deformation of the sample, respectively.
The Lennard-Jones (L-J) potential is composed of two interactions: the vdW attraction and the Pauli repulsion [147,148], which is the repulsion caused by the overlap of the electron clouds of two atoms. The quantum mechanical calculations for the resulting potential of the overlap of the wave functions yield an exponential dependence [149], which is normally approximated by a power law with n > 9. For the Lennard-Jones potential n = 12 is chosen. At relatively large separations, typically of the order of 1 nm or more, vdW interactions lead to a negative interaction potential and thus to attractive forces, which are present in any environment. For a pair potential in the form w(D) = −G/D^{n}, where G is the constant in the atom-atom pair potential, and assuming that the potential is additive, the interaction energies between macroscopic bodies may be obtained via integration. In the case of two interacting spheres at distance D, the force F(D) can be obtained by integrating over small circular sections of surface 2πxdx on both spheres [150], as depicted in Figure 8:
in which f(z) is the normal force per unit area. Thus, the total force between the sphere and the plate is:
where w(D)_{planes} is the energy per unit area between two identical flat plates (surfaces), and R_{1} and R_{2} are the radii of the two spheres interacting. This relationship shows that the force between a sphere and a plate is directly proportional to the energy per area between identical flat plates. Equation 5.11 is known as the Derjaguin approximation [150,151], which applies when R >> D [152], i.e., whenever the interaction range and the separation D are much smaller than R_{1} and R_{2}. From the Derjaguin approximation, with R_{2} >> R_{1}, one obtains the force between a sphere and a flat surface:
where R_{t} is the radius of the AFM tip.
vdW energies between macroscopic bodies in vacuum may be computed via integration only in the approximation that the forces are assumed additive and non-retarded. The interaction laws obtained via integration are listed in Table 3 for the most common geometries. For extended electrically neutral bodies, e.g., a sphere above a flat plane, a proper accounting of geometry must be included, resulting in an interacting force that varies with the sphere-substrate separation as D^{−2}.
Using the form of the vdW potential for two flat surfaces (Derjaguin’s equation), the vdW force between a sphere and a flat surface in vacuum is [153]:
where z_{c} is the height from the bottom to the tip above the surface in the absence of external forces, z or δ_{c} is the deflection of the cantilever due to short- and long-ranged forces acting on the tip and D is the tip-surface separation, D = z_{c} − z (see Figure 9).
The experimental determination of the tip-surface separation (D) (see Table 1), often-named jump-to-contact distance (D_{jtc}), is not straightforward, requiring a more accurate quantitative analysis. When AFM is operated in vacuum and the tip and sample are electrically neutral, the tip will be subjected to three forces: a spring force due to the cantilever, a short-ranged repulsive contact force, and a long-ranged attractive vdW force. In the absence of short-ranged repulsion, the tip position at equilibrium will be such as to balance the vdW and spring forces. This point may be determined by finding the energy minimum for the system. Additionally, to convert the diode-voltage versus sample-displacement data to a force vs. tip-sample separation curve, it is necessary to define zeros of both force and separation and to convert the diode signal to cantilever deflection and force. The zero of force can be chosen when the deflection is constant (where the tip and sample surface are far apart), and the zero of distance can be chosen when the cantilever deflection was linear with respect to the sample at large forces [144]. In the experiments, the relationship between sample displacement and diode response in the region of constant compliance is independent of the surface force and is used to convert the diode response into the deflection of the cantilever. This conversion is then used to determine changes in tip-surface separation, with the relative surface separation being calculated by adding the displacement of the sample to the deflection of the cantilever.
The potential energy may be written as [154]:
Local minima of the energy function are found by setting its derivative to zero:
Thus, the length scale at which the vdW forces are able to deflect the spring significantly is given by $\beta \equiv \sqrt[3]{\frac{A{R}_{t}}{{k}_{c}}}$. The jump-to-contact distance, D_{jtc}, is specified as ${D}_{jtc}\equiv \frac{\beta}{\sqrt[3]{3}}$ [154], and:
For typical values of the Hamaker constant, radius tip and spring constant (10^{−19} J, 50 nm, and 0.1 N/m, respectively), the tip will jump into contact with the surface when it is 26 Å apart [154].
Butt et al. [98] considered the sample stiffness, k_{s}, in which case the potential energy described in Equation 5.15 can be written as:
where δ_{s} is the deformation of the sample. For a sphere-plane system, it can be shown that the distance at D_{jtc} is given by:
where ${k}_{eff}=\frac{{k}_{c}{k}_{s}}{{k}_{c}+{k}_{s}}$.
Equation 5.18 allows one to calculate A, R (k_{eff}) and D_{jtc} once the elastic constant of the cantilever k_{c} and the effective elastic constant of the system k_{eff} are known. Equation 5.18 differs from Equation 5.16 due to the inclusion of the sample elastic constant, k_{s}. For separations D_{jtc} < r_{0}, where r_{0} is an intermolecular distance introduced to avoid the divergence of Equation 5.9, often given by r_{0} = 0.165 nm [23], the resulting vdW force is identified with the adhesion force derived from one of the models presented in the previous section.
Several experiments have demonstrated the capability of AFM in probing vdW forces with high resolution in distance and force [29,93,98] with measurements in vacuum or in dry N_{2} for systems such as silicon tungsten/graphite or tungsten/gold [116], tungsten/mica or tungsten/alumina [155] and Ni/Au [156]. Burnham et al. [155] measured forces between a tungsten tip and several samples under dry nitrogen, as shown in Table 4. They concluded that the attraction force with AFM depends on the sample surface energy and contact area, which was normalized for the tip radius by dividing by 4πR_{t}. Goodman and Garcia [157] estimated vdW forces in vacuum as being of the order of 10–20 nN, whereas these forces between metallic tips and samples were as high as 100 nN when the AFM was operated in the purely repulsive mode.
The vdW interactions (energy and force) between a spherical particle and an infinite cylinder were derived by [158] using the method of additive summation of the pair interactions described by the potential of the general form $w(r)=-\frac{{C}_{vdW}}{{r}^{m}}$, where C_{vdW} is the interaction constant. The authors also derived a compact formula for the energy of vdW interactions of a point-like particle (atom, molecule) with a sphere and a cylinder for the case of arbitrary m. This study is important since many problems in physics, chemistry, and biology deal with the vdW interaction of fine spherical particles with bodies of cylindrical shape, like nanowires, nanotubes, and fibers. The non-retarded vdW force between a sphere (s) and a cylinder (c) is [158]:
where R _{s} and R _{c} are the radii of the sphere and cylinder, respectively, D is the distance between both, c = D + R_{s} + R_{c}, p = 1+s/2, s = ((D+R_{s})^{2}−R_{s}^{2})/2cR_{c}. K and w are the complete elliptic integrals defined as [159]:
For distances larger than 20 nm, retardation effects (Casimir Effects) become dominant. Casimir and Polder [160] showed that the interaction energy between two atoms is approximately described by −C_{3}/r^{7} rather than −C_{1}/r^{6}, i.e., if the time required for light to travel from atom 1 to interacting atom 2 is comparable to the inverse of the frequency of fluctuations dipoles, attraction is reduced. Therefore, at distances r ≥ λ_{0}, where λ_{0} is the characteristic wavelength of radiation in the spectra of interacting atoms given by λ_{0} = 2πcϖ_{0} ^{−1} [158] (ϖ_{0} is the atomic frequency, c is the light velocity in vacuum), the dispersion interaction is no longer instantaneous. It is determined by the finite time of the signal propagation from one dipole to another, 2rc^{−1}, which results in the retardation of the vdW interaction. In the limit r >> λ_{0} the London forces do not exist. In this case, the vdW interaction is fully retarded and reduced. The full expression for the Casimir and Polder potential, valid for all separations r >> a, is given by a cumbersome integral for which it is convenient to use a simple analytical approximation.
In the case of AFM systems, the retarded vdW force between a sphere and cylinder is:
Theoretical issues of vdW forces in connection with force microscopy are discussed in detail in Hartmann [161]. Wennerstrom et al. [162] have also discussed the origins and effects of retardation on interactions between bodies.
5.1.2. Adhesion Forces (Pull-Off Forces)
The concept of adhesion force or pull-off forces, a material property reflecting the influence from elastic deformation, surface roughness [163–165], and interfacial surface energy, is an efficient, quantitative measure of the adhering tendency of a powder or surface. The adhesion forces, F_{adh} or F_{pull–off}, in vacuum, can comprise two components: the non-electrostatic, F_{ne} and the electrostatic forces, F_{e} [166]:
where F_{ne} contains the vdW forces (F_{vdW}) or vdW adhesiveness and the chemical bonding force (F_{chem}). Thus, the total adhesion force or pull-off force in vacuum is given by:
5.1.2.1. Electrostatic Forces (F_{e})
Owing to local inhomogeneities in the work function of a material, a microscopic charge transfer takes place, resulting in a dipole. If the work function of two patches varied by a total Δφ, a particle would have a dipole moment p = 4πɛR^{2}Δφ. If the cores of two particles are separated by r, the force on each particle will have a maximum value of [167]:
and will vary with the orientation of the dipoles. This model is referred to as the patch charge model.
The interactions amid particles and surfaces become more intricate than simply distinguishing between patch charges and vdW interactions, since real particles are not perfect spheres and usually have an electric charge. For illustration, a 10 μm xerographic toner particle may have a typical charge of the order of 8fC [168]. If these toner particles were spherical and the charge uniformly distributed over their surface, the Coulombic forces would be small compared to the vdW interactions for the particles in contact with the surface. Therefore, the Coulombic attraction between these particles in contact with a grounded metal plate would be given simply by [167]:
where α is a factor to correct for the polarization of the particle, q and R are the charge and radius of the particle, respectively and ɛ_{0} is the permittivity of free space. For a material with a dielectric constant (k) of 4, α = 1.9. For the ideal particle under consideration, F_{I}= 10 nN [167].
Particles can acquire charge in several ways, with the most common source being charge buildup in powder handling due to triboelectric charge transfer. Tribocharging is expected to result in non-uniform charge distributions over particle surfaces, and this nonuniformity can play a significant role in adhesive effects [169]. Hays [168] proposed that the total charged area A_{t} on a tribo-electrically charged toner particle represents a small part of the total toner particle’s surface area. Based on Hays’ model, the total charge would be Q = σA_{t}, where σ is the surface charge density. A small fraction, like 20%, of the charged surface area, A_{c}, might be in close proximity to the conducting surface. If A_{c} is much larger than the average distance between the charged surface and the conducting substrate, the magnitude of the electrostatic forces of adhesion can be expressed as ${F}_{E}=-\frac{{a}^{2}{A}_{c}}{2{\varepsilon}_{0}}$, and the total adhesion can be written as,
where W_{Ac} represents a non-electrostatic (i.e., surface-energy based) adhesion contribution. Estimates in the literature indicate that contact charging can produce surface charge densities ranging from 0.5 to 5 mC/m^{2} depending on the materials involved [170].
5.1.2.2. Van der Waals Adhesiveness (F_{vdW} )
The non-electrostatic component (F_{ne}) can be understood as the sum of vdW and capillary forces. In vacuum, capillary forces are neglected. Thus, if the measurement is made in a ‘dry’ atmosphere, such as nitrogen or vacuum, the adhesion force, F_{adh}, is due mainly to dispersion forces and may be explained with adhesion mechanics. For deformable bodies, the vdW adhesion force between two fine smooth spheres displaying ideal Hertzian elastic behavior was solved in the 1970s. Much of the present understanding of the elastic adhesion mechanics (adhesion and deformation) of spheres on planar substrates is based on the theoretical work of Johnson, Kendall and Roberts (JKR) (1971) [171] and of Derjaguin, Muller and Toporov (DMT) (1975) [172]. For a heterogeneous sphere/flat system, within the Derjaguin approximation one can write:
where ϖ_{ij} is the work of adhesion between two surfaces i and j in a medium k. The concept of measuring the strength of adhesion in terms of the work of adhesion, ϖ_{ikj}, was first introduced by Harkins in 1928 [173]. From the JKR theory, separation will occur when the contact area between the surfaces is a_{adh} = 63a_{0}, where a_{0} is the contact area at zero applied load. This separation occurs for a pull-off force of:
The JKR model should describe appropriately adhesion for larger spheres with high surface energies and low Young’s moduli, while the DMT model should be appropriate for describing adhesion of smaller spheres of low surface energies and higher Young’s moduli.
