The adsorption models developed from statistical physics face significant limitations that affect their practical applications. Many models are based on simplified assumptions about surface homogeneity, the accessibility of adsorption sites, and interactions between the adsorbent and the adsorbate, but real adsorbents exhibit complex characteristics, including varying pore sizes and heterogeneous surfaces. The fitted parameters, such as the aggregation number or adsorption energy, lack unambiguous physical interpretations and require validation through independent experiments. The majority of current research focuses on single-solute systems, thereby neglecting the complexity of real wastewater, which contains multiple pollutants and factors such as pH and temperature that influence adsorption behavior. The lack of validation under realistic steady-state flow conditions further undermines the reliability of the models. Refining these models can advance both fundamental science and environmental remediation, particularly when integrated with the design of advanced materials and molecular simulations. Future research should extend the models to multicomponent systems to better reflect complex pollutant mixtures and incorporate machine learning.
It is essential to strengthen the relationships among theoretical modeling, computational simulations, and process technology to translate statistical-physics-derived adsorption models into solutions for large-scale environmental treatment. The establishment of accurate predictive models requires systematic validation and their application in practical contexts.
Statistical physics modeling
Classical isotherms, including the Freundlich, Langmuir, and Redlich-Peterson equations, are routinely applied to equilibrium adsorption data but offer limited mechanistic insight and fail to clarify phenomena at the molecular scale due to their specific assumptions17. They provide only qualitative indications of surface uniformity or adsorbate interactions and cannot determine essential parameters such as site occupancy, adsorption energies, or layer numbers. To address these shortcomings, statistical physics has been introduced as a powerful theoretical framework that provides physically meaningful parameters18. This formalism relies on key assumptions: adsorbate-adsorbate interactions are initially neglected via an ideal-gas approximation valid at low concentrations19,20, while a real-gas model becomes necessary at higher concentrations to account for lateral interactions21. Interactions with water and most rotational, vibrational, and electronic degrees of freedom are typically omitted, making translation the dominant contribution22,23,24,25,26. In this context, adsorbent sites with characteristic energy ε accommodate variable particle numbers, and adsorption is viewed as particle transfer from the liquid reservoir to the surface, justifying the use of the grand canonical ensemble20,27. The partition function depends critically on adsorption energy (−ε) and chemical potential (μ)28,29,30. The complete mathematical derivation of these statistical physics models is thoroughly presented in Supplementary File 1. Furthermore, Figure 3 provides a visual roadmap, illustrating the progression from foundational system assumptions through the grand canonical ensemble and partition function to the development of specific models for monolayer, multilayer, single-solute, and multicomponent adsorption. Finally, the adjusted parameters from these models provide molecular-level and thermodynamic information, enabling a comprehensive interpretation of the adsorption mechanisms and surface heterogeneity.
Models for single adsorption systems
The single-energy monolayer model describes adsorption with one layer and energy (−ε), allowing variable adsorbate particle numbers n18,35. The partition function for one site is:
(1)
Two site states contribute to this partition function. The term 1 denotes an empty adsorption site, while eβ(ε+μ) denotes a site occupied by adsorbed species. The mean number of occupied adsorption sites, N0, is calculated as26:
(2)
The uptake as a function of concentration is given by:
(3)
C1/2 is the half-saturation concentration, C is the equilibrium concentration, and NM is the site density. For n=1, it resembles Langmuir; at low concentration, it approaches Freundlich26. At saturation, the amount retained is37:
(4)
The surface configuration expected for this model is shown in Figure 4A.
Single-layer model with dual energies
The two-energy monolayer model describes adsorption on two distinct site categories. Each category has its own adsorption energy, (−ε1) or (−ε2), and its own density of equivalent sites, NM1 or NM2. The number of ions or molecules hosted by each site category may differ and is represented by n1 and n218,22,35. The corresponding grand canonical partition functions are26:
(5)
(6)
The mean number of occupied adsorption sites is then written as:
(7)
The equilibrium uptake is related to concentration by17:
(8)
where C1 and C2 denote the half-saturation concentrations corresponding to the first and second site categories. The arrangement associated with this two-energy monolayer model is illustrated in Figure 4B.
Model with two layers and a single energy
In the single-energy double-layer model, the adsorbate is distributed over two adsorbed layers, both represented by the same adsorption energy ((−εi)22,35 (Figure 4C). For this arrangement, the grand canonical partition function is 17:
(9)
The total mean number of occupied adsorption sites is obtained from:
(10)
The amount adsorbed as a concentration-dependent quantity is given by38:
(11)
Two-energy double-layer model
The two-energy double-layer model represents ion or molecule adsorption over two layers, with different adsorption energies assigned to the first and second layers, (−ε1) and (−ε2), respectively, where |ε1| > |ε2|18,22,35. Under this assumption, the grand canonical partition function is:
(12)
The mean number of occupied adsorption sites, N0, is obtained from:
(13)
The adsorbed quantity can therefore be expressed as:
(14)
where C1 and C2 are the half-saturation concentrations for the first and second layers, respectively. Figure 4D shows the adsorbate distribution predicted by this model.
Three-layer model with a single energy
In the three-layer model with a single energy, adsorption produces three layers on the adsorbent surface, all described by a single adsorption energy (−εi) (Figure 4E). The associated grand canonical partition function is27:
(15)
The average number of occupied adsorption sites is obtained from:
(16)
The adsorbed amount is determined using39:
(17)
Multi-layer model with two energies
In the two-energy multilayer model, the first layer, L1, arises from direct interactions between adsorbate species and the adsorbent surface and is associated with the adsorption energy (−ε1). The following layers, L2, are associated with adsorption energy (−ε2), with |ε1| > |ε2| > 017,18,40. With this assumption, the grand canonical partition function is19,41:
(18)
The amount retained in the solid phase is calculated from41:
(19)
With
(20)
(21)
(22)
where C1 and C2 denote the half-saturation concentrations associated with layers L1 and L2, respectively. The overall number of layers is LT = L1 + L2. Under saturation conditions, the amount adsorbed on the adsorbent surface is42:
(23)
The generation of L1 and L2 layers in this multilayer model is represented schematically in Figure 4F.
Infinite multilayer framework with three energy levels
The three-energy infinite multilayer model assumes that the first fraction of adsorbate is fixed directly on adsorption sites, generating layer L1 with adsorption energy (−ε1). A second layer, L2, is then formed with adsorption energy (−ε2), whereas the remaining adsorbate contributes to an unlimited set of L3 layers described by energy (−ε3). The energy sequence follows |ε1| > |ε2| > |ε3| 43. The corresponding grand canonical partition function is43:
(24)
The equilibrium uptake as a function of concentration is43:
(25)
With
(26)
(27)
(28)
(29)
where C1, C2, and C3 are the half-saturation concentrations for L1, L2, and L3, respectively. Figure 4G shows the infinite multilayer arrangement produced through the intermediate L2 layer.
Finite multilayer model
The finite multilayer model assumes that the first adsorbate layer forms through interaction with the adsorbent surface with adsorption energy (−ε1). The second layer interacts with the first layer through adsorption energy (−ε2). Further layers are represented by the adsorption energy assigned to La, where La is the average number of layers35,44,45. Under these assumptions, the grand canonical partition function is:
(30)
For this model, the adsorbed amount as a function of equilibrium concentration is obtained from44:
(31)
where C1 and C2 are the half-saturation concentrations for layers L1 and La, respectively. The distribution of adsorbed species predicted by this model is presented in Figure 4H.
Models for binary adsorption systems
Competing single-layer model
The competitive monolayer model describes two solutes, A and B, competing for the same adsorption site27, where each filled site holds either A or B.
(32)
where the occupancy variables describe adsorption sites filled by A and B, while μ1 and μ2 are the chemical potentials of A and B, respectively. The mean number of occupied sites associated with A (
) and B (
) are27:
(33)
(34)
At equilibrium, the adsorbed amounts of A and B are27,45,46:
(35)
(36)
n1 and n2 are adsorbed A and B molecules; C1, C2 are their equilibrium concentrations, with C01 and C02 as half-saturation concentrations. The arrangement of the two adsorbates on the solid surface is depicted in Figure 5A.
Expanded Hill model
The extended Hill model represents an adsorbent surface containing two different site classes. Their densities are NM1 and NM2, and their adsorption energies are (−ε1) and (−ε2), respectively. The grand canonical partition functions for these site classes are17,22:
(37)
(38)
The mean number of occupied sites in each class is calculated as:
(39)
(40)
For each adsorption-site class, equilibrium uptake as a function of concentration is therefore:
(41)
(42)
Figure 5B shows the distribution of adsorbate species on the solid surface according to the extended Hill model.
Models for ternary adsorption systems
Ternary adsorption model for identical adsorption sites
A ternary model includes identical adsorption sites in a liquid phase with three species and an NM adsorbent density47,48:
(43)
The average amount for each occupied-site class is written as47,48:
(44)
(45)
(46)
At equilibrium, the amount retained by each species as a function of concentration is48:
(47)
(48)
(49)
n1, n2, n3 are adsorbed A, B, C molecules; C1, C2, C3 are equilibrium concentrations; C01, C02, C03 are half-saturation concentrations. The arrangement predicted by the ternary model with identical adsorption sites is shown in Figure 5C.
Ternary adsorption model for specific adsorption sites.
The ternary model includes three adsorbed species, A, B, and C, at specific sites, allowing for independent or competitive retention during adsorption48.
(50)
(51)
(52)
For each site class, the mean number of occupied sites is:
(53)
(54)
(55)
At equilibrium, the concentration-dependent amount retained by each species on its corresponding site class i 48:
(56)
(57)
(58)
Models for Quaternary adsorption systems
Quaternary adsorption model for identical adsorption sites
The quaternary model can be applied in cases when there are four species in the liquid, all with identical adsorption sites and the same density NM at the adsorbent (Figure 5E). The formulation uses one adsorption energy and is written as49:
(59)
The average amount associated with each class of occupied site is49:
(60)
(61)
(62)
(63)
At equilibrium, the concentration-dependent amount of each species fixed at the adsorption sites is49:
(64)
(65)
(66)
(67)
Where n1, n2, n3, and n4 are the numbers of A, B, C, and D molecules adsorbed on one site, respectively. C1, C2, C3, and C4 are their equilibrium concentrations. C01, C02, C03, and C04 denote the half-saturation concentrations of A, B, C, and D. Figure 5E shows the adsorbate arrangement expected for the quaternary model with identical adsorption sites.
Quaternary adsorption model for specific adsorption sites.
The quaternary model considers four adsorbed species (A, B, C, D), which interact with each other independently or competitively at various adsorption site types49.
(68)
(69)
(70)
(71)
For each site class, the mean number of occupied sites is:
(72)
(73)
(74)
(75)
At equilibrium, the concentration-dependent amount retained by each species on its corresponding site class is48:
(76)
(77)
(78)
(79)
Advanced Statistical Physics Frameworks
The advanced statistical physics approach includes the real-gas chemical potential in the adsorption equations, accounting for adsorbate interactions and improving adsorption modeling by incorporating lateral effects.
Advanced monolayer model with one energy49,50:
(80)
Advanced monolayer model with two energy states50:
(81)
Advanced double-layer model49:
(82)
Advanced multilayer model with two energies49:
(83)
Advanced finite multilayer model51:
(84)
(85)
(86)
Numerical fitting methods
The significance of an adsorption-at-equilibrium model is evaluated by comparing it with experimental adsorption values and those predicted by a fitted equation, which requires parameter optimization to minimize deviations. A good fit is indicated by a coefficient of determination close to one (R2 ≈ 1) and by low residual error measures (SSE, ARE, SAE, RMSE)52,53,54,55,56,57,58,59,60,61,62,63,64,65,66 (Table 1). Two optimization methods are used: the sum of normalized errors (SNE) with Excel Solver, and nonlinear least-squares regression using the Levenberg-Marquardt algorithm, usually in Origin software61,62,63,64,65,66.
(87)
The aim of this work is to minimize the gap between experimental and calculated adsorption capacities, often by minimizing SSE. The LM algorithm is useful for nonlinear equations because it combines the Gauss-Newton and gradient descent methods. The selection of an optimization algorithm requires consideration of the model's form, the number of parameters, and the initial values. The important parameters include parameter bounds and convergence checks. The evaluation of a model's reliability requires consideration of R2, residual errors, complexity, behavior, and feasibility, not just R2.
Thermodynamic properties
The adsorption process is characterized using thermodynamic functions related to disorder and spontaneity, derived from the grand-canonical partition function at the molecular scale. These functions provide a more complete description of microscopic states and allow calculation of free enthalpy, internal energy, and entropy17,22,63,67,68,69,70,71,72,73. Specifically, the single-layer, double-layer, and multilayer models define the configuration entropy (Sad), Gibbs free energy (Gad), and internal energy (Eint), thereby revealing the interactions between adsorbates and receptor sites. The corresponding analytical expressions are given in the equations of Supplementary Table 1.
Isosteric enthalpy
The isosteric heat of adsorption highlights the heterogeneities in surface energy and allows the interactions between adsorbates to be measured; a fixed quantity of material adsorbed at two temperatures facilitates calculation using the Clausius-Clapeyron equation57,67.
(88)
In this expression, C denotes the equilibrium adsorbate concentration at temperature T (K) for a specified adsorbed loading Qