1. Introduction
Increasing contamination of water is one of the most pressing environmental challenges. The development of the industrial, pharmaceutical and textile industries generates wastewater containing dyes, pesticides and other persistent organic pollutants that are hazardous for human life [
1,
2]. Traditional wastewater treatment methods, such as chemical treatment, filtration or bio-treatment, are becoming ineffective in removing persistent organic pollutants [
3]. In this context, the advanced oxidation processes, whose degradation mechanism of persistent organic pollutants relies on the generation of radical oxidating species (ROS), seems to be a promising field [
4]. Among them, photocatalysis has been postulated as a natural candidate for this environmental problem due to its low cost, the chemical stability of the main catalysts and the capability of complete degradation of the polluted water [
1,
5].
Photocatalysis can be distinguished depending on the mode of generating electron–hole pairs: by ultraviolet light (UV photocatalysis) or visible light (visible photocatalysis). This distinction is usually made with regard to the experimental method and its results, since UV photocatalysis is more effective than visible photocatalysis [
1]. Nevertheless, visible photocatalysis has become more acceptance since visible light is directly available from the sun and hence more eco-friendly [
6]. In both cases, the underlying physical mechanisms are the same, and as long as the photon energy is high enough to overcome the band gap, independent of the photon source.
The fundamentals of photocatalysis are based on concepts that involve solid state physics and surface physics. For the sake of explanation, let us assume it to be in UV photocatalysis, and assume also that a solid semiconductor catalyst is submerged in a liquid phase with a dissolved pollutant. In this case, the semiconductor is irradiated with light whose wavelength is greater than the bandgap energy and, therefore, electrons from the valence band are promoted to the conduction band, which involves creating electron–hole pairs. Such pairs migrate to the surface of the catalyst and can react with adsorbed water molecules or dissolved gaseous oxygen to generate ROS, which will in turn react with the adsorbed pollutant and will degrade it into non-pollutant species. It is important to consider that the process of photocatalysis takes place on the surface of the catalyst all the time, and this is the reason why so much effort is made to increase the effective surface of the catalysts [
7,
8,
9,
10]. More specifically, the chemical reactions taking place in the process, following Houas et al. [
11], are as follows:
Absorption of photons by the catalyst:
Oxygen ionosorption:
Neutralization of OH− groups by photoholes:
Neutralization of by protons:
Hydrogen peroxide formation and dismutation of oxygen:
Decomposition of hydrogen peroxide:
Oxidation of organic reactants (R) by OH radicals:
Direct oxidation by reaction with holes:
Theoretical photocatalysis studies began with gas–solid adsorption studies by Langmuir, which settled the bases for current theories [
12,
13]. Later, many theoretical studies of photocatalysis have focused on the mechanisms governing this process, which yields the formulation of several models, the Langmuir–Hinshelwood (LH) equation being the most used among them to describe the experiments [
14,
15]. However, the mathematical treatment of this equation has often been relegated to a second plane, due to its complexity and the subsequent difficulty finding a closed solution. In previous works [
15,
16], different approximations have been developed to determine the different kinetical parameters; however, the conditions for these approximations to be valid are quite restrictive. In this complex context, most experimental works implicitly assume that the limiting step in the process is the reaction of the adsorbed species, and the concentration of adsorbed species is low. With these hypotheses, the approximate solution of the LH equation yields a first-order kinetics. However, verifying the validity of the hypothesis is mathematically complex and cumbersome.
In this work, we have made a detailed study of the mathematical description of the Langmuir–Hinshelwood equation, and we have been able to find a closed solution for it. From this solution, some numerical parameters which can act as indicators for identifying the custom regimes in terms of the experiment conditions have been derived, without the need of complex mathematical treatment. It is then a sort of discriminating tool that lets us easily decide which is the optimum approximation for the experimental conditions under study.
To test the validity of the proposed theoretical treatment, several experiments have been performed.
Section 2 of the paper details the experimental conditions used for the experiments that will be described in
Section 4.
Section 3 is devoted to the theoretical model. First, a summary of the LH approximations is given to establish the general context; then, the solution of the Lambert equation will be addressed.
2. Experimental Method
To check the validity of the analytical model, commercial powder samples of anatase (Aldrich Chemical Company (St. Louis, MO, USA), 1317-70-0) and zinc oxide (Sigma-Aldrich (St. Louis, MO, USA), #MKCL7155) have been used as catalysts, which are known for their good photocatalytic properties [
17,
18], and whose bandgap is around 3.2 eV at room temperature [
19,
20]. Commercial powder was directly added to the final solution, stirred by the vibrating plate, and aliquots were taken from the flask at different time intervals for each material. We used methylene blue (SigmaAldrich, CAS 122965-43-9) as pollutant. The photocatalysis reactor was homemade, open to air, and equipped with two commercial visible LED lamps (Brookes lamp (Grow The Jungle, Madrid, Spain), P = 35 W each one) and two commercial UV LED lamps (Mantis lamp (Grow The Jungle, Madrid, Spain), P = 25 W each one). Each UV lamp provides an illuminance of 4.5 mW/cm
2 at the position of the flask and each visible one provides 14 mW/cm
2. A simple scheme of the reactor is shown in
Figure 2a. The dissolution is placed in the middle of the reactor, on top of the magnetic stirrer. The UV and visible lamps are placed around the dissolution, each one pointing at the centre in a straight line. Both lamps, whose normalized spectra are shown in
Figure 2b, were used together during all the time in all experiments.
The test solutions used in this work are prepared from a parent solution of 10 mg of methylene blue (MB) in 100 mL of distilled water, having 100 ppm in volume (stock solution). Then, two different sets of experiments were performed. For the first one, we diluted 12.5 mL of stock solution into 500 mL of distilled water. This dissolution will have 2.5 ppm in volume (daughter solution) and will be tested with 2.5 mg of anatase or ZnO. For the second, we distilled 250 mL of this latter solution into 500 mL to decrease the concentration to half of the initial. This solution, having 1.25 ppm in volume (granddaughter solution), will be tested with 1.25 mg of anatase or ZnO.
Table 1 shows the sets used to check the validity of the model and assigns a number to each experiment to ease the discussion of results. A control experiment with MB dissolution and no samples under UV and visible light was also made to discard the influence of photolysis. To monitor the degradation, one aliquot was taken out from the reactor at different time intervals.
Figure 3 illustrates these procedures. In all experiments, the dissolution with catalysts was stirred for 30 min in darkness to achieve the absorption/desorption equilibrium, and was then magnetically stirred during all the irradiation time and irradiated under UV and visible light. The absorption spectra of the aliquots were performed with a Jasco V-770 spectrometer. Finally, the fittings were calculated with Matlab 2020a Optimization Toolbox.
3. Theoretical Study
The most common kinetic model used for the degradation of organic pollutants is the Langmuir–Hinshelwood equation (LH equation). This model describes the evolution of concentration of pollutants with time,
(mg L
−1), in terms of a differential equation [
16]:
In short, the starting point for simple decomposition reactions is
where A refers to the reactant and S to the active adsorption sites on the catalyst surface. Although the form of the reaction will depend on the process, at least one step is controlled by the adsorption on active sites.
Let us consider the simple reaction mentioned above in further detail. The catalytic reaction may be separated in three different reactions, each with its characteristic equilibrium constant,
for adsorption,
for desorption and
for the reaction that we want to activate. The ratio
is always positive, since it is defined as a quotient of powers of concentrations. The global reaction rate
r may be written as
where
: Concentration of adsorbate (mol/m
3);
: Surface concentration of occupied sites (mol/m
2);
: Surface concentration of total sites (occupied by adsorbate or not) (mol/m
2); and
: Surface coverage; fraction of occupied sites
. We have already mentioned the influence of the surface, according to this model, which can be quantified through
.
When the steady state is reached
Then
where the different terms refer to the different processes taking place:
, adsorption of adsorbates onto all sites;
, adsorption taking account that only empty sites are available for adsorption;
, reaction between adsorbate and sites; and
, desorption.
In terms of coverage
, we can rewrite the equation as
and
Considering that in steady state
Now we can describe two scenarios in terms of the limiting step.
If the limiting step is the adsorption
If the limiting step is the reaction of adsorbed species, and setting
(which is also positive as a quotient of positive ratios), we obtain the equation of Langmuir isotherms:
We can establish two regimes depending on the value of :
At low concentration, , , which is a first order reaction in .
At high concentration , , which does not depend on and, consequently, is a zeroth-order reaction in .
For our purposes, we would need a further refinement since our reaction is as follows:
To achieve the final products, a second adsorbate on a neighbouring site is necessary. Then, the reactions are as follows:
and finally
Now, adsorption and desorption must be considered for both species and the corresponding equilibrium constants will be
and
for A,
and
for B, and
for the reaction towards the final products, as in the simple Langmuir case. The reaction rate will be
Following the same reasoning as for the Langmuir isotherm:
where now we have introduced the fraction of empty sites,
so that
The probability that two adsorbates A and B adsorb on adjacent sites is low. Then, considering that the adsorption is the limiting step for the global reaction, it follows that
and
We can simplify this expression in two limiting cases.
and the reaction is of first order in both components.
- II.
If one of the components, let us say B, has a much lower adsorption:
and the reaction is of first order in A. For this rate, we can consider the low and high concentration limits for adsorbate A:
When , , which is a first-order reaction in
When , , which is a minus one order reaction in
The higher the A concentration is, the slower the reaction is, so A inhibits the reaction.
- c.
A third possibility is that one of the molecules has a much higher adsorption rate, let us say A:
The reaction now is of first order with respect to B and of minus one order respect to A, which can inhibit the reaction at any concentration.
The Langmuir–Hinshelwood kinetics is observed in many catalytic reactions as an example with an oxide as catalyst:
Further development of this model was made in 1938 by Ealy and Rideal, assuming that only one of the reactants adsorbs onto the catalyst, the second reacting directly from the gas (liquid) phase.
In that case, equilibrium constants will be
and
for A and
for the reaction towards the final products. As the second reacting species is commonly supposed to be saturated, the product
[
12,
13] is set equal to 1. In these conditions, the rate equation
is simplified to
which is formally identical to Langmuir isotherm Equation (9).
In a steady state and considering that the reaction is the limiting step
Since the second reacting does not play any role in this equation, the nomenclature of the terms can be simplified. The term
will be denoted by
; and
will be simplified to
. Finally, the Langmuir–Hinshelwood equation can be rewritten as follows:
where
(mg min
−1 L
−1) is the reaction constant,
is the adsorption constant of the reactant (L/mg) and
the reactant (pollutant) concentration.
Two standard approximations can be made:
And may be easily determined from the slope of the graph versus .
The main disadvantage of approximating in these ways is the impossibility of obtaining these two constants, ke and kapp, at the same time.
It has been customary to think that the LH solution has no closed form, which has forced us to work in only one of these regimes, or to use a semiempirical power rate equation [
15] to obtain a simple expression of the concentration. In the next section, we will show an analytical closed solution of the LH equation obtained in terms of the Lambert function. The main strengths of our model are that customary solutions of the zeroth- and first-order regime can be recovered, and new enhanced approximations depending on
ke and
kapp can be obtained, which would simplify the mathematical and computational treatment of the solution.
In this work, we will first show the solution of the LH equation (
Section 3.1 and
Section 3.2); then, in
Section 3.3, we will show how the zeroth- and first-order LH fits may be recovered from the general solution.
3.1. Solution of the LH Equation
Assuming that the concentration of pollutant is a continuous function, its derivative is also continuous for all
by virtue of the LH equation and the non-negativeness of
. Joining the initial condition, it can be checked that the function
satisfies the LH equation with initial condition
.
is the principal branch of the Lambert function. This is an analytical, monotone injective defined as the inverse of
[
21]. The plot of the Lambert function can be seen in
Figure 4 (black line).