If there is plastic or elasto-plastic deformation neither the DMT nor JKR models hold. Instead, the Maugis and Pollock (M–P) analysis [174] can be used, at least for full plasticity. The MP analysis gives the pull-off force as [146]:
where H is the hardness of the yielding material and K is the effective elastic constant of the system given by: $K=\frac{4}{3}{\left(\frac{1-{\nu}_{s}^{2}}{{E}_{s}}+\frac{1-{\nu}_{t}^{2}}{{E}_{t}}\right)}^{-1}$ (ν_{s}, E_{s}, ν_{t}, and Et, are the Poisson’s ratio and the Young’s moduli of surface and tip, respectively). The reduced Young’s modulus is ${E}_{o}=\frac{1}{K}$.
For ideally smooth surfaces the theoretically predicted F^{DMT}_{adh} and F ^{JKR}_{adh} represent the lower and the upper limits of the experimentally measured F_{adh}, respectively. Hence, one can write [175]:
where α_{adh} (adhesiveness parameter) lies between $\left(\frac{3}{2}\right)\pi $ (for soft surfaces) and 2π (for hard surfaces). The two models differ substantially in predicted contact area, adhesion force and surface profile. JKR theory predicts a finite radius of contact under zero load and when surfaces separate: ${a}_{o(JKR)}={\left(\frac{6\pi {\varpi}_{ikj}{R}^{2}}{K}\right)}^{1/3}$ and ${a}_{s(JKR)}=\frac{{a}_{o}}{{4}^{1/3}}\approx 0.63{a}_{o}$, respectively. One can estimate the number of molecular contacts in adhesive interactions by dividing the contact area at pull-off, a_{s}_{(}_{JKR}_{)}, by the area occupied by a single functional group [176]. Corresponding quantities for DMT theory are ${a}_{o(DMT)}={\left(\frac{2\pi {\varpi}_{ikj}{R}^{2}}{K}\right)}^{1/3}$ and a_{s(DMT)} = 0. The estimate of the number of molecular contacts in the DMT model must consider the range of intermolecular of forces z_{o} (equilibrium size of the atoms at contact).
A self-consistent approach to the contact problem typically requires numerical solutions. Such calculations based on the Lennard-Jones potential showed that the DMT and JKR results correspond to the opposite ends of a spectrum of a non-dimensional parameter (so-called Tabor elasticity parameter) [177]: ${\mu}_{T}=2.92{\left(\frac{{\varpi}^{2}R}{{K}^{2}{z}_{0}^{3}}\right)}^{1/3}$.
Tabor suggested that when μ exceeds unity, the JKR theory is applicable (μ_{T} > 1); otherwise the DMT model should be used (μ_{T} < 1). A description of the transition between these limits (μ_{T} ≈ 1) was provided by Müller et al. [178], Maugis [179] and Johnson and Greenwood [180]. Xu et al. [181] suggested a modified Tabor parameter for the JKR-DMT transition in the presence of a liquid meniscus, as did Fogden and White [182], who introduced a parameter to include the Kelvin radius for the JKR–DMT transition. This topic was also addressed by Maugis and Gauthiermanuel [183] who included capillary effects within the framework that Maugis had previously established. The Maugis-Dugdale (M-D) theory can be expressed mainly in terms of dimensionless parameters, such as an elasticity parameter, λ, related to μ_{T} by:
Using this theory, Johnson [184] constructed an adhesion map with co-ordinates μ and F̄, where F̄ is the reduced load given by:
Significant adhesion has been encountered in nanotribology where the contact size may be measured in nanometers. Most practical applications fall in the JKR zone of the map, but a small radius of an AFM tip, for example, leads to operating values of λ which are in the Maugis-Dugdale transition zone. For AFM systems Carpick et al. reported λ ≅ 0.8 [185] while Lantz et al. [186] found λ ≅ 0.2→0.3. Upon inserting appropriate estimates for ϖ, K, and R in Equation 5.33, an approximate choice between Equations 5.28 and 5.30 can be made. Carpick et al. [187] presented a conversion table between λ and associated values of F̄, which can be estimated using an empirical equation [187]:
Using Equations 5.33 and 5.34, one obtains empirical values for the adhesion force. For λ values in the literature the expression of the adhesion force is approximately:
Shi et al. [188] showed a comparison of the three models, viz. JKR, DMT and M–D and the influence of the dimensionless load parameter. Both the dimensionless load parameter, F̄, and the transition parameter affect the contact area at micro/nano-scale and should not be ignored in nano-indentation tests. Patrick et al. [189] also demonstrated the accuracy of the three models using molecular dynamics simulations. These simulations, experimentally verified by Lantz et al. [186], indicate that an exact determination of the work of adhesion, ϖ_{ijk}, only from force–distance curves, is impossible (for determination of work of adhesion see section V-3). For the slope of the contact line and the jump-off-contact depend on each other in a way described by the parameter λ, but in order to calculate λ both ϖ_{ijk} and K must be known. When the surfaces are rough, the M-D model (Equation 5.35) is no longer valid, the vdW adhesiveness between a spherical particle and a rough substrate can be calculated with the Rumpf formula [190]:
where A is the Hamaker constant and D_{o} is the “cut off” distance, which represents the effective separation between two surfaces or particles in contact (interatomic spacing).The first term in the brackets stands for the interaction between the particle with radius R and the semispherical asperity with radius r_{a}. The second term represents the “noncontact” force between the particle and the flat surface with a separation r + D_{o} ≈ r.
The asperity on surfaces is not hemispherical. Rabinovich et al. [190] suggested an approximation for this case, using root-mean-square (rms) roughness and the peak-to-peak distance, which can be measured with an AFM. Within such approximation, the adhesion force is:
where the separation distance between the particle and the flat substrate is approximated by z_{max} = 1.817 rms. The other terms are defined as in Equation 5.36. Unfortunately, the rms values depend on the scanned areas, and bring additional difficulties for estimating the force. The model described the decrease in adhesion for increasing roughness on titanium deposited on silicon wafers [191] and served to analyze adhesion force of glass and lactose particles from rough surfaces, e.g., polycarbonate and acrylonitrile-butadiene-styrene [192]. Zhou et al. [193] studied the influence from electrostatic interactions and roughness of particles and substrates on adhesion. They concluded that the vdW adhesion forces can be drastically reduced if two conditions are fulfilled: (i) the surface must be appropriately rough and (ii) the peak-to-peak distance between rough spots must be in the right proportion to minimize the density between the two adhering partners. This topic was also investigated by other research groups [81,194–196].
The measured adhesion force for two rough surfaces in contact may also be expressed as [196]:
where n denotes the number of asperity contacts and α_{int} is the intrinsic adhesiveness, defined as the adhesion force for a unit effective surface area [196]. This equation provides the explanation for the high variability of AFM adhesion results. Schaefer et al. [197,198] showed that surface-particle adhesion with the colloid probe technique was much lower than expected for a simple sphere-plate geometry, which was attributed to the roughness of the contacting surfaces. Other roughness models for particle adhesion have been studied, where rough surfaces and interactions were modeled with fractals, boundary element technique, semi-empirical models, and using fast Fourier transform algorithms [199–210].
5.1.3. Work of Adhesion and Surface Energy
5.1.3.1. Wettability
Wetting is the ability of a liquid to maintain contact with a solid surface resulting from intermolecular interactions when the two are brought together. The degree of wetting (wettability) is determined by a force balance between adhesive and cohesive forces [23]. Adhesive forces between a liquid and solid cause a liquid drop to spread across the surface. Cohesive forces within the liquid cause the drop to ball up and avoid contact with the surface. If a liquid is forced to cover a substrate, which it does not wet, under equilibrium conditions it will break up and form drops. This phenomenon is called dewetting [211]. Dewetting is driven by the balance of capillary forces acting at the three phase contact line (substrate, liquid and air), as shown in Figure 10. The balance between the liquid–air, liquid–substrate, and substrate–air interfacial tensions determines this capillary force, being related to the contact angle. If the interfacial tension between the solid and the liquid is higher than the surface energy of the solid, dewetting will happen because it is energetically more favorable to remove the liquid from the substrate than to keep it spread on the substrate [211]. The position of the triple interface will change in response to the horizontal components of the interfacial tensions acting on it. At equilibrium these tensions will be in balance and one obtains the so-called Young Equation [212]:
Although Equation 5.39 describes the equilibrium contact angle in terms of the interfacial tensions involved, it gives no real insight into the reason why a certain value of contact angle is reached. Some surfaces have very high contact angles for water, while for others it is negligible. As already mentioned, an understanding of the origin of contact angle requires knowledge of the balance of forces between molecules in the liquid drop (cohesive forces), and those between the liquid molecules and the surface (adhesive forces). A surface with primarily polar groups, such as hydroxyl groups, will have a good affinity for water and, therefore, strong adhesive forces and a low contact angle (hydrophilic surfaces). If the surface is made up of non-polar groups, which is common for polymer surfaces or surfaces covered by an organic layer, the surface is hydrophobic, and the contact angle will be large. Wetting is determined by the equilibrium contact angle, θ. If θ < 90°, the liquid is said to wet the surface; if θ = 0° there is complete or perfect wetting and if θ > 90°, the liquid does not wet the surface. Contact angles of 180° are not found, as there are always interactions between the liquid and the solid.
5.1.3.2. Work of Adhesion
If two phases (i and j) in contact are pulled apart inside a third phase k, the original interface is destroyed and two new interfaces are formed (see Figure 10b).The work energy per unit area in performing this operation is called the work of adhesion, ϖ. There is a contribution from each interface removed from or added to the system:
If, instead of two distinct phases, a column of single liquid is pulled apart, the work of cohesion is:
where γ_{ik} is the surface tension and ϖ_{iki} is the free energy of cohesion in vacuum. Thus, the work of adhesion is the energy to create two new surfaces from one interface (Equation 5.40), while the work of cohesion is the energy to create two new surfaces (Equation 5.41). Surface tension (or surface free energy per unit area) of a liquid or solid is defined as half of the free energy change due to cohesion of the material in vacuum [213,214]. When one of the phases is a solid, the expression for the work of adhesion (Equation 5.40) can be combined with the equation for the contact angle (Equation 5.39):
This is commonly known as the equation of Young-Dupré [212,215]. Its significance is that it relates the work of adhesion to the really measured quantities γ_{ik} and θ, rather than to the inaccessible interfacial tensions involving the solid surface. A common approach to treating solid surface energies is that of expressing any surface tension (usually against air) as the sum of components due to dispersion forces (γ^{d}) and polar (e.g., hydrogen bonding) forces (γ^{p}) [216]. Thus, the interfacial tension between two phases i and j is expressed in terms of the two components for each phase:
Four cases arise in describing the work of adhesion:
unequal surfaces i and j in contact in vapor (V)
${\varpi}_{iVj}=2\left(\sqrt{{\gamma}_{i}^{d}{\gamma}_{j}^{d}}+\sqrt{{\gamma}_{i}^{p}{\gamma}_{j}^{p}}\right)$equal surfaces i and j in contact in vapor
${\varpi}_{iVi}=2\left({\gamma}_{iV}^{d}+{\gamma}_{iV}^{p}\right)$unequal surfaces i and j in contact with a liquid (L) or immersed solids [217]
${\varpi}_{iLj}=2\left\{\left({\gamma}_{L}^{d}+{\gamma}_{L}^{p}\right)-\left[\sqrt{{\gamma}_{i}^{d}{\gamma}_{L}^{d}}+\sqrt{{\gamma}_{i}^{p}{\gamma}_{L}^{p}}\right]-\left[\sqrt{{\gamma}_{j}^{d}{\gamma}_{L}^{d}}+\sqrt{{\gamma}_{j}^{p}{\gamma}_{L}^{p}}\right]+\left[\sqrt{{\gamma}_{i}^{d}{\gamma}_{j}^{d}}+\sqrt{{\gamma}_{i}^{p}{\gamma}_{j}^{p}}\right]\right\}$equal surfaces i and i in contact under a liquid
${\varpi}_{iLi}=2\left\{\left({\gamma}_{L}^{d}+{\gamma}_{L}^{p}\right)-2\left[\sqrt{{\gamma}_{i}^{d}{\gamma}_{L}^{d}}+\sqrt{{\gamma}_{i}^{p}{\gamma}_{l}^{p}}\right]+\left[\sqrt{{\gamma}_{i}^{d}{\gamma}_{i}^{d}}+\sqrt{{\gamma}_{i}^{p}{\gamma}_{i}^{p}}\right]\right\}$
The cross-dispersion as well as the cross-polar interactions are more appropriately expressed using harmonic rather than geometric means [218], so that:
The so called polarity matching $\left(\frac{{\gamma}_{S}^{p}}{{\gamma}_{S}^{d}}=\frac{{\gamma}_{L}^{p}}{{\gamma}_{L}^{d}}\right)$ states that optimum adhesives for non-polar materials are non-polar while those for polar materials are polar (Bruyne’s rule).The adherent surface may be characterized, i.e., given values of γ_{S}^{d} and γ_{S}^{p}, by using a pair of probe liquids, each with known γ_{L}^{d} and γ_{L}^{p} values, which are tabulated or may be determined from interfacial tension measurements against polar liquids. The work of adhesion of these probe liquids against the solid is measured from their contact angles against the solid and their surface tensions [218]:
providing two equations for the variables γ_{S}^{d} and γ_{S}^{p}. The polarity matching principle has achieved some measure of qualitative success in estimating contact adhesion.
