A Study of Strong Confinement Regions Using Informational Entropy

Abstract

We present an informational study of a spherically confined hydrogen atom, a hydrogenic ion confined in a strongly coupled plasma, a spherically confined harmonic oscillator, and a particle confined in a cage. For this, we have implemented a numerical procedure to obtain information entropies of these confined quantum systems. The procedure is based on the variational formalism that uses the finite element method (FEM) for the expansion of the wavefunction in terms of local base functions. Such a study is carried out in order to analyze what happens in the rigorous confinement regime. In particular, we have shown that the effects of the interaction potential is no longer important for rigorous confinements and the studied systems start to behave just like an electron confined by a impenetrable spherical cage. When possible, we compared our results with those published in the literature.

1. Introduction

The study of confined quantum systems is a field that examines the spatial limitation effects on the physical properties of the electrons, nuclei, atoms, or molecules. The literature contains several theoretical and experimental works indicating that the spatial confinement changes the physical and chemical properties of the systems [1,2,3]. For instance, when the hydrogen atom is confined by impenetrable walls the energy spectrum is altered; moreover, in confined environments some alkali metals present electronic configurations similar to those of transition metals [4,5]. In recent years, with the increases in computational capacity and the development of modern techniques, this question has received considerable attention [6,7,8,9,10].

In the Schrödinger equation that describes the confined system, we can use a model potential that has both nuclear and confinement potential properties [11]. The choice of the potential model depends on the physical system of interest and of the characteristics of the confinement [12,13,14,15,16]. For instance, we can use infinite potential barriers models [17,18] or soft barriers models [19,20].

In particular, strong or rigorous confinement region includes interesting details such as: (a) it has a highly concentrated probability density when compared to the weakly confined regions; (b) the kinetic energy of electrons is large in contrast to their potential energy; and (c) the influence of the confinement barrier becomes greater than the free system potential [21,22,23,24]. The rigorous confinement region is established when the confinement radius of the system goes to zero. Energy studies based on ionization energy have been successfully undertaken in mapping this specific region [25,26,27].

In the atomic, molecular and chemical-physical context we define the informational entropies (or Shannon entropy) on position, $S_r$; on momentum, $S_p$; spaces; and the entropy sum, $S_t$, by adding $S_r$ and $S_p$ [28,29]. These informational quantities have been utilized in the study of various confined quantum systems such as the confined hydrogen-like atoms [30,31,32,33,34,35], the confined He-like atoms [36,37], plasma environments [38,39], and in many other systems [40,41,42]. Analysis of basis functions [29,43] and electronic correlation [36,44,45], as well as physical and chemical phenomena [46,47,48,49] are also being approached in the informational field.

Despite of the energy analysis, the information entropies have been used as a powerful tool to study the regions where the effects of confinement are extreme. According to previous studies using entropic quantities, we have that the influence of the one-dimensional harmonic [50] and Coulomb [29] potentials is practically nullified by the presence of strong confinement. Moreover, in this specific region of the system (where the confinement radius tends to zero) the effects of Coulomb correlation in confined helium-like atoms become negligible [36].

The main goal of this work is to analyze how information entropy can contribute to the understanding of the strong confinement regime. For this, we have determined entropic quantities of interest for the spherically confined hydrogen atom, the hydrogenic ion confined in a strongly coupled plasma, and the spherically confined harmonic oscillator and compare them with the results of a particle confined in a cage.

This paper is organized as follows: in Section 2 we present the physical systems of interest, the numerical procedures based on the variational formalism using the finite element method, and beyond the informational formalism adopted; in Section 3 we discuss the results obtained; and, finally, in Section 4 we summarize the central aspects of our investigation.

2. Theoretical Background

In this section, we present the concepts and methods applied in our research. In Section 2.1, we discuss the physical systems and the variational formulation of the problem. Moreover, in Section 2.2, we define the informational quantities of interest.