From now on, we will make an abuse of notation, and we will refer to the principal branch of the Lambert function as the Lambert function. Lambert function is quite frequently found in physical processes as Wien displacement’s law or the travelling time of a falling body in a medium with friction [
21,
22,
23]. Also, the inverse of the Brillouin function, used in statistical mechanics to describe paramagnetism, is a particular example of a generalized Lambert function [
21].
3.2. Approximations of the LH Solution
First, recall that is a decreasing function of time (Equation (23)).
As the approximations of Equations (21) and (22) rely on the value of
versus 1, let us calculate the solution of the equation
. This value is the intersection of the green line of
Figure 1 with the Lambert function graph. The result is as follows:
This parameter will be called critical time. By introducing the concept of critical time, we can study the kinetic process purely in a time scale: the linear first-order condition is transformed into and the zeroth-order condition into .
It is important to highlight that t
c has time dimensions, but it is not a time in the physical sense, since it may have positive or negative values. A brief inspection of the expression used to define the critical time shows that
The meaning of an extremely negative critical time, , requires an additional explanation. If 0, then , which is the condition for the photocatalytic process taking place under the first-order regime. That is, the entire experiment occurs in the first-order regime, with no existence of any time interval for which the zeroth order could apply.
Table 2 summaries the mathematical formulation of the LH problem and its approximations yielding zeroth-order and first-order regimes, their respective solutions and the assumptions made to arrive at them.
After all, the solution described by the function is the generalization of the first-order or zeroth-order regime depending on the value of . The more we approach the assumptions validating a certain regime, the more the values of (for first order) and (for zeroth order) obtained from the general solution and the approximated solution should coincide, as they are the limit cases of it. A small relative error between these constants might be an indicator of how close we are to a particular regime, but the main test for ascribing an experiment to a regime should be the calculation of the critical time, as it is a direct translation of the value . Similarly, other nonphysical results, such as obtaining negative and ratios in a particular regime, would be indicative for discarding it.
3.2.1. First-Order Regime
In this case, the Lambert function (Equation (23)) and its argument can be replaced by their first-order Taylor series (
around
at a fixed time:
which is the solution of the first-order regime, as seen comparing this equation with Equation (21).
If we want a more accurate expression for the first-order regime, we could keep the first order of
Taylor series for
. This yields the following:
This fitting, which could be called the “enhanced first-order solution”, is much easier computationally than the adjustment of the general solution, and it permits the obtention of all ratios involved.
3.2.2. Zeroth-Order Regime
In the case of the zeroth-order regime,
As
then the argument of the Lambert function
The Lambert function W(x) is known to have an asymptotic series when
, whose first term is
[
20], then
As
and
, then
which corresponds to the zeroth-order solution of Equation (22).
As in the prior case, we could obtain a computationally powerful expression for this fitting. In the zeroth-order regime, whose solution is a linear tendency, small corrections could be enhanced by a quadratic term. As our solution is analytic, we could fit the data to the Taylor polynomial of second-order in
t of the function. It is known that the Taylor series of the quotient is as follows:
Fitting the data to the quadratic polynomial
, simple expressions for the parameters can be achieved:
This method, which could be seen as the “enhanced zeroth-order solution”, is extremely powerful, as it can drop the two parameters with a simple parabolic fitting.
Table 3 subsumes all the above approximations.
3.3. Numerical Treatment of the LH Solution
To link experimental data to the mathematical model, the Beer–Lambert law states that the concentration of pollutant,
, has a linear relationship with light absorption,
. Then, we can calculate the quotients of experimental absorption data and link them with the general closed solution:
This function describing the relative concentration (Equation (33)) has some mathematical subtleties which should be carefully considered. First, this quotient of concentrations can be adjusted to the following function, where
and
:
This function may encounter some problems due to the magnitude orders of
and
. The case of
, which is an apparent rate, is usually between 10
−3 and 10
−2 min
−1;
tends to be around 10
−1 L/mg, always depending on the characteristics of each experiment [
24,
25]. In particular, the main problem arises in the fitting of
, which is a minute value on the denominator. Therefore, small variations in
can affect fitting. This non-linear fitting should be solved with iterative algorithms, such as Levenberg–Marquandt [
26,
27,
28], in which the least squares problem would reduce the sum of residuals by approaching
and
to zero. Hence, special attention must be paid to avoid saturating the numerical minimization with the imposed lower boundaries.
Before going further, some considerations about the error determination are needed. As mentioned, the fitting parameters must be nearly close to zero in both cases, and the only physical restriction that the parameters have is that they must be positive. This poses an intrinsically ill-conditioned problem. Consequently, the errors associated with the fitted parameters cannot be calculated accurately. It is possible to estimate the errors of a fit using the variance–covariance matrix, which depends on the Jacobian matrix of the function evaluated at the fitted parameters [
26,
27,
28,
29]. However, they would not provide practical information for a confidence interval, as the derivative of the function would enlarge it considerably.
General results might be derived to set conditions for these boundaries [
27,
29], or to explore the implementation of modified least square methods, such as Ridge regression [
30]. However, such an elevated level of optimization is beyond the scope of this work. In our case, keeping in mind the above reasons during the mathematical treatment, we have set the lower boundaries at zero for both parameters, proving with several initial conditions until obtaining fitted parameters that did not saturate them.
Despite the complexity we have described, the solution we propose for the Lambert function has a major advantage that must be emphasized. Whereas the customary approximations of the LH equation can only find
kapp (from the first-order solution) or
kr (from the zeroth-order solution), with this method, both ratios are determined successively in one experiment. This eliminates the need for an additional isotherm to calculate the value of
Ke without [
31], or for multiple experiments where only one parameter varies to build a linear regression [
32,
33]. Hence, it is compulsory to tackle a deeper study of the quotient
in order to achieve simpler computational expressions, but without losing the main advantage of finding
and
simultaneously by solving the exact equation.
4. Validation of the Model with Experimental Results
At this point, it is not our aim to find the best experimental conditions and/or photocatalyst, but to validate the theorical model to consolidate it. The main virtue of this model is to rule out, mathematically, one regime or another, instead of assuming canonically that the experiment follows a particular regime, as is often recurrently seen in the literature. For that, the model has been tested with two sets of samples of commercial powder which have been commented on in the experimental method section: on the one hand, two experiments using different quantities of anatase as tester to degrade several MB dissolutions (experiments #1 and #2 of
Table 1), and two other identical experiments having the same mass of catalyst and concentration of MB dissolution, but using ZnO as catalyst (experiments #3 and #4). The idea of using these quantities is to provide two distinguishable scenarios: one showing a clear first-order degradation (anatase experiments), and the other showing that the data are not so easy to assign to a specific tendency, and therefore, there is a more delicate discussion regarding how to exploit the power of the model (ZnO experiments).
Photocatalysis experiments using powder as catalysts have been performed. Whatever the samples, the effectiveness of the photocatalysis is calculated from the degradation efficiency at a time
t, following Fernández-Calzado et al. [
34]:
Figure 5 shows the evolution of the quotient
. As seen, anatase degrades better than ZnO in all experiments having the same mass of catalyst and the same concentration of MB. Indeed, the experiments with anatase were ended before 120 min, since the dissolution had already been completely degraded. Using 2.5 mg of catalyst in a MB dissolution of 2.5 ppm in volume (
Figure 5a), anatase reached ~95% in 90 min, while ZnO reached ~32% in two hours. For the case of 1.25 mg of catalyst in a MB dissolution of 1.25 mg in volume (
Figure 5b), anatase nearly degraded completely (~99%), whereas the ZnO degradation efficiency, around ~40%, is considerably lower than of anatase. The control experiment, performed to monitor the degradation efficiency of the photolysis, has given an efficiency of ~13% and a degradation ratio is
min
−1. From what we can conclude, the photolysis effect does not play the main role in the experiments. In addition, the tendency of degradation of anatase experiments is quite like an exponential decay, which would correspond to first-order degradation. Conversely, ZnO degradation does not have such a recognizable tendency to decay.
To deepen into the kinetic study, several fittings have been performed to all experiments. The fittings having been performed, a quantitative indicator of the goodness of fit is the determination coefficient, R
2, which is a canonical tool in regression analysis. A R
2 coefficient close to 1 evidences the fact that the model explains the data accurately. If
represents the experimental data,
the fitted data, and
the mean of the data, the determination coefficient is calculated as follows [
29]:
Anatase experiments will be studied first.
Figure 6 shows the fitting of experiments #1 and #2 to the previously derived functions: Lambert fit, zeroth-order fit, first-order fit, enhanced zeroth-order fit and enhanced first-order fit.
Table 4 shows the parameters obtained from these calculations.
Figure 6a shows the kinetic study for experiment #1 (2.5 mg of anatase in MB solution having 2.5 ppm in volume), and
Figure 6b shows that of experiment #2 (1.25 mg of anatase in MB solution having 1.25 ppm in volume). As seen, the first order does not describe the data completely, since
R2 = 0.81. While this value is not bad, is not as good as we would like. Instead, the Lambert fitting, which fits the data to the analytical real solution, describes the data accurately. This visual fact is supported by a R
2 = 0.95, which proves quantitatively the suitability of the model. Furthermore, the enhanced first-order fitting completely overlaps with this Lambert fit and has its same R
2. This means that, in this case, the first-order enhanced solutions, which is an exponential-like fit and mathematically simpler than the Lambert fit, describes the data just as well as the Lambert fit. This reasoning highlights the advantages of the derivation of these enhanced approximations: as well as describing the data better than the traditional first-order approach, it enables the two fit constants to be fitted at the same time. Indeed, enhanced first-order fitting is better than the Lambert fit because it yields values of
and
in consonance with the literature [
24,
25], whereas the Lambert parameters seem unrealistic. This is due to the fact that the pure Lambert fit is an ill-conditioned problem, which could give mathematically accurate and unphysical results. On the other hand, enhanced first-order fitting has a simpler expression, so its results are physically more reliable than the prior ones. Nevertheless, the Lambert fit is essential to derive these powerful approximations. Furthermore, the negative critical time also supports the fact of performing the experiment perpetually throughout the first-order regime. At the same time, the first order is assessed since the zeroth order can be completely discarded for several reasons: their R
2 coefficients are poorer than those of the first order; they do not describe well the evolution of the data; and negative K
e and
kr ratios are derived by the enhanced zeroth-order fitting, which has no physical meaning, and sometimes
C/
C0 < 0, which also makes no physical sense.
Now, let us turn to the ZnO kinetics.
Figure 7a shows the results and fittings of experiment #3 (2.5 mg of ZnO in MB solution having 2.5 ppm in volume), and
Figure 7b those of experiment #4 (1.25 mg of ZnO in MB solution having 1.25 ppm in volume). The results appear in
Table 5. Unlike anatase experiments, the tendency of the data is not so clear, as all the fittings overlap. For this reason, it is necessary to make a detailed discussion instead of assuming first-order degradation carelessly, especially when all R
2 values are quite close to each other. Firstly, the inspection of the kinetic ratios obtained for the zeroth order reveals that they are negative, which rules out this degradation regime. In addition, the negative critical time also hints at first-order degradation. For these reasons, the first-order degradation is established by discarding the zeroth-order regime. As in the prior case, the constants obtained by the enhanced fitting have more physical meaning than those obtained by the Lambert function. Finally, we might conclude that this first-order degradation is weaker than that observed in anatase experiments (
Figure 6), since the overlap of all fittings attenuates the evidence for a clear first-order degradation. Further analyses are required to fully elucidate this behaviour; however, it seems plausible that it is related to the reduced adsorption sites.