5.1.3.3. Surface Tension
The total surface tensions of liquids are easily determined by a variety of methods [219–222] or can in many cases be found in published tables [23,223]. In an attempt to relate components to the chemical nature of the phase, van Oss et al. [224] suggested that the polar component could be better described in terms of acid-base interactions. Thus, an interfacial tension can be expressed as γ=γ^{LW} γ^{AB}, where LW and AB are Lifshitz-vdW and acid-base interactions. Unlike γ^{LW}, the polar London-vdW component, the acid-base component γ^{AB} comprises two non-additive parameters. These acid-base interactions are complementary in nature and are the electron-acceptor surface tension parameter (γ+) and the electron-donor surface tension parameter (γ^{−}). The total interfacial between two phases is [225]:
For LW interactions, the free energies of interaction between two identical or different materials, in vacuum or immersed in a liquid, can be directly obtained from surface tensions of the materials. If one wishes to characterize the wetting behavior of a particular liquid-solid pair, one needs only to obtain the contact angle θ for three liquids (two of which must be polar) with known γ_{L}^{LW}, γ_{L}^{+}, and values γ_{L}^{−}, and then use Equation 5.52 [226].
Another approach includes the Owens-Wendt theory [227], in which it is assumed that the polar and non-polar components of surface energy can be combined as a geometric average: ${\gamma}_{L}(1+\text{cos}\theta )=2\left(\sqrt{{\gamma}_{s}^{d}{\gamma}_{L}^{d}}+\sqrt{{\gamma}_{s}^{p}{\gamma}_{L}^{p}}\right)$. Dividing this relationship by $2\sqrt{{\gamma}_{L}^{d}}$:
Hence, a graph of $\frac{{\gamma}_{L}(1+\text{cos}\hspace{0.17em}\theta )}{2\sqrt{{\gamma}_{L}^{d}}}$ versus $\sqrt{{\gamma}_{L}^{p}/{\gamma}_{L}^{d}}$ leads to a straight line with intercept $\sqrt{{\gamma}_{s}^{d}}$ and angular coefficient equal to $\sqrt{{\gamma}_{s}^{p}}$, which is the surface energy of the material.
The surface energy between two surfaces can also be determined from the intermolecular forces. The pairwise summation of energies between all the atoms of one medium with all the atoms of the other medium, for vdW forces, leads to the interaction energy between two identical media as $\varpi =-\frac{A}{12\pi {D}^{2}}$ (see Table 3). Had the summation been carried out between all atoms, including atoms in the same medium, one should obtain two additional energy terms: $\varpi =-C+\frac{A}{12\pi {D}^{2}}$, where the constant is simply the bulk cohesive energy [21]. The positive term arises from the unsaturated bonds at the two surfaces. This term is always positive, indicating that a free liquid tends to minimize surface energy by minimizing its surface area [21]. Thus, besides the bulk energy, the total energy of two planar surfaces at a distance D is given by $\varpi =\frac{A}{12\pi {D}_{o}^{2}}\left(1-\frac{{D}_{o}^{2}}{{D}^{2}}\right)$ per unit area. At D = D_{o} (two surfaces in contact), ϖ = 0, while for D = ∞ (two isolated surfaces), $\varpi =\frac{A}{12\pi {D}_{o}^{2}}=2\gamma $ or:
In other words, the surface energy γ equals half the energy needed to separate two flat surfaces from contact to infinity, viz. it is half the adhesion energy. To use Equation 5.52 for calculating surface energies a “cut off” distance D_{0} should be found, which represents the effective separation between two surfaces or particles in contact. D_{0} is substantially less than the interatomic or intermolecular center-to-center distance r (see Equation 5.10) [228]. In order to estimate the strength of interaction forces and energies, as in Table 1, a cut-off distance of D_{0} ≈ 0.165 nm is sometimes used for macroscopic surfaces, and D_{0} ≈ 0.3–0.4 nm for individual atoms or small molecules [43]. However, the use of molecular diameters, i.e., D_{0} = σ, does not give reasonable results in Equation 5.54. Instead, by considering that there should be nine neighbor molecules in a planar, closely-packed structure, a semi-empirical equation was developed for the cut-distance for D_{0} which is significantly lower than σ [229]:
Thus, one may now test Equations 5.52 and 5.53 as to how well they predict surface energies determined with AFM or contact angle measurements. Equations 5.52 and 5.53 are not applicable only for highly polar H-bonding liquids such as formamide, glycerol, and glycol, for which the surface energies are underestimated. These equations are reliable for liquids interacting only with dispersion forces to within ±20% [229]. The equations cited previously do not describe the effect of surface topography and treatment on the surface energy or contact angle, although these parameters are greatly affected by the roughness of the solid surfaces [163,230,231].
Another method for measuring surface energy is to AFM and the mechanics of the contacts (JKR and DMT). The difference between JKR and DMT models lies in assuming the nature of forces acting between particle and substrate. Both models describe the correlation between pull-off force (F_{pull–off}) and work of adhesion (ϖ) through a simple analytical equation (Equation 5.31). Thus, equaling Equation 5.31 with Equation 5.39 [232,233]one obtain:
where α_{adh} = 2 in the DMT model and α_{adh} = 1.5 in the JKR model. Thus, knowing which mechanical model applies to a particular system under study, and setting operation conditions during AFM measurements that satisfy the particular model, γ_{ik} can be determined.
5.2. Interactions in Ambient Conditions
5.2.1. The Thin Water Film
If a liquid vapor is introduced in the system, the surface energy of the solids may be modified by adsorption. At a certain relative vapor pressure capillary condensation occurs at the point of contact between the tip and sample. An annulus of capillary condensate forms around the tip, yielding a capillary force that could be the main contribution in the measured pull-on and pull-off force. For measurements under ambient conditions in which a layer of adsorbed water is formed on the sample surface, two main nanoscale effects have to be considered: the disjoining pressure, Π, experienced by thin films, and in the case of non-flat interfaces the Laplace pressure (L), which determines the curvature of the adsorbed layer. The disjoining pressure is the interaction force per unit area between flat liquid/gas interfaces, and is induced by long-range interactions. For films of micrometer thickness, the disjoining pressure is negligible, but it must be considered for films in the range from 2 nm to 100 nm thick. Several forces contribute to the disjoining pressure, as follows [86]: Π(t) = Π_{disp.} + Π_{EDL} + Π_{ads} + Π_{HB} + Π_{st}, where Π_{disp} arises from the vdW or London dispersion forces, Π_{EDL} are the electrical double layer interaction forces, Π_{ads.} arises from the solute adsorption, Π_{HB} is due to hydrogen bonding and Π_{st} arises from steric forces.
For some systems, the vdW interaction dominates and the disjoining pressure for a film of thickness, t, can be written as:
Depending on the sign of the Hamaker constant, A_{SLV}, i.e., on the dielectric properties of the three media, the force responsible for the disjoining pressure can be attractive, repulsive or a mixture of both, as shown in Figure 11. Curve A is typical of a stable film (wetting), curve C corresponds to an unstable film (non-wetting), and curve B corresponds to a metastable film.
Another possible origin for the disjoining pressure is the so-called repulsive double layer force, which is relevant for charged surfaces or ionic solutions [23]. For an electrolyte solution, the disjoining pressure can be described by:
Where χ is the Debye screening length of ions in the solution and K_{s} is a constant factor related to the surface charge. In the case of pure water, the ions come mainly from the solid surface, their concentration being very low. DLVO theory includes the effects of both long-range forces, namely, the vdW and the double layer, for the disjoining pressure. Hence, the Π ( z) plot can take complicated shapes owing to the superposition of the two contributions, as illustrated in Figure 11. In effect, the disjoining pressure displaces the gas/liquid interface away from or towards the solid/liquid interface. This implies a change in the internal energy of the system and, as a consequence, a change in chemical potential of the liquid, which will change from zero to μ_{liq} = Π(t)/n_{1}. In order to keep the equilibrium between vapor and liquid phases, both chemical potentials must be equal: μ_{vapor} = kT ln (n_{ν}/n_{sat}) = −Π(t)/n_{l}. From these expressions, it is possible to obtain the film thickness for a given temperature and gas density.
Considering only the vdW contribution to the disjoining pressure and a hydrophilic substrate, the thickness of the water film can be approximated by:
where η is related to the Hamaker constant between water and the substrate and the density of water ρ by η = A_{sw} (6πρ), and p and p_{s} are the partial vapor pressure and saturated vapor pressure of water, i.e., relative vapor pressure [235].
As an AFM tip approaches the substrate, the capillary force on the tip is initially near zero until the tip contacts the surface of the water film. When contact is made, water is adsorbed around the tip to form a meniscus bridge between the tip and the substrate. Therefore, the force curve (pull-on force) depends directly on the height of the water film adsorbed on the substrate. The minimum thickness required for the water to spread [236] is:
where a_{m} is a molecular length given by a_{m} = A/6πγ_{SV} [237], ζ is the spreading coefficient given by ς = γ_{SV} − γ_{SL} − γ_{LV}, and γ_{sv} is the solid-vacuum interfacial energy. The formation of the capillary neck requires a minimum height of the water film. No capillary neck forms between two surfaces until the water film thickness reaches the minimum thickness, s. Clearly, if ς is negative then γ_{SV} < γ_{SL} < γ_{LV}, and the liquid will not spread on the substrate but will form a finite contact angle θ_{c} given by Young’s equation [212]: γ_{SV} = γ_{SL} + γ_{LV}, cosθ_{c}. To calculate θ_{c}, using the Hamaker constant, one can use the Hough–White equation (valid only for alkanes with carbon number above 10) [87]:
Techniques used to analyze water films on surfaces include ellipsometry [238], the surface force apparatus [239] and atomic force microscopy [240–243]. Forcada et al. [244] measured the thicknesses of solid-supported thin lubricant films using AFM, where the differences between the thicknesses measured with the force microscope and ellipsometric thicknesses were explained by the appearance of an instability in the liquid film. The theoretical description also predicts the dependence of these differences on the film thickness.
In our group, measurements of water layer thickness were carried out on mica, silica and silicon substrates. Figure 12a shows the thickness of the liquid film determined by AFM and the influence of the type of substrate. Figure 12b shows a force curve enlarged in the attractive region (approach curve) identifying the jump-to-contact distance (Djct). The thickness of the liquid film is determined by Djtc values in the force curve (relative humidity, RH, ≈ 70%), since in “dryer” conditions (RH ≈ 36%) this distance decreases to D_{itc}^{vdw}, which is directly related to vdW forces (D_{jtc} = 2.1 nm). The theoretical value using Equation 5.16 is 1.4 nm for dry conditions.
5.2.2. Attractive Interactions (vdW) (Pull-On Forces)
In 1969, Tabor and Winterton [47] measured the attractive vdW force-law (with SFA) between two glass or mica surfaces down to surface separations of D = 1.5 nm, and confirmed the Lifshitz theory of vdW forces. In 2003, Götzinger and Peukert [96] measured dispersive forces of particle-surface interactions by AFM and observed this force in the jump-in plot about 12 nm above the surface. In silicon surfaces, the vdW forces were approximately 4.5 nN in air and 0.7 nN in water. The vdW force between the surfaces (sphere-flat surface) covered by an adsorbed liquid film is given by (see Figure 4) [103]:
where t_{i} and t_{j} are the thickness of the water film adsorbed on surfaces i and j, whose values may be obtained with Equation 5.59.
At small separations, when $D\langle \langle (t+{t}^{\prime}),\hspace{0.17em}F{(D)}_{sphere-plane}=-\frac{{A}_{{jkj}^{\prime}}R}{6{D}^{2}}$, while at large separations, when $D\rangle \rangle (t+{t}^{\prime}),\hspace{0.17em}F{(D)}_{sphere-plane}=-\frac{{A}_{ikj}R}{6{D}^{2}}$. Thus, the vdW interactions are dominated by the properties of the bulk or substrate materials at large separations and by the properties of the adsorbed layers at separations less than the thickness of the layers. This means that the adhesion energies are largely determined by the properties of any adsorbed films even when these are only one monolayer thick [23].
5.2.3. Adhesion Forces (Pull-Off Forces)
5.2.3.1. Capillary Forces
The formation and disappearance of liquid bridges between two surfaces can occur either through equilibrium or nonequilibrium processes. In the first case, the bridge molecules are in thermodynamic equilibrium with the surrounding vapor medium. In the second, chemical potential gradients result in material transfer [245]. Figure 13 illustrates some of the important concepts associated with the formation and disappearance of liquid bridges. The equilibrium states depicted in Figure 13A,B are uniquely determined by the Kelvin length (2r_{k} cosθ). However, thermodynamics alone does not tell us how long it will take for transitions to occur between two equilibrium states. Such transitions typically occur by means of nonequilibrium processes involving material transfer. In the limit of very rapid processes, mechanical instabilities may occur at constant liquid volume, as depicted in Figure 13C–E.
At equilibrium, the meniscus curvature is related to the relative vapor pressure (relative humidity for water), p/p_{s}, by the well-known Kelvin equation [246]:
where r_{k} is the Kelvin radius, R is the gas constant, T is the temperature, r_{1} and r_{2} are the radius of the droplets, p is the actual vapor pressure, p_{s} is the saturated vapor pressure, and ν_{m} is the molar volume for water at 20 °C. Thus, for the spherical concave water meniscus in Figure 14, putting r_{1} = r_{2} = r_{m}, r_{m} = ∞ at p/p_{s} = 1 and rm ≈ −0.5 nm r_{m} ≈ −0.5nm at p/p_{s} = 0.1 (10% relative humidity).
A consequence of the dependence of vapor pressure on curvature is the phenomenon of capillary condensation [247]. To investigate the effect of a liquid condensate on the adhesion force between a surface and a macroscopic sphere (SFA) or AFM tip (nanoscale), we consider here that the surfaces are smooth and non-porous (sphere and flat plate). The surfaces are surrounded by vapor, which is in chemical and thermal equilibrium with the liquid bridge. The volume of the condensation is expected to depend strongly on the relative vapor pressure, the distance between the surfaces as well as on the three-phase contact angle [248]. The contribution of capillary forces to the total interaction between an AFM tip and sample increases above a certain critical humidity [249]. Moreover, the adhesion force depends strongly on whether the substrate is hydrophilic or hydrophobic [250,251]. Hartholt et al. [252] reported a decreased mobility of glass particles when relative humidity increased from 45% to ca. 65%. For humidity above 65%, the particles became immobile, indicating increased capillary forces. Xu et al. [13] obtained a flat response in force at relative humidity less than 20%. The reason for adhesion after reaching the critical humidity is the capillary force due to the liquid meniscus formed near the contact area (see Figure 14).
The resulting capillary force between a plate and a sphere with radius R was calculated by O’Brien and Hermann [253] as:
For two identical materials, θ_{1} = θ_{2}, thus
Equation 5.65 is useful for estimating the capillary force of a micro-contact; note that it is described as dependent only on the surface tension of bulk water, γ_{lv}, and the contact angle, θ, but is independent of the solid–solid and solid–liquid interaction parameters. This equation does not explain the force transition experimentally observed in several papers as a function of the relative humidity. Miranda et al. [254] discovered by scanning polarization microscopy that the force instability was caused by a low coverage of water at the solid surface. The authors suggested that water, condensed from water vapor at room temperature on mica, forms a partially developed monolayer of an ice-like phase. They concluded that with decreasing humidity the ice-like water monolayer, which is formed around 90% RH, breaks into islands, until the water coverage is too low (20% RH).
When the relative humidity is less than 90%, both the water film thickness and the radius of the meniscus bridge are less than 10 nm [255], which is much smaller than the radius of the AFM tips used in many studies. In this case, the capillary force can be well described by:
or for different contact angles:
where D is the distance between the tip and the substrate, d is the distance the tip extends into the water bridge and can be calculated by d = −1.08 cosθ/ln(RH) [256], where RH is the relative humidity. Generally, it is assumed that D/d is small and Equation 5.67 is reduced to Equation 5.65.
5.2.3.2. Chemical Forces
The decrease in adhesive force during descending with increasing humidity can be understood as a superposition of physical and chemical phenomena (microscopic origin) [257]. The adhesive force on the tip is the sum of the capillary force and the interaction force between the two solid surfaces mediated by the water in the gaps between the contacting rough points. The solid-solid interaction is more complex than the capillary force. It may contain vdW forces, electrostatic forces, and chemical bonding. The presence of water in the gap can greatly change the nature of the interaction. Since the liquid water is at equilibrium with the water vapor, the chemical potential of the liquid in the gaps around the contacting asperities is [250]:
From thermodynamics, the component of the chemical attractive force acting on the tip from the liquid in the gaps is given by [29,250]:
where G is the Gibb’s free energy, a_{L} is the area of the liquid film, and ϑ is the molar volume. Therefore, the force from water in the gaps becomes less attractive, i.e., more repulsive, with higher relative humidity.
Xu et al. [13] employed AFM adhesion measurements on mica surfaces to show that adhesion varies with humidity, which was confirmed with hydrophilic AFM tips on mica [251,258]. Pull-off force measurements with hydrophilic tips and hydrophobic substrates (coated silicon), or hydrophobic tip and hydrophilic substrates, are independent of relative humidity [236,259]. However, the force instability originates from the ability or inability of the water film to form a liquid joining the neck between the adjacent surfaces at high and low RH, respectively [29]. The decrease of the pull-off forces in high relative humidity for a hydrophilic tip was discussed by Binggeli and Mate [250,260]. The influence from varying air humidity on the pull-off force was also studied for particle-surface, particle-particle or surface-surface adhesion [164,261–266].
5.2.3.3. Electric Forces
Burnham et al. [94] studied another type of Coulomb-like force which ascends from the patch charges distribution on the tip and sample, i.e., from regions of different surface charge density interacting through a long range force law. Consider a spherical tip and a flat sample, each one with its own initial surface charge, and each one with an image charge due to the presence of the other charged body, then the electric force is [29,94]:
in which Q_{t} represents an image charge associated with the tip, D is the tip–sample distance, B is the position of Q_{t} within the tip, Q_{s} represents an image charge on the sample surface, r_{c} is the effective radius of curvature of the tip and Z is the position of Q_{s}. The relative permittivities ɛ_{1}, ɛ_{2} and ɛ_{3} correspond to the tip, sample and intervening medium, respectively.
The force is then independent of D, so that the patch charge effect is not noticed and vdW forces prevail. An AFM with an extremely curved tip retains the sensitivity to D. Recent extensions have led to methods to study surface-electrical variables: Kelvin Force Probe Microscopy, Scanning Capacitance Microscopy and Charge Detection Microscopy [29,267–271]. Once the tip and sample are exposed to air for quite a long time, no net charges are expected to persist and the electrostatic force is zero; nevertheless, capillary forces are present [29]. Through the control of the cleanliness of the surfaces (UHV environment), the adhesion due to vdW forces must become the principal attractive force amid uncharged, non-magnetic surfaces. In a solution, other forces related with double-layer, hydration and hydrophobicity need to be considered.
5.6.4. Total Adhesion Forces
The total pull-off force measured in air by force spectroscopy or adhesion force between the AFM tip and flat inorganic surfaces is given by:
In the absence of electrostatic charges:
where the term $\frac{{(1+\text{cos}\hspace{0.17em}\varphi )}^{2}}{\text{cos}\hspace{0.17em}\varphi}$ is applicable only to small contacts or small asperity contacts [235], i.e., large ϕ values (see Figure 13).
5.3. Interactions in Solution
5.3.1. Screened vdW Forces in Electrolyte Solutions
Situations in which vdW forces alone determine the total interaction are restricted to a few simple systems, e.g., to interactions in a vacuum or to non-polar wetting films on surfaces, both already discussed in previous sections. In more complex systems long-range electrostatic forces are also involved, and the interplay between these two interactions has many consequences. For instance, clay particles and silt carried by rivers coagulate upon coming across the high salt concentration of the sea to form extensive deltas [272]. Electrostatic forces are also crucial in the behavior of biological systems [273], swelling of lipid bilayers in water [274,275], the unexpected stability of lattices at high salt concentrations [276], etc.
In an earlier section, we mentioned that the zero-frequency contribution to the vdW force is essentially an electrostatic interaction. Now, in any medium containing free charges, e.g., water containing free ions in solution or a conducting polymer containing free electrons, all electrostatic fields are screened due to polarization of these charges. In particular, highly polar H-bonding liquids, e.g., water, are known to cause a considerable reduction (by factors of 10 or more) in the vdW forces with respect to those for the vacuum level [277]. The tip/sample combination in a liquid medium can result in a more isotropic polarizable system than does the same combination in air or vacuum, with a resulting substantial reduction of the vdW forces. Across an electrolyte solution, the screened non-retarded Hamaker constant A_{e} is given by [278]:
where κ is known as the Debye screening length and D is the distance between the surfaces. For example, in a 0.1 M aqueous NaCl solution the vdW screening length is ca. 0.5 nm, so that by D = 1 nm the zero-frequency contribution (A_{ν}_{=0}) has already fallen to about 10% of its value at D = 0. Thus, for inter-particle interactions across such a solution, at separations greater than 1 nm, the vdW interaction is effectively determined solely by the dispersion (A_{ν}_{>}_{0}).
Hence, vdW interactions (pull-on force) in solution for the geometry described for AFM can be modeled as:
This model indicates that vdW forces are reduced in salt solutions. However, as will be seen later, within the framework of the conventional DLVO colloid stability model, an increase in electrolyte concentration typically has more influence on the electrostatic interaction energy than on the vdW interaction energies, and results in increased attraction between two similar surfaces [279]. One concludes that solution chemistry can significantly affect interfacial forces between particles, even altering stability [277,280]. For example, when the muscovite mica is immersed in a polar liquid medium-like water, surface charges are induced on both the tip and the sample surface due to ionization, dissociation or spontaneous adsorption of charged species. To keep the electrical neutrality, opposite ionic species are held together closer to the tip/sample surface forming an electric doublelayer. When mica is placed in water, the mechanism of the double-layer formation is attributed to the K^{+} dissolution, as well as ionic exchange between K^{+} and H_{3}O^{+} (or H^{−}) [281]. The effects from ionic strength on the vdW interaction energy have been studied extensively [282–284]. Toikka et al. [285] showed that the double layer decreases the adhesion force, and that the apparent adhesion force depends on the pH of the solution. The authors confirmed the existence of this phenomenon by measuring adhesion forces in different pH solutions between an iron sample and a silica colloidal probe. Changes in vdW interactions as a function of electrolyte concentration can be attributed to screening of the non-dispersion portion of the Hamaker constant A_{ν}_{=0}, which was assumed not to be affected by electrolytes that cannot respond to high frequencies [278].