2.1. System of Interest

The radial Schrödinger equation, using atomic units, is given by

$$\left[-\frac{1}{2r^2}\frac{d}{dr}{r}^2\frac{d}{dr}+\frac{l(l+1)}{2r^2}+V\left(r\right)-E_{nl}\right]{\phi }_{nl}\left(r\right)=0,$$

(1)

where ${\phi }_{nl}\left(r\right)$ is the radial wavefunction solution, $E_{nl}$ the energy of the stationary state, and $V\left(r\right)$ the potential model. The labels n and l refer to the main and angular quantum numbers, respectively. The total wavefunction solution for a particular $(n,l,m)$ quantum numbers is given by

$${\psi }_{nlm}\left(\overrightarrow{r}\right)={\phi }_{nl}\left(r\right)Y_{lm}(\Omega ),$$

(2)

where $Y_{lm}(\Omega )$ is the correspondent spherical harmonic and $\Omega$ is the solid angled.

Here, we consider four different model potentials of the type infinite spherical barrier to confine an electron. For models that contain an atomic nucleus, it is located at the center of the hard sphere. Our starting point is the potential that describes a particle (electron) confined in a spherical cage, that is,

$$V_1\left(r\right)=\left\{\begin{array}{cc}0,& 0<r<r_c\\ \infty ,& r\ge r_c\end{array}\right.,$$

(3)

where $r_c$ is the confinement radius. For the r range of values between $0<r<r_c$ the particle is free of potential and at the confinement frontier the value of the potential is infinite.

Following, we have the Coulomb potential model of confined hydrogenic-like atoms,

$$V_2\left(r\right)=\left\{\begin{array}{cc}-\frac{Z}{r},& 0<r<r_c\\ \infty ,& r\ge r_c\end{array}\right.,$$

(4)

where Z is the nuclear charge. We also consider an electron under influence of the isotropic harmonic potential, given by,

$$V_3\left(r\right)=\left\{\begin{array}{cc}\frac{1}{2}{\omega }^2{r}^2,& 0<r<r_c\\ \infty ,& r\ge r_c\end{array}\right.,$$

(5)

where $\omega$ is the angular frequency.

Finally, we selected to study one electron in a plasmatic environment of the sphere model. For strongly coupled plasma surrounding an ion having a single valence electron, one can define a sphere of radius $r_c$ such that the plasma electrons with density $\gamma$ is sufficient to neutralize ($Z-1$) of central positive charge:

$$r_c={\left[\frac{Z-1}{4\pi \gamma /3}\right]}^{\frac{1}{3}}.$$

Under this condition the interaction potential energy of the electron with an ion is

$$V_4\left(r\right)=\left\{\begin{array}{cc}-\frac{Z}{r}+\frac{(Z-1)}{2r_c}\left[3-{\left(\frac{r}{r_c}\right)}^2\right]& \mathrm{and}r<r_c\\ \infty & \mathrm{and}r\ge r_c\end{array}\right..$$

(6)

To solve the radial Schrödinger Equation (1) with the potentials (3), (4), (5), or (6) by using the variational principle, for a given angular moment l, it corresponds to find the results that agree with the extreme condition of the energy functional, $\delta J_l\left[{\chi }_{nl}\right]=0$, where the function ${\chi }_{nl}\left(r\right)=r{\phi }_{nl}\left(r\right)$ must vanish at the origin and at the surface of a sphere of radius $r=r_c$ due to confinement (boundary conditions).

In variational context, the radial wavefunctions and energy eigenvalues are found by expanding the function ${\chi }_{nl}$ in terms of a finite basis set $\left\{f_j\right\}$, that is,

$${\chi }_{nl}\left(r\right)=\sum _{j=1}^p{c}_j{f}_j\left(r\right),$$

(7)

where $\left\{c_j\right\}$ are the coefficients of the expansion. The efficiency of the numerical calculation depends on the choice of the finite basis set. The variational solutions are obtained by solving the generalized eigenvalue eigenvector problem

$${\mathbf{H}}^l\mathbf{c}=E\mathbf{O}\mathbf{c},$$

(8)

where $\mathbf{c}$ is the vector of the expansion coefficients $\left\{c_j\right\}$, being

$${\left\{{\mathbf{H}}^l\right\}}_{ij}={\int }_0^{r_c}dr\left\{\frac{1}{2}\frac{d{f}_i^{*}\left(r\right)}{dr}\frac{d{f}_j\left(r\right)}{dr}+f_i^{*}\left(r\right)V_l^{ef}\left(r\right)f_j\left(r\right)\right\}$$

(9)

and

$${\left\{\mathbf{O}\right\}}_{ij}={\int }_0^{r_c}dr{f}_i^{*}\left(r\right)f_j\left(r\right),$$

(10)

where the effective potential is written as $V_l^{ef}\left(r\right)=V\left(r\right)+l(l+1)/2r^2$.

The variational methodology that we use to solve the problem is the p-version of the finite element method (p-FEM). In the radial case, the p-FEM consist of dividing the range of integration $[0,r_c]$ into $N_e$ elements, being the i-th element defined in the range of $r_{i-1}$ up to $r_i$ with $r_0=0$ and $r_{N_e}=r_c$, and the radial wavefunction is expanded in local base functions {$f_j^i$} satisfying the following property:

$$f_j^i\left(r\right)=0\mathrm{if}r\notin [r_{i-1},r_i],$$

(11)

where $f_j^i\left(r\right)$ is the j-th polynomial associated with i-th element and is its highest order given by the parameter $k_i$. Thus, considering the properties (11), the matrix representation of any local operator assumes a block tridiagonal form and the spatial confinement on the radial wavefunction can be imposed easily just removing the basis function $f_{k_i}^{N_e}\left(r\right)$ of the expansion. For more details, see references [11,51,52].

2.2. Shannon Informational Entropy

The Shannon information entropy in the atomic, molecular, and chemical physics context can be defined in terms of quantum-mechanical wavefunction. Therefore, information entropies on position, $S_r$, and momentum, $S_p$, spaces, in atomic units, are recognized as [29]

$$S_r=-\int d\overrightarrow{r}{|{\psi }_{nlm}\left(\overrightarrow{r}\right)|}^{2}ln\left[{|{\psi }_{nlm}\left(\overrightarrow{r}\right)|}^2\right]$$

(12)

and

$$S_p=-\int d\overrightarrow{p}{|{\tilde{\psi }}_{nlm}\left(\overrightarrow{p}\right)|}^{2}ln\left[{|{\tilde{\psi }}_{nlm}\left(\overrightarrow{p}\right)|}^2\right],$$

(13)

where ${\psi }_{nlm}\left(\overrightarrow{r}\right)$ and ${\tilde{\psi }}_{nlm}\left(\overrightarrow{p}\right)$ are the total position and momentum space wavefunction, respectively. Detailed discussions of the dimensionality of expressions (12) and (13) can be found in Refs. [29,53].

Using the variable separation method the wavefunctions can be written as

$${\psi }_{nlm}\left(\overrightarrow{r}\right)={\phi }_{nl}\left(r\right)Y_{lm}(\Omega )\mathrm{and}{\tilde{\psi }}_{nlm}\left(\overrightarrow{p}\right)={\tilde{\phi }}_{nl}\left(p\right)Y_{lm}(\Omega ),$$

(14)

where $Y_{lm}$ are the spherical harmonics and $\Omega$ is the solid angled. Furthermore, the relationship between ${\tilde{\phi }}_{nl}\left(p\right)$ and ${\phi }_{nl}\left(r\right)$ is given by [54]

$${\tilde{\phi }}_{nl}\left(p\right)={\int }_0^{r_c}{r}^2{j}_l\left(pr\right){\phi }_{nl}\left(r\right)dr,$$

(15)

being $j_l$ the spherical Bessel function. Employing the expressions (14) in Equations (12) and (13) we separate the $S_r$ and $S_p$ entropies into two parts, that is [55],

$$S_r=S_{\phi }+S_{\Omega }$$

(16)

and

$$S_p=S_{\tilde{\phi }}+S_{\Omega }.$$

(17)

The radial parts $S_{\phi }$ and $S_{\tilde{\phi }}$ that depends on the potential function are

$$S_{\phi }=-{\int }_0^{r_c}dr{r}^2{\left|{\phi }_{nl}\left(r\right)\right|}^{2}ln\left[|{\phi }_{nl}\left(r\right){|}^2\right],$$

(18)

and

$$S_{\tilde{\phi }}=-{\int }_0^{\infty }dp{p}^2{\left|{\tilde{\phi }}_{nl}\left(p\right)\right|}^{2}ln\left[|{\tilde{\phi }}_{nl}\left(p\right){|}^2\right].$$

(19)

The angular contribution known as angular entropy (common for $S_r$ and $S_p$) is given by

$$S_{\Omega }=-{\int }_{\Omega }d\Omega {\left|Y_{lm}(\Omega )\right|}^{2}ln\left[|Y_{lm}(\Omega ){|}^2\right].$$

(20)

The $S_{\Omega }$ quantity is independent of the potential and has a closed form determined by

$$S_{\Omega }=-log\left(\frac{(2l+1)(l-m)!}{4\pi (l+m)!}\right)-\left(\frac{(2l+1)(l-m)!}{2(l+m)!}\right){\int }_{-1}^1{\left[P_l^m\left(t\right)\right]}^{2}ln{\left[P_l^m\left(t\right)\right]}^{2}dt,$$

(21)

where $P_l^m$ is the Legendre function.

The $S_t$ quantity is obtained from entropy sum of $S_r+S_p$. From the entropy sum we can still derive the following entropy uncertainty relation:

$$\begin{array}{ccc}\hfill S_t& =& S_r+S_p\hfill \\ & =& -{\int }_0^{r_c}{\int }_0^{\infty }drdp{r}^2{p}^2|{\phi }_{nl}\left(r\right){|}^2{\left|{\tilde{\phi }}_{nl}\left(p\right)\right|}^{2}ln\left(|{\phi }_{nl}\left(r\right){|}^2{\left|{\tilde{\phi }}_{nl}\left(p\right)\right|}^2\right)+2S_{\Omega }\hfill \\ & \ge & 3(1+ln\pi ).\hfill \end{array}$$

(22)

This entropy uncertainty relationship is also known as the BBM inequality relation [56], which it is a common theorem for any quantum system. From expression (23) we can obtain Kennard’s uncertainty relationship as discussed in Ref. [56].

3. Results and Discussions

This section presents the data obtained respective analysis of Shannon entropies, in atomic units, for a particle confined in a spherical cage (Equation (3)), the confined hydrogen atom (Equation (4) with $Z=1$), spherically confined harmonic oscillator (Equation (5) with $\omega =1$), and hydrogenic ion confined in a strongly coupled plasma (Equation (6) with $Z=2$). For this, we have implemented the procedure based on the theory presented previously using the computer language Fortran. Unless stated otherwise, all curves were fitted with cubic spline interpolation utilizing the free application SciDAVis. Particularly, for the hydrogen atom, our computational implementation obtained values equivalent to accurate results existing in the literature [33].

The difference, $\Delta S_r$, between the values of position space entropy of each of the three systems and that of the particle confined in a cage, calculated by Equation (16), as function of confinement radius, $r_c$, on a logarithmic scale, are shown in Figure 1a–c, for the confined hydrogen atom, the confined ion in a strongly coupled plasma, and the spherically confined harmonic oscillator, respectively. We plot all states with principal quantum numbers $1\le n\le 5$ and $0\le l\le 4$. The first observation is that for the three systems the quantities $\Delta S_r$ tend to zero when the confinement radius decreases, indicating that in a rigorous confinement regime the position entropy of the systems tends to behave like that of a particle confined in a cage. The second observation is that, in general, the more excited the state, the faster $\Delta S_r$ moves towards zero. This is in agreement with our intuition that since the more excited states are less influenced by the interaction potential, they tend more quickly towards the behavior of a particle in a spherical cage.

Particularly, it can be seen that the behavior of the entropy difference of the hydrogen confined and the ion-sphere are very similar. By zooming the graph in the region of small radii (Figure 1a,b), it is visible that the $1s$ state is less influenced by confinement when compared to the others states. In turn, by zooming in on the graph (Figure 1c), it can be seen that the values of the position space entropy difference of the harmonic oscillator tend to zero for larger values of $r_c$ than the others systems.

It is also remarkable that some regions of $r_c$ have states with positive entropy differences. This is counterintuitive since the position Shannon entropy indicates the delocalization of density. Considering that one of the systems has an attractive potential, our intuition is that the density of this system would always be less spread out than that of the particle in a cage. The states that present $\Delta S_r>0$ are $2s$, $3s$, $4s$, $5s$, $3p$, $4p$, $5p$, and $5d$, for the confined hydrogen and the ion-sphere; and, in the case of the harmonic oscillator, the states $4d$ and $5f$ are added.

In Figure 2a–c are shown the difference, $\Delta S_p$, between the values of momentum space entropy of each of the three systems and that of the particle confined in a spherical cage, calculated from Equation (17), as function of $r_c$ on a logarithmic scale, for the confined hydrogen atom, the confined ion in a strongly coupled plasma and the spherically confined harmonic oscillator, respectively. We have displayed in Figure all states with principal quantum numbers $1\le n\le 5$ and $0\le l\le 4$. We observe similar behavior to that of position space entropy when the confinement radius tends to zero, decreasing its amplitude gradually to zero. This confirms that the interaction potential is no longer important for rigorous confinements and the system starts to behave like an electron confined in a spherical cage.

In the case of moment space entropy, the comparison between states and systems is quite similar to the one made for position space entropy. The sign change behavior of the entropy difference in some regions of $r_c$ is also noticed for the hydrogen confined and the ion-sphere systems. In particular, the entropy difference of some states seems to oscillate more prominently when compared to the position space ones. The states that present $\Delta S_p<0$ are $2s$, $3s$, $4s$, $5s$, $4p$, and $5p$ and $5d$, for the confined hydrogen and the ion-sphere, respectively; and, in the case of the harmonic oscillator, there are no regions with sign change.

Now, we analyze the difference, $\Delta S_t$, between the values of entropy sum of each of the three systems and that of the particle confined in a cage, calculated by Equation (23), as function of confinement radius, $r_c$. Specifically, $\Delta S_t$ for states with $1\le n\le 5$ and $0\le l\le 4$ are shown in Figure 3a–c for the confined hydrogen atom, the confined ion in a strongly coupled plasma and the spherically confined harmonic oscillator, respectively. Again we observe that all $\Delta S_t$, for the three systems, tend to zero when the confinement radius decreases. This indicates that in a rigorous confinement regime the entropy sum tends to behave like that of a particle confined in a spherical cage.

However, a different behavior of $\Delta S_t$ can be noticed when compared with $\Delta S_r$ and $\Delta S_p$ for intermediate and large values of $r_c$. In the entropy sum case, the values of $\Delta S_t$ converge asymptotically to constant values. For the $\Delta S_r$ and $\Delta S_p$ quantities, the values increase (positively or negatively) due to the behavior of $S_r$ and $S_p$ for an electron confined in a spherical cage (see discussion at the end of this section).

Note that a particular state of a given system with $\Delta S_t>0$ ($\Delta S_t<0$) has a larger (smaller) entropy sum than the same state for a particle confined in a cage for a given radius of confinement. That is, several states of the three systems under study have a lower entropy sum when free ($r_c>>1$) than when subjected to strong confinement. For intermediate values of $r_c$ we can observe oscillations in $\Delta S_t$, confirming that confinement affects the position and momentum spaces differently.

The strong or rigorous confinement regime can be defined when the influence of the confining potential becomes greater than the free atomic system potential to specific configurations (or $r_c$ values). Based on the entropy sum, $S_t$, of the ground state Nascimento et al. [36] defined three regions for confined atomic systems. The intermediate region is formed by $r_c$ values that limit the half well depth in the ground state $S_t$ versus $r_c$ curve. The half well depth is given by

$$\begin{array}{c}\hfill \sigma =\frac{S_t(r_c\to \infty )-S_t\left(r_c^{min}\right)}{2},\end{array}$$

(23)

where $S_t$ values are calculated in $r_c$ tending to infinity and in $r_c^{min}$ ($r_c$ value where $S_t$ assumes a minimal value). The strong and weak confinement correspond to the regions where are dominant the confinement ($r_c\to 0$) or Coulombian ($r_c\to \infty$) potentials, respectively. In

Table 1. Confinement regions for the hydrogen confined (HC), ion-sphere (IS), and confined harmonic oscillator (HO).

	$\mathit{\sigma }$	Strong	Intermediate	Weak
HC	0.040	$r_c<1.17$	$1.17\le r_c\le 4.51$	$r_c>4.51$
IS	0.035	$r_c<0.56$	$0.56\le r_c\le 2.36$	$r_c>2.36$
HO	0.000	$r_c<2.00{}^{†}$	–	–

${}^{†}$ Obtained from Figure 4.

, we determine the three regions from each of the three examined systems.

Note in Table 1 that the strong confinement region is smaller in the ion-sphere model than in the confined hydrogen atom. This indicates that, with respect to the confinement radius, the interaction potential of a hydrogen ion in a strongly coupled plasma surrounding is less influenced than the Coulomb potential of hydrogen atom. On the other hand, in the case of the harmonic oscillator, we verified that it was not possible to establish the three confinement regions by Equation (23), since there is no well in the ground state curve of $S_t$ versus $r_c$. Indeed, as seen in Figure 3c, the influence of the confinement potential is greater even for larger confinement radii. To overcome this difficulty, we propose an additional criterion to deal with the harmonic oscillator case. To propose it, we consider Figure 4 where we show the values of $\Delta S_r$ in the ground state as a function of $r_c$ for the three systems. In such a figure we notice that $\Delta S_r\approx -0.17$ in the confinement radius that defines the beginning of the strong confinement region for the hydrogenoid models. Thus, we propose the value of $r_c$ when $\Delta S_r=-0.17$ to define the strong confinement region of the harmonic oscillator, written in Table 1. Establishing a criterion using $S_r$ can be particularly advantageous in situations where it is difficult to calculate $S_p$.

Furthermore, in Figure 5a–d are shown the entropy sum, $S_t$, of the four systems as function of $r_c$ on a logarithmic scale in the weak and intermediate regions ($1\le r_c\le 100$). We plot all states with principal quantum numbers $1\le n\le 4$ and $0\le l\le 3$. Thus, it becomes clear from the figures for approximately which confinement radius, $r_c$, a given state of a specific system is in its lowest entropy sum configuration. Specifically, the $1s$ state is always the lowest entropy sum for all systems studied. On the other hand, some states have the lowest entropy sum for intermediate values of $r_c$, while others have a lower entropy for the free configuration or in the strong confinement region. Moreover, we see that for the confined hydrogen atom and the ion confined in a strongly coupled plasma the states with angular momentum quantum number s (except the $1s$ state) are the most affected by confinement, while for the harmonic oscillator the $3s$ and $4s$ states, although affected, decrease their entropy sum.

We now investigate only the particle confined in a spherical cage. In Figure 6, are displayed the entropies $S_r$ and $S_p$ as a function as a function of $r_c$ on a logarithmic scale. We plot all states with principal quantum numbers $1\le n\le 3$ and $0\le l\le 2$. Note that the values of $S_r$ are quite close for different quantum states. The same behavior was also observed by Nascimento et al. in [53] for the problem of one-dimensional infinite potential well. They have qualitatively explained such behavior by analyzing the probability densities in the position and momentum spaces. According to their explanation, the probability densities in the position are spread by same range of r values leading to equal values of $S_r$ for all levels while in the momentum space the probability densities are spread for increasing ranges of p values leading to increase in $S_p$ with the level increment.

Moreover, Figure 6 also shows that entropies are linear on the monolog axes. In fact, the coefficient of determination gives $R^2=1$, demonstrating that the linear model fits perfectly to the sample of points. For the $1s$ state, for example, the linear regression fit of dataset gives $S_r=3.0log\left(r_c\right)+0.7$ and $S_p=-3.0log\left(r_c\right)+5.9$; and for $2p$ state gives $S_r=3.0log\left(r_c\right)+0.5$ and $S_p=-3.0log\left(r_c\right)+6.5$. As expected, the slopes of the straight lines $S_r$ and $S_p$ have opposite values so that in the sum $S_t=S_r+S_p$ the term with the $log\left(r_c\right)$ will be canceled, showing that the entropy sum is constant, as it can be seen in Figure 5d. Note that the entropy curves for states $1s$ and $2p$ form two parallel lines (same slope) and that the $S_r$ lines are much closer to each other (nearby y-intercepts) than the $S_p$ lines.

Since it has been shown, in the strong confinement regime, that the three systems previously studied begin to behave like a particle confined in a spherical cage, then this also means that in this regime the entropies of these systems start to have a linear behavior as a function of $log\left(r_c\right)$. Such behavior is evidenced by Figure 7, where we plot the graph of the values of entropy $S_r$ in the ground state as a function of $r_c$ on the logarithmic scale for the four systems in question. We can see in Figure 7 that the changes in behaviors for the linear trend of the confined particle happen almost abruptly near the regions of strong confinement defined in Table 1.

4. Conclusions

In this work, we presented a comparative study between some confined systems using Shannon’s informational entropies as tools to analyze how the effects of confinement impact in these systems. For that, we implemented a computational code in Fortran based on the finite element method to solve the radial part of the Schorödinger equation. In particular, we determined the position and momentum space entropies and the entropy sum for different states of the following systems: a particle confined in a spherical cage, the spherically confined hydrogen atom, the hydrogenic ion confined in a strongly coupled plasma, and the spherically confined harmonic oscillator.

Our main observation was that the difference between values of entropies for all states of each of the three systems and that of the particle confined in a spherical cage tend to zero when the confinement radius decreases. This confirms that the interaction potential is no longer important for rigorous confinements and the system starts to behave just like an confined electron. Furthermore, we observed that the behavior of these entropies differences for the hydrogen confined and the ion-sphere are very similar, while for the harmonic oscillator they tend to zero faster. A counterintuitive behavior also noticed for the hydrogen confined and the ion-sphere systems was the sign change of the entropy difference on position and momentum spaces in some regions of confinement radius indicating that the density of these systems is more spread out than that of the particle in a cage.

We also determined in this work the three confinement regions of three of the examined systems using a procedure based on entropy sum proposed by Nascimento et al. [36]; and an additional criterion, using the entropy of space, was required to define the strong confinement region of the harmonic oscillator. Lastly, we only investigate the particle confined in a spherical cage. Besides the quite close values of entropy in the position space for different quantum states, we observed that entropies are linear on monolog axis. This means that in strong confinement regime the entropies of the other systems start to behave as a logarithmic function of the confinement radius.

As a final conclusion, with the employment of a very accurate numerical procedure, we have shown significant results on the behavior of strongly confined quantum systems and demonstrated the feasibility of using Shannon’s informational entropies as a tool to analyze such behavior. As a perspective, we intend to extend the method to calculate Shannon’s informational entropy for excited states of two-electron atoms and artificial atoms in the presence of external fields.