The fact that colloidal particles in liquid medium at high enough electrolyte concentration tend to form persistent aggregates through collisions caused by Brownian motion implies an interparticle attractive force (vdW force). In aqueous electrolyte solutions long-range electrical double layer forces also appear. The JKR theory of contact mechanics can serve as a reasonable basis for understanding adhesion forces (pull-off force or vdW adhesiveness) in an aqueous medium. Since it is based on energy balance, no adhesion is expected when the free energy of a double-layer per unit area w_{DL} balances the interfacial surface tension γ_{SL} Quantitatively, the pull-off force or adhesion force can be related to these two terms as follows [176]:
where P_{DL} ≈ 2πRw_{DL} is an additional load that has to be applied to a spherically shaped tip due to the presence of a double-layer and ω̄_{iki} is the free energy of cohesion in vacuum. Thus, repulsion between like-charged surfaces (P_{DL} > 0) will decrease the magnitude of the pull-off force compared to that given by the JKR theory.
5.3.2. The DLVO Theory: vdW and Double-Layer Forces Acting Together
The first theories for the stability of hydrophobic colloids by Hamaker [286] and de Boer [287] were based on a balance between vdW attraction and electrical double-layer (DL) repulsion. These theories were further elaborated by Derjaguin [288], Derjaguin and Landau [289] and, independently, by Verwey and Overbeek [290], leading to the theory now known as DLVO theory [291]. At low salt concentration, the double-layer repulsion is sufficiently strong to keep the colloidal particles apart. With increasing salt concentration the electrostatic repulsion is increasingly screened [8]. At a certain concentration, the vdW attraction overcomes the repulsive electrostatic barrier and coagulation sets in.
The earliest model of the electrical double layer is usually attributed to von Helmholtz [292,293] (Figure 15), who treated the double layer mathematically as a simple capacitor, based on a physical model in which a single layer of ions is adsorbed at the surface. However, the classical theory for the electrical double-layer is the Gouy-Chapman-Stern [294–296] model, which combines the Helmholtz adsorbed layer with the Gouy-Chapman diffuse layer. It was proposed by Gouy [294], Chapman [295], and Debye and Huckel [297] that if a charged interface exists in a polar solvent, then ions of opposite charge are attracted to that surface. Entropy ensures that the ions do not all adsorb at the surface and form a crystal in many cases, leaving the ions to exist as a diffuse layer close to the charged surface [298]. In the stern layer, counterions are strongly adsorbed and they lower the electrical potential at points adjacent to the particle surface.
The form of the interaction is well known to all colloid scientists and is roughly exponential, given by:
where D is the distance between the surfaces. The decay length is given by the inverse of the Debye-Huckel parameter, κ, and the intercept at zero separation is given by the surface potential, ψ_{o}. The Debye length falls with increasing ionic strength and valence of the ions in the solution.
An analytical expression for measurements in AFM has been provided by Butt [28] on the basis of an equation of Parsegian and Gingell [299]. For a spherical tip and a flat sample, the double-layer force is given by [8]:
where R_{t} is the tip radius, κ_{D} is the inverse of the Debye length, D is the distance between the surfaces, σ_{T} and σ_{S} are the surface charge densities of tip and sample, respectively, ɛ_{l} is the dielectric constant of the liquid, and ɛ_{0} is the permittivity of free space.
There are many approximate expressions for this interaction, some of which are in terms of the surface charge density σ. Others are related to the surface potential ψ_{o}, which is easier to measure, or take into account “charge-regulation” effects where neither the surface charge nor the potential remain constant during an interaction [300]. In aqueous solutions, since vdW and electrostatic forces usually occur together, it is common practice to plot the two forces when describing the net interaction of two surfaces. Figure 16 shows how these forces may determine whether an interaction will be attractive or repulsive at a given separation. The subtleties in the plots arise because the forces have different distance dependencies—the one being a power law, the other an exponential [43].
Hartley et al. [302] performed AFM measurements of vdW attraction between a silica sphere and a silica plate separated by 5–20 nm in aqueous solutions near the isoelectric pH 2.2–3.0 of silica. The measured forces were stronger than predicted by the non-retarded theory, which were attributed to weak electrostatic attraction. They also measured an attractive force between a silica sphere and a mica flat surface at pH 2.5, which was stronger than predicted for the vdW attraction, even including effects from retardation. Again, the discrepancy was attributed to a weak electrostatic attraction. Practically all of the measurements of vdW interactions mentioned above are for strong interactions experienced at separation distances of 20 nm or less where retardation effects are mild or unimportant. Interactions at larger separations tend to be severely retarded and much weaker. To measure accurately these weaker interactions, a different technique can be utilized. Bevan and Prieve [303] measured retarded vdW attraction with total internal reflection microscopy (TIRM) [304]. Teschke et al. [305] measured the force acting on the tip during its immersion in the double layer region for various tip-approaching velocities. Milling et al. [306] measured vdW repulsion between a gold sphere and a flat plate of poly(tetrafluoroethylene) separated by up to 20 nm of various liquids. The non-retarded Lifshitz theory was able to predict which interactions should be repulsive and that the force decays with the inverse square of the separation distance. A similar study was carried out by Lee and Sigmund [307], where the distance dependence of the measured forces between a flat Teflon AFTM foil and an α-alumina or amorphous silica sphere in cyclohexane agreed with the theoretically calculated forces, including the retardation contribution. Figure 17 shows that one can minimize vdW interactions by choosing a medium with dielectric constant and refractive index close to those of either the tip or the sample. Since both mica and Si_{3}N_{4} have rather high refractive indices (1.57 and 1.97, respectively) [307], few liquids meet these criteria.
Borato et al. [308] showed that water is aged upon exposure to air, which was confirmed with impedance spectroscopy measurements made with taste sensors containing bare metal electrodes. Figure 17b shows that the force curves can be affected by water ageing in the liquid cell. For short periods, the curve displays a minimum with the distance between the tip of silicon nitrite (ɛ_{tip} = 7.4) and a flat mica surface (ɛ_{mica} = 5.4) [309], which indicated the predominance of attractive vdW interactions. For longer times, repulsive double-layer forces are practically purely repulsive (for t″). This is due to ageing of the water, which is accompanied by a change to lower pH values, and this increases the charge of the silicon nitride tip (whose isoelectric point is pH 6.3) [281], whereas mica is negatively charged. The net result is an increase in the repulsive, double-layer force.
Figure 18 shows representative curves for three media, viz. 1-bromonaphthalene, 1-methylnaphthalene and ethanol. These curves indicate the tip deflection as the tip approaches the sample. The vdW interaction is strongly attractive for ethanol, as one would expect. The other liquids yield a repulsive interaction.
5.3.3. Non-DLVO Forces: vdW and Structural Forces Acting Together
Repulsive or attractive forces may also arise from structural forces referred to as solvation or hydration forces [279]. The continuum theories of vdW force and double-layer force cannot describe the mutual interaction of two surfaces approaching at distances below a few nanometers, because (i) they are not valid at small separations and (ii) other forces arise, which are named non-DLVO forces [224,310]. The latter can be roughly grouped into three categories: solvation forces, repulsive hydration forces and hydrophobic attractive forces. Derjaguin and Voropayeva [311] found an extra repulsive force between crossed platinum wires in aqueous solutions at high electrolyte concentrations. The stability of soap films [312] is an important example of a system where DLVO theory fails to explain the experimental observations of the thin film stability.
Solvation forces appear around particles suspended in an aqueous medium. This structured hydrogen-bonded network decays away from the surface. In most cases, these forces exhibit an oscillatory behavior, i.e., the liquid density profiles and interaction potentials in liquids oscillate with the distance, with a periodicity close to the molecular size and with a range of a few molecular diameters [98]. In this range, the molecules are ordered in layers. When two surfaces approach each other, layers after layers are squeezed out of the closing gap. Here, attractive interactions between the wall and liquid molecules and the geometric constraining effect of the “hard wall” on these molecules force them to order (or structure) into quasi-discrete layers, as shown in Figure 19. This layering is reflected in an oscillatory density profile extending several molecule diameters into the liquid, as also illustrated in Figure 19 [313]. Such forces were termed solvation forces because they are a consequence of the adsorption of solvent molecules onto solid surfaces [314].
For simple spherical molecules between two hard, smooth surfaces the solvation force is usually a decaying oscillatory function of the distance (D). The solvation force between a sphere and planar surface can be calculated within the Derjaguin’s approximation [315,316]:
where σ is the molecular diameter, λ_{S} is the decay length, D is the distance between the walls, ϕ is the phase shift and F_{o} is the measured force amplitude. Richetti et al. [317] suggested a similar equation to describe the interaction between two surfaces across a smectic liquid, studied with AFM [318].
There is another short-range force that cannot be accounted for by the DLVO theory, which is not oscillatory but smoothly varying, i.e., monotonic. This force is exponentially repulsive and is commonly referred to as the hydration or structural force (or solvation force in fluids other than water) [319–322]. Because of the correlation with the low (or negative) energy of wetting of the solids with water, the repulsive force has been attributed to the energy required to remove the water of hydration from the surface, or the surface adsorbed species (secondary hydration), presumably because of strong charge-dipole, dipole-dipole or H-bonding interactions [323,324]. The concept of hydration force emerged to explain measurements of forces between neutral lipid bilayer membranes [324]. Repulsive hydration forces appear to arise whenever water molecules strongly bind to surfaces containing hydrophilic groups, i.e., certain ionic, zwitterionic, or H-bonding groups. Hydrogen bonding commonly serves as the mechanistic basis of structural forces. Generally, for a solvated surface, solvent molecules highly restricted in their motion experience structural forces. When the solvent is water, this orientation restriction is referred to as hydration pressure [279]. Israelachvili [23] further explains that this effect is not limited to a primary hydration shell, but rather propagates radially towards the bulk solution into a secondary hydration shell. Hydration forces are relatively short-ranged so that at salt concentrations below 0.1 M they can easily be distinguished from the longer range electrostatic and vdW forces. In contrast to the electrostatic double-layer force, hydration forces tend to become stronger and longer ranged with increasing salt concentration, especially for divalent cations [8]. A large hydration force could have important implications for AFM imaging, because to probe the true surface of a macromolecule, the probe would have to break through the hydration “shell” [325]. If the required force is too large, the structure below the “shell” could be deformed, resulting in a lower resolution.
The hydration pressure decays with the distance, and therefore the repulsive hydration may be represented by an empirical exponential function [326]:
where the decay length λ_{H} is the range λ_{H} ≈ 0.6–1.1 nm for 1:1 electrolytes [327], w_{o} is the hydration force constant which depends on the hydration of the surfaces but it is usually below 3–30 mJ m^{−2}, and D is the distance between the surfaces.
Hydration forces have been suggested as responsible for the short-range repulsion observed between silica surfaces [328,329]. Equations 5.80 and 5.81 were used to fit the experimental short-range forces (that exponentially decay on the separation distance) between different surfaces: silica, mica, montmorillonite and lipid bilayers [274,330,331]:
where F(x) is the short-range force, D is the separation between the surfaces, and C_{H} is a hydration constant, assuming that the short-range force is due to hydration forces. Equations 5.80 and 5.81 are empirical relations, which are not supported by any theory [332]. Valle-Delgado et al. [333] utilized these equations to estimate interaction forces between bovine serum albumin (BSA) layers adsorbed on different substrates (silica and polystyrene), as a function of pH and salt concentration. They observed that electrostatic and steric forces dominate the interactions at low salt concentrations; in contrast, at high salt concentrations an attractive interaction was observed, which was explained with hydration forces obtained with Equation 5.80. The same authors used this relation to estimate hydration forces in the interaction between apoferritin (protein) molecules adsorbed on silica surfaces [334] and between silica surfaces [332].
Paunov et al. [335] suggested that hydration forces in protein suspensions are due to the overlap of a layer of hydrated ions adsorbed on the surfaces. Figure 20 shows a schematic picture of this repulsive mechanism. The force between a plane and a sphere of radius R due to the overlap of the hydrated ions layers (Stern layers) is given, according to the model of Paunov et al. [335] by:
where υ_{W} is the volume occupied by a water molecule (υ_{w} ≈ 0.03 nm^{3}), ϕ_{s} is the volume fraction of hydrated ions in the Stern layer, and δ_{0} is the diameter of the hydrated ions.
In addition to the equations above, other models have been proposed to explain the hydration repulsion:
Water Structure Theory: in the water-structuring models, the short-range repulsive interaction is attributed to an alignment of water dipoles in the vicinity of a hydrophilic surface, where the range of the surface force is determined by the orientation-correlation length of the solvent molecules [336]. Other researchers also suggested that the origin of the hydration force between silica surfaces may be related to the structuring of water molecules at the silica-water interface [337–339]. It is known that water can form strong H-bonds with the silanol groups. Derjaguin suggested that next to the silica surface there might be a layer of structured water up to 900 Å thick [340]. Attard and Batchelor [341] suggested that due to the strong orientation of water molecules near polar surfaces, there are fewer configurations available to maintain the bulk water structure and this represents lost entropy, which leads to a repulsive force.
Image-charge model: the image-charge models take into account the discreteness of the surface charges, which induce orientation in the adjacent water dipoles [342].
Dielectric-saturation model: this model assigns the hydration repulsion to a layer with lower dielectric constant, ɛ, in the vicinity of the interfaces [343]. Henderson and Lozadacassau [344] suggested that since the water molecules at the surface are strongly oriented, there should be a region of smaller dielectric constant at the solvent substrate interface when compared to the bulk.
Excluded-volume model: it takes into account the finite size of the ions, leading to a lower counterion concentration near a charged surface, and to a weaker Debye screening of the electrostatic field, which results in a stronger repulsion between two charged surfaces at short separations [345].
Gel-like layer model: the presence of a porous gel-like layer on silica was proposed by Lyklema [346] to explain the high surface charge and low potentials of the silica surface. Theoretical calculations to account for the observed charging characteristics of oxides have indicated that the gel layer maybe ~2–6 nm thick. Vigil et al. [347] used this explanation in the analysis of their experiments using silica surfaces and SFA.
Layer of co-ions model: this relatively simple model [348] assumes that at sufficiently small thicknesses all co-ions are pressed out of the film so that it contains only counterions dissociated from the ionized surface groups. Under such conditions, the screening of the electric field of the film surface weakens, which considerably enhances the electrostatic repulsion in comparison with that predicted by DLVO theory. Such reduced screening of the electric field could exist only in a narrow range of film thicknesses, which practically coincides with the range where hydration is observed.
Experimentally, the magnitude of the hydration force could only be inferred because of the presence of other longer range forces [28]. However, owing to the lack of control over the shape of the AFM tip, it is difficult to establish a direct connection between hydration force and tip geometry [325]. For example, it is not clear how far the hydration force extends laterally and whether the surface beyond the very end of the tip could contribute substantially to the hydration force. The existence of a short range (≤4 nm) repulsive pressure was observed in experiments on the swelling of clays [349], on the stabilization on foam films [312,348], proteins [332,334,335] and interactions between phospholipid bilayers [274]. Pashley and Israelachvili observed at electrolytes concentrations below 10^{−4} M a typical DLVO maximum; however, at electrolyte concentrations higher than 10^{−3} M they did not observe the expected DLVO maximum and primary minimum [350,351]. When Israelachvili and Pashley measured the force between two mica surfaces in electrolytes, they found, in addition to the electrostatic and vdW force, a short-range repulsive force at higher salt concentrations [352]. The more hydrated cations such as Mg^{2+} and Ca^{2+} gave stronger repulsive forces than the less hydrated monovalent ions such as K^{+} and Cs^{+}. The authors concluded that the repulsive force was due to the work required to dehydrate the adsorbed ions on forcing the mica sheets together. Similar results were observed by Horn et al. [353], Butt [28] and Claesson et al. [354]. The magnitude of the hydration repulsion was found to decrease in the order Mg^{+} > Ca^{+} > Li^{+} ≈ Na^{+} > K^{+} > Cs^{+} > >> H_{3}O^{+} [135,355]. As a consequence, the conventional electrostatic (double layer) repulsion was suppressed if the solution’s ionic strength was increased; in contrast, the hydration repulsion was detected at higher ionic strengths. Further experimental evidence of hydration forces can be found in coagulation studies of silica sols [356–359]; lecithin bilayers [360]; glass fibers [337]; glass sphere [30], silica [338,361] and conducting polymers [8]. Additional information can be found in review articles [29,98,324].
Initial studies on mica surfaces with adsorbed surfactant molecules pointed to an attractive force that exceeded the calculated vdW attraction between the bare substrates. This force is termed hydrophobic, whose existence was confirmed by Christenson and Claesson [362] and Rabinovich and Derjaguin [363], who showed that the force range could be greatly enhanced by increasing the hydrophobicity of the surface. Hydrophobic attractive forces (that act between solvated molecules and nonpolar interfaces) between hydrophobic macroscopic bodies in water have been measured for different systems. Hydrophobic effects roughly fall in two classes, namely those that are influenced by the addition of salt and those that are not [364]. The origin of the force appears to depend on the type of surface [365], but is still not completely understood. Several hypotheses have been proposed as follows [135,366–370]: (1) The hydrophobic force could originate from changes of the water structure in the thin layer between hydrophobic surfaces compared to the structure of bulk water; (2) it could be the capillary force due to cavitation in the vicinity of hydrophobic surfaces [371,372], (3) it could arise from hydrodynamic fluctuations at a hydrophobic surface/water interface; (4) it could arise from correlated dipole-dipole or dipole-charge interactions (electrostatic phenomena) [373–375]; (5) it may result from dipole interactions associated with the large domains of ordered hydrocarbon chains or (6) it may arise from capillary bridging of nanobubbles attached on hydrophobic surfaces [376,377]. Hypothesis (6) is probably the most important to cause very long-range interaction.
A hydrophobic surface is one that is inert to water in the sense that it cannot bind to water molecules via ionic or hydrogen bonds. For surfaces having both the electron-donor and electron-acceptor values greater than that of water, the surface is termed hydrophobic. The orientation of water molecules in contact with other hydrophobic molecules is entropically unfavorable [378]. Therefore, such hydrophobic molecules will attract each other, since by coming together the entropically disfavor water is ejected into the bulk thereby reducing the total energy of the system [23,379]; see Figure 21a for further description. According to basic electrostatic principles, the domains of polarized water will establish long-range dipole-dipole interactions with each other. These interactions depend on the magnitude of the effective polarization fields Q⃗ (see Figure 21b) [380]. Thus, the origin is in the polarization field produced by the strong correlation and coupling of the water molecules dipoles at the surfaces. This polarization field has been shown to give rise to dipoles on the surface of hydrophobic solutes that generate long-range hydrophobic attractions, which is crucial for colloidal interactions [224]. The hydrophobic force has resisted quantitative experimental determination as well as theoretical definition until relatively recently [226].
The hydrophobic force between two macroscopic surfaces was found to be of surprisingly long-range, decaying exponentially with a characteristic decay length λ_{H} = 1–2 nm, and then more gradually farther out [363,381,382]. The hydrophobic force can be far stronger than the vdW attraction, especially between hydrocarbon surfaces for which the Hamaker constant is quite small [279]. Therefore, for two surfaces in water, their purely hydrophobic interaction energy, i.e., ignoring DLVO and oscillatory forces, in the range 0–10 nm is given by [383]:
where typically γ_{i} = 10–50 mJ m^{−2} [23].
The data are normally fitted by an empirical force law in the following form [384]:
where R is the tip radius, D is the tip-sample distance, and Γ is grafting density.
Rabinovich and Yoon [385] measured the hydrophobic force between a silica plate and a glass colloidal probe hydrophobized with octadecyltrichlorosilane (ODTCS). They obtained Γ by measuring the jump-to-contact of the curves, according to the following relationship:
in which the subscript “jtc” means that this value is obtained with the “jump” method and k_{c} is the elastic constant of the cantilever.
The effects from salt and chemical potential on adhesion between hydrophobic surfaces were investigated by Kokkoli and Zukoski [386], where they concluded that the adhesion is sensitive to surface roughness and lowering the solvent chemical potential produces an increase in the pull-off force. Freitas and Sharma [387] measured interactions between hydrophilic and hydrophobic surfaces in an aqueous medium at various pHs and ionic strengths as well as in some organic solvents using AFM. In hydrophilic systems the forces were well described by the DLVO theory at large separation distances. Long-range hydrophobic forces were not observed in hydrophilic-hydrophobic systems. However, the interaction between two hydrophobic surfaces (see Figure 22) was dominated by the long-range attraction due to hydrophobic forces [107]. Other experiments were carried out using AFM [388,389] and surface force apparatus (SFA) in the detection of hydrophobic forces [175,390].
6. Conclusions
This review was primarily aimed at theoretical models and direct measurements of vdW forces, particularly in the context of the use of atomic force spectroscopy (AFS). Because the molecular systems, for which vdW forces are so important, are affected by other interactions—especially H-bonding and electrostatic forces—we included in the review some discussion on other forces as well. This was important for understanding AFS measurements carried out in different media. In air, for instance, the formation of a thin water film and the capillary forces need to be addressed for a complete understanding of the whole system. For AFS measurements in liquid cells, on the other hand, the appearance of double-layer forces is essential, which is the reason why emphasis was placed on models for the double layers. All in all, we hope to have convinced the reader of the wide applicability of AFS, with potential impact in many areas of science and technology. The successful use of AFS however, requires identification and quantification of intermolecular forces, which is now becoming possible with the many physical models discussed in the review.
Acknowledgments
We gratefully acknowledge to FAPESP (2007/05089-9), CNPq (483303/2011-9), CAPES (02880/09-1) and nBioNet for the financial support. We also acknowledge the support from the University of São Paulo and Federal University of São Carlos and important insights provided by Adriano Moraes Amarante.
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Table 1. List of Hamaker constants in vacuum (air) and water for inorganic materials often used in experiments of force spectroscopy [23,87,93,98–100], as well as the Hamaker constants for some organic materials [101,102]. |
Material (1) | Material (2) | Medium (3) | Calculated × 10^{−20} J | Experimental × 10^{−20} J |
---|---|---|---|---|
Si_{3}N_{4} | Si_{3}N_{4} | Air 1 | 16.70 | - |
Si_{3}N_{4} | Si_{3}N_{4} | Water | 4.80–5.90 | 6.10 |
Si_{3}N_{4} | Mica | Water | 2.45 | 3.40 |
SiO_{2} | SiO_{2} | Air | 6.50 | - |
SiO_{2} | SiO_{2} | Water | 0.77–0.84 | 0.85–1.00 |
SiO_{2} | Air | Water | −1.00 | −1.00 |
SiO_{2} | Mica | Water | 1.20 | 1.20 |
SiO_{2} | PTFE | Vacuum | 16.44 | 13.70 |
Mica | Mica | Water | 2.00–2.20 | 2.20 |
Mica | Mica | Air | 9.86 | - |
Au | Au | Water | 40.00 | 25.00 |
Silicon | Silicon | Air | 18.65 | - |
Silicon | Silicon | Water | 9.75 | - |
MgO | MgO | Air | 12.10 | - |
MgO | MgO | Water | 2.21 | |
Teflon | Teflon | Air | 2.75 | - |
Teflon | Teflon | Water | 0.33 | |
Polystyrene | Polystyrene | Air | 6.58 | - |
Polystyrene | Polystyrene | Water | 0.95 | - |
Poly(isoprene) | Poly(isoprene) | Air | 5.99 | - |
Poly(isoprene) | Poly(isoprene) | Water | 0.743 | - |
Ag | Ag | Air | 20.00–49.00 | 38.50 |
C (diamondIIa) | C (diamondIIa) | Air | 29.60 | - |
Cellulose | Cellulose | Air | 5.80 ± 0.20 | - |
Cellulose | Cellulose | Water | 0.80 ± 0.05 | - |
Hexadecane | Hexadecane | Air | 5.20 | - |
Hexadecane | Hexadecane | Water | - | - |
Cellulose | CaCO_{3} | Air | 7.40 ± 0.30 | - |
Cellulose | CaCO_{3} | Water | 0.57 ± 0.10 | - |
Cellulose | Si_{3}N_{4} | Air | 9.50 ± 0.40 | - |
Cellulose | Si_{3}N_{4} | Water | 0.80 ± 0.20 | - |
Cellulose | SiO_{2} | Air | 5.90 ± 0.30 | - |
Cellulose | SiO_{2} | Water | 0.35 ± 0.03 | - |
Cellulose | Mica | Air | 7.20 ± 0.30 | - |
Cellulose | Mica | Water | 0.43 ± 0.08 | - |
Cellulose | TiO_{2} | Air | 9.30 ± 0.40 | - |
Cellulose | TiO_{2} | Water | 1.20 ± 0.20 | - |
Octane | TPFP | Air | 4.50 | - |
Octane | TPFP | Water | 29.00 | - |
Octane | AF 2400 | Air | 4.00 | - |
Octane | AF 2400 | Water | 31.00 | - |
Octane | AF 1600 | Air | 4.10 | - |
Octane | AF 1600 | Water | 32.00 | - |
Octane | PTFE. LD | Air | 4.60 | - |
Octane | PTFE. LD | Water | 40.00 | - |
Octane | PTFE. HD | Air | 5.10 | - |
Octane | PTFE. HD | Water | 42.00 | - |
Octane | PDMS (liq) | Air | 4.05 | - |
Octane | PDMS (liq) | Water | 38.00 | - |
Octane | PDMS (s) | Air | 4.50 | - |
Octane | PDMS (s) | Water | 40.00 | - |
Octane | PE. LD | Air | 4.90 | - |
Octane | PE. LD | Water | 43.00 | - |
Octane | Rubber | Air | 5.05 | - |
Octane | Rubber | Water | 50.00 | - |
P-Xylene | TPFP | Air | 3.40 | - |
P-Xylene | TPFP | Water | 22.00 | - |
P-Xylene | AF 2400 | Air | 4.00 | - |
P-Xylene | AF 2400 | Water | 27.00 | - |
P-Xylene | AF 1600 | Air | 4.10 | - |
P-Xylene | AF 1600 | Water | 30.00 | - |
P-Xylene | PTFE. LD | Air | 4.70 | - |
P-Xylene | PTFE. LD | Water | 31.00 | - |
P-Xylene | PTFE. HD | Air | 5.07 | - |
P-Xylene | PTFE. HD | Water | 34.00 | - |
P-Xylene | PDMS (liq) | Air | 4.10 | - |
P-Xylene | PDMS (liq) | Water | 42.00 | - |
P-Xylene | PDMS (s) | Air | 4.50 | - |
P-Xylene | PDMS (s) | Water | 45.00 | - |
P-Xylene | PE. LD | Air | 5.00 | - |
P-Xylene | PE. LD | Water | 51.00 | - |
P-Xylene | Rubber | Air | 5.30 | - |
P-Xylene | Rubber | Water | 60.00 | - |
D-α-Pinene | TPFP | Air | 4.00 | - |
D-α-Pinene | TPFP | Water | 21.00 | - |
D-α-Pinene | AF 2400 | Air | 4.40 | - |
D-α-Pinene | AF 2400 | Water | 30.00 | - |
D-α-Pinene | AF 1600 | Air | 4.50 | - |
D-α-Pinene | AF 1600 | Water | 32.00 | - |
D-α-Pinene | PTFE. LD | Air | 5.10 | - |
D-α-Pinene | PTFE. LD | Water | 41.00 | - |
D-α-Pinene | PTFE. HD | Air | 5.60 | - |
D-α-Pinene | PTFE. HD | Water | 51.00 | - |
D-α-Pinene | PDMS (liq) | Air | 4.50 | - |
D-α-Pinene | PDMS (liq) | Water | 40.00 | - |
D-α-Pinene | PDMS (s) | Air | 5.00 | - |
D-α-Pinene | PDMS (s) | Water | 48.00 | - |
D-α-Pinene | PE. LD | Air | 5.40 | - |
D-α-Pinene | PE. LD | Water | 59.00 | - |
D-α-Pinene | Rubber | Air | 5.60 | - |
D-α-Pinene | Rubber | Water | 61.00 | - |
Olive oil | TPFP | Air | 4.10 | - |
Olive oil | TPFP | Water | 21.00 | - |
Olive oil | AF 2400 | Air | 4.50 | - |
Olive oil | AF 2400 | Water | 30.00 | - |
Olive oil | AF 1600 | Air | 4.80 | - |
Olive oil | AF 1600 | Water | 35.00 | - |
Olive oil | PTFE. LD | Air | 5.40 | - |
Olive oil | PTFE. LD | Water | 50.00 | - |
Olive oil | PTFE. HD | Air | 5.95 | - |
Olive oil | PTFE. HD | Water | 60.00 | - |
Olive oil | PDMS (liq) | Air | 4.80 | - |
Olive oil | PDMS (liq) | Water | 40.00 | - |
Olive oil | PDMS (s) | Air | 5.00 | - |
Olive oil | PDMS (s) | Water | 48.00 | - |
Olive oil | PE. LD | Air | 5.60 | - |
Olive oil | PE. LD | Water | 59.00 | - |
Olive oil | Rubber | Air | 5.90 | - |
Olive oil | Rubber | Water | 69.00 | - |
Sunfloweroil | TPFP | Air | 4.00 | - |
Sunfloweroil | TPFP | Water | 20.00 | - |
Sunfloweroil | AF 2400 | Air | 4.60 | - |
Sunfloweroil | AF 2400 | Water | 30.00 | - |
Sunfloweroil | AF 1600 | Air | 4.70 | - |
Sunfloweroil | AF 1600 | Water | 35.00 | - |
Sunfloweroil | PTFE. LD | Air | 5.20 | - |
Sunfloweroil | PTFE. LD | Water | 44.00 | - |
Sunfloweroil | PTFE. HD | Air | 5.90 | - |
Sunfloweroil | PTFE. HD | Water | 57.00 | - |
Sunfloweroil | PDMS (liq) | Air | 4.80 | - |
Sunfloweroil | PDMS (liq) | Water | 40.00 | - |
Sunfloweroil | PDMS (s) | Air | 5.00 | - |
Sunfloweroil | PDMS (s) | Water | 49.00 | - |
Sunfloweroil | PE. LD | Air | 5.70 | - |
Sunfloweroil | PE. LD | Water | 60.00 | - |
Sunfloweroil | Rubber | Air | 5.90 | - |
Sunfloweroil | Rubber | Water | 64.00 | - |
Tricosenoicacid | TPFP | Air | 4.30 | - |
Tricosenoicacid | TPFP | Water | 19.00 | - |
Tricosenoicacid | AF 2400 | Air | 4.90 | - |
Tricosenoicacid | AF 2400 | Water | 30.00 | - |
Tricosenoicacid | AF 1600 | Air | 5.00 | - |
Tricosenoicacid | AF 1600 | Water | 39.00 | - |
Tricosenoicacid | PTFE. LD | Air | 5.70 | - |
Tricosenoicacid | PTFE. LD | Water | 58.00 | - |
Tricosenoicacid | PTFE. HD | Air | 6.20 | - |
Tricosenoicacid | PTFE. HD | Water | 70.00 | - |
Tricosenoicacid | PDMS (liq) | Air | 5.00 | - |
Tricosenoicacid | PDMS (liq) | Water | 40.05 | - |
Tricosenoicacid | PDMS (s) | Air | 5.40 | - |
Tricosenoicacid | PDMS (s) | Water | 50.00 | - |
Tricosenoicacid | PE. LD | Air | 5.90 | - |
Tricosenoicacid | PE. LD | Water | 69.00 | - |
Tricosenoicacid | Rubber | Air | 6.10 | - |
Tricosenoicacid | Rubber | Water | 74.00 | - |
Cd-Arachidate | TPFP | Air | 4.00 | - |
Cd-Arachidate | TPFP | Water | 19.00 | - |
Cd-Arachidate | AF 2400 | Air | 4.30 | - |
Cd-Arachidate | AF 2400 | Water | 27.00 | - |
Cd-Arachidate | AF 1600 | Air | 4.30 | - |
Cd-Arachidate | AF 1600 | Water | 30.00 | - |
Cd-Arachidate | PTFE. LD | Air | 5.08 | - |
Cd-Arachidate | PTFE. LD | Water | 37.00 | - |
Cd-Arachidate | PTFE. HD | Air | 5.50 | - |
Cd-Arachidate | PTFE. HD | Water | 46.00 | - |
Cd-Arachidate | PDMS (liq) | Air | 4.70 | - |
Cd-Arachidate | PDMS (liq) | Water | 42.00 | - |
Cd-Arachidate | PDMS (s) | Air | 5.00 | - |
Cd-Arachidate | PDMS (s) | Water | 50.00 | - |
Cd-Arachidate | PE. LD | Air | 5.40 | - |
Cd-Arachidate | PE. LD | Water | 62.00 | - |
Cd-Arachidate | Rubber | Air | 5.70 | - |
Cd-Arachidate | Rubber | Water | 70.00 | - |
Cellulose | TPFP | Air | 4.90 | - |
Cellulose | TPFP | Water | 18.00 | - |
Cellulose | AF 2400 | Air | 5.20 | - |
Cellulose | AF 2400 | Water | 37.00 | - |
Cellulose | AF 1600 | Air | 5.50 | - |
Cellulose | AF 1600 | Water | 39.00 | - |
Cellulose | PTFE. LD | Air | 6.20 | - |
Cellulose | PTFE. LD | Water | 60.00 | - |
Cellulose | PTFE. HD | Air | 6.90 | - |
Cellulose | PTFE. HD | Water | 83.00 | - |
Cellulose | PDMS (liq) | Air | 5.70 | - |
Cellulose | PDMS (liq) | Water | 40.00 | - |
Cellulose | PDMS (s) | Air | 6.00 | - |
Cellulose | PDMS (s) | Water | 51.00 | - |
Cellulose | PE. LD | Air | 6.50 | - |
Cellulose | PE. LD | Water | 78.00 | - |
Cellulose | Rubber | Air | 6.70 | - |
Cellulose | Rubber | Water | 82.00 | - |
Hexadecane | TPFP | Air | 4.00 | - |
Hexadecane | TPFP | Water | 22.00 | - |
Hexadecane | AF 2400 | Air | 4.50 | - |
Hexadecane | AF 2400 | Water | 32.00 | - |
Hexadecane | AF 1600 | Air | 4.70 | - |
Hexadecane | AF 1600 | Water | 34.00 | - |
Hexadecane | PTFE. LD | Air | 5.10 | - |
Hexadecane | PTFE. LD | Water | 42.00 | - |
Hexadecane | PTFE. HD | Air | 5.60 | - |
Hexadecane | PTFE. HD | Water | 55.00 | - |
Hexadecane | PDMS (liq) | Air | 4.50 | - |
Hexadecane | PDMS (liq) | Water | 38.00 | - |
Hexadecane | PDMS (s) | Air | 5.00 | - |
Hexadecane | PDMS (s) | Water | 31.00 | - |
Hexadecane | PE. LD | Air | 5.10 | - |
Hexadecane | PE. LD | Water | 53.00 | - |
Hexadecane | Rubber | Air | 5.30 | - |
Hexadecane | Rubber | Water | 59.00 | - |
PVA | TPFP | Air | 4.60 | - |
PVA | TPFP | Water | 18.00 | - |
PVA | AF 2400 | Air | 5.10 | - |
PVA | AF 2400 | Water | 33.00 | - |
PVA | AF 1600 | Air | 5.40 | - |
PVA | AF 1600 | Water | 40.00 | - |
PVA | PTFE. LD | Air | 6.08 | - |
PVA | PTFE. LD | Water | 60.00 | - |
PVA | PTFE. HD | Air | 6.40 | - |
PVA | PTFE. HD | Water | 78.00 | - |
PVA | PDMS (liq) | Air | 5.50 | - |
PVA | PDMS (liq) | Water | 40.05 | - |
PVA | PDMS (s) | Air | 5.70 | - |
PVA | PDMS (s) | Water | 71.00 | - |
PVA | PE. LD | Air | 6.10 | - |
PVA | PE. LD | Water | 77.00 | - |
PVA | Rubber | Air | 6.30 | - |
PVA | Rubber | Water | 80.00 | - |
BSA | TPFP | Air | 5.00 | - |
BSA | TPFP | Water | 16.00 | - |
BSA | AF 2400 | Air | 5.50 | - |
BSA | AF 2400 | Water | 29.00 | - |
BSA | AF 1600 | Air | 5.80 | - |
BSA | AF 1600 | Water | 40.00 | - |
BSA | PTFE. LD | Air | 6.40 | - |
BSA | PTFE. LD | Water | 61.00 | - |
BSA | PTFE. HD | Air | 7.00 | - |
BSA | PTFE. HD | Water | 80.05 | - |
BSA | PDMS (liq) | Air | 5.60 | - |
BSA | PDMS (liq) | Water | 42.00 | - |
BSA | PDMS (s) | Air | 6.00 | - |
BSA | PDMS (s) | Water | 60.00 | - |
BSA | PE. LD | Air | 6.50 | - |
BSA | PE. LD | Water | 80.00 | - |
BSA | Rubber | Air | 7.00 | - |
BSA | Rubber | Water | 82.00 | - |
Nylon 6 | TPFP | Air | 4.50 | - |
Nylon 6 | TPFP | Water | 17.00 | - |
Nylon 6 | AF 2400 | Air | 5.00 | - |
Nylon 6 | AF 2400 | Water | 23.00 | - |
Nylon 6 | AF 1600 | Air | 5.10 | - |
Nylon 6 | AF 1600 | Water | 37.00 | - |
Nylon 6 | PTFE. LD | Air | 5.80 | - |
Nylon 6 | PTFE. LD | Water | 50.00 | - |
Nylon 6 | PTFE. HD | Air | 6.20 | - |
Nylon 6 | PTFE. HD | Water | 64.00 | - |
Nylon 6 | PDMS (liq) | Air | 5.20 | - |
Nylon 6 | PDMS (liq) | Water | 40.00 | - |
Nylon 6 | PDMS (s) | Air | 5.40 | - |
Nylon 6 | PDMS (s) | Water | 53.00 | - |
Nylon 6 | PE. LD | Air | 6.08 | - |
Nylon 6 | PE. LD | Water | 79.00 | - |
Nylon 6 | Rubber | Air | 6.30 | |
Nylon 6 | Rubber | Water | 80.00 | - |
Silver | Silver | Vacuum | 20.30 | 38.20 |
Silver | Silver | Nitrogen | 20.30 | 37.90 |
Copper | Copper | Vacuum | 24.82 | 27.20 |
Copper | Copper | Nitrogen | 24.82 | 27.10 |
PTFE | PTFE | Vacuum | 3.63 | - |
PTFE | PTFE | Nitrogen | 3.63 | - |
Silicon Dioxide | Silicon Dioxide | Vacuum | 6.55 | - |
Silicon Dioxide | Silicon Dioxide | Nitrogen | 6.55 | 7.20 |
Titanium Nitride | Titanium Nitride | Vacuum | 15.73 | - |
Titanium Nitride | Titanium Nitride | Nitrogen | 15.73 | - |
Parylene-n | Parylene-n | Vacuum | 11.10 | - |
Parylene-n | Parylene-n | Nitrogen | 11.10 | - |
Silver | Copper | Vacuum | 22.45 | 32.60 |
Silver | Copper | Nitrogen | 22.45 | 32.40 |
Silver | Silicon Dioxide | Vacuum | 11.12 | 12.92 |
Silver | Silicon Dioxide | Nitrogen | 11.12 | 12.70 |
Silver | PTFE | Vacuum | 8.34 | 13.70 |
Silver | PTFE | Nitrogen | 8.34 | 13.60 |
Silver | Parylene-n | Vacuum | 14.30 | 11.80 |
Silver | Parylene-n | Nitrogen | 14.30 | 11.60 |
Silver | Cross linked Parylene-n | Vacuum | 14.30 | 12.10 |
Silver | Cross linked Parylene-n | Nitrogen | 14.30 | 12.00 |
Silver | Titanium Nitride | Vacuum | 16.80 | 16.40 |
Silver | Titanium Nitride | Nitrogen | 16.80 | 16.10 |
Copper | Silicon Dioxide | Vacuum | 11.60 | 14.10 |
Copper | Silicon Dioxide | Nitrogen | 11.60 | 13.90 |
Copper | PTFE | Vacuum | 8.72 | 13.10 |
Copper | PTFE | Nitrogen | 8.72 | 12.80 |
Copper | Parylene-n | Vacuum | 15.00 | 9.80 |
Copper | Parylene-n | Nitrogen | 15.00 | 10.10 |
Copper | Cross linked Parylene-n | Vacuum | 15.00 | 11.00 |
Copper | Cross linked Parylene-n | Nitrogen | 15.00 | 11.10 |
Copper | Titanium Nitride | Vacuum | 17.59 | 12.30 |
Copper | Titanium Nitride | Nitrogen | 17.59 | 12.50 |
Silicon Dioxide | PTFE | Vacuum | 4.87 | - |
Silicon Dioxide | PTFE | Nitrogen | 4.87 | 7.60 |
Silicon Dioxide | Parylene-n | Vacuum | 8.55 | - |
Silicon Dioxide | Parylene-n | Nitrogen | 8.55 | 6.80 |
Silicon Dioxide | Cross linked Parylene-n | Vacuum | 8.55 | - |
Silicon Dioxide | Cross linked Parylene-n | Nitrogen | 8.55 | 6.90 |
Silicon Dioxide | Titanium Nitride | Vacuum | 10.10 | - |
Silicon Dioxide | Titanium Nitride | Nitrogen | 10.10 | 8.80 |
^{1}Hamaker constants for water (j) and air (vacuum) (k) interacting across air (vacuum) are 3.7 and 0, respectively.
Table 2. Forces in AFM measurements, where the type of force is given in the first column, that also specifies whether the interaction is more common in air (a), vacuum (v) or solution (s). Special features of each of the forces are mentioned in the 3rd column, while the second column provides either the expression for the force or the Section in this paper in which further information can be found [43,107,108]. |
Pull-on force | ||
---|---|---|
Types of force | Topics or equations | Special features |
van der Waals (a, v & s) | See Section2 | Ubiquitous force both in vacuum and in liquids, existing between all bodies. |
Hydration (s) | See Section5 (Topic C) | Hydration repulsive force attributed to the energy required to remove the water of hydration from the surface, or the surface adsorbed species. |
Solvation (s) | See Section5 (Topic C) | Solvation forces arise whenever liquid molecules are compelled to order in almost discrete layers between two surfaces. |
Double-Layer (s) | See Section 5 (Topic C) | A force that exists only between charged molecules (ions) or surfaces, and depends on the electrolyte concentration. |
Elastic (a, v & s) | ${F}_{els}=\frac{4E\sqrt{{R}_{t}}}{3\left(1-{\nu}^{2}\right)}{\delta}^{3/2}$ | Relation between the applied forces to the depth of indentation as the tip is pushed against the sample. |
Brush (a, v & s) | ${F}_{b}=\frac{50L{k}_{B}T}{{d}^{3}}{e}^{-2\pi D/L}$ | Polymer-brushing forces that result from the thermally driven motion of polymers grafted onto a solid surface in solution. |
Pull-off force | ||
Adhesion (a, v & s) | See Section 5 (Topic A) | Adhesion between a sphere and a plane in the absence of contaminating adsorbates (typically in a vacuum). |
Capillary (a) | See Section 5 (Topic B) | Capillary adhesion–very common under ambient conditions, under which many surfaces have a thin water layer. |
Hydrophobic (s) | See Section 5 (Topic C) | The hydrophobic force has different origins depending on the system. For example, when two hydrophobic surfaces are in contact, a vapor cavity bridging is formed to cause strong adhesion. |
Polymer Extension (a, v & s) | ${F}_{pol}=\frac{{k}_{B}T}{\varsigma}L*\left(\frac{x}{N\varsigma}\right)$ | Polymers break or detach from one of the surfaces (tip and sample). |
Specific Binding (a, v & s) | ${F}_{B}=\frac{U-kT\hspace{0.17em}\text{ln}\left(\tau /{\tau}_{o}\right)}{\mathrm{\Lambda}}$ | Specific interactions (chemical force microscopy). Antibody-antigen interactions, receptor-ligand interactions and complementary binding. |
Note: (v), (s) and (a) apply to interactions in vacuum, solution and air, respectively. Definitions: E: Elastic modulus, R_{t}: Radius of probe sphere (tip), ν: Poisson ratio, δ: Indentation depth, L: Brush thickness in a good solvent, D: Probe-sample distance, U: Bond energy, τ: Period over which the bond will rupture, τo: Reciprocal of the natural bond frequency, ζ: Monomer length, L*: Inverse Langevin function, x : Elongation of a polymer, N: Number of units in a polymer, d: mean distance between polymers.
Table 3. vdW interaction potential (w(r)) and force (F = −dw/dr) between macroscopic bodies, for the most common geometries. R is the radius of the spheres or cylinders, D is the distance between the interacting bodies, and A is the Hamaker constant [23,43]. A negative force F implies attraction (A positive), a positive force means repulsion (A negative). |
Geometry (D << R) | vdW Interactions | |
---|---|---|
Force | Energy | |
Two atoms or small molecules | $F(r)=-\frac{6{C}_{vdW}}{{r}^{7}}$ | $w(r)=-\frac{{C}_{vdW}}{{r}^{6}}$ |
Atom-surface | $F(D)=-\frac{3\pi C\rho}{6{D}^{4}}$ | $w(D)=-\frac{\pi C\rho}{6{D}^{3}}$ |
Two spheres | $F(D)=-\frac{A}{6{D}^{2}}\left(\frac{{R}_{1}{R}_{2}}{{R}_{1}+{R}_{2}}\right)$ | $w(D)=-\frac{A}{6D}\left(\frac{{R}_{1}{R}_{2}}{{R}_{1}+{R}_{2}}\right)$ |
Sphere-flat surface | $F(D)=-\frac{AR}{6{D}^{2}}$ | $w(D)=-\frac{AR}{6D}$ |
Two flat plates | $F(D)=-\frac{A}{6\pi {D}^{3}}$ | $w(D)=-\frac{A}{12\pi {D}^{2}}$ |
Two cylinders or fi1aments crossed at 90° | $F(D)=\frac{-A\sqrt{{R}_{1}{R}_{2}}}{6{D}^{2}}$ | $w(D)=\frac{-A\sqrt{{R}_{1}{R}_{2}}}{6D}$ |
Cylinder near a flat surface | $F(D)=-\frac{-A\sqrt{R}}{8\sqrt{2}{D}^{{\scriptstyle \frac{5}{2}}}}$ | $w(D)=-\frac{-A\sqrt{R}}{12\sqrt{2}{D}^{{\scriptstyle \frac{3}{2}}}}$ |
Two parallel cylinders or rods | $F(D)=\frac{-A}{8\sqrt{2}{D}^{{\scriptstyle \frac{5}{2}}}}{\left(\frac{{R}_{1}{R}_{2}}{{R}_{1}+{R}_{2}}\right)}^{1/2}$ | $w(D)=\frac{-A}{12\sqrt{2}{D}^{{\scriptstyle \frac{3}{2}}}}{\left(\frac{{R}_{1}{R}_{2}}{{R}_{1}+{R}_{2}}\right)}^{1/2}$ |
Table 4. Experimental results for several samples in vacuum [154]. |
Sample | Surface Energy γ_{lit} (mJ/m^{2}) | Tip radius (μm) | Attractive force (nN) |
---|---|---|---|
Mica | 300, 375 | 2.5 ± 0.5 | 230 ± 30 |
Graphite | 96, 123 | 2.5 ± 0.5 | 140 ± 90 |
Al_{2}O_{3} | 45 | 2.0 ± 0.5 | 85 ± 25 |
CH_{3}(CH_{2})_{16}COOH | 21 | 2.0 ± 0.5 | 17 ± 11 |
CF_{3}(CH_{2})_{16}COOH | 20 | 3.0 ± 0.5 | 5.0 ± 4.0 |
PTFE | 18 | 2.5 ± 0.5 | 2.0 ± 2.0 |
© 2012 by the authors; licensee Molecular Diversity Preservation International, Basel, Switzerland. This article is an open-access article distributed under the terms and conditions of the Creative Commons Attribution license (http://creativecommons.org/licenses/by/3.0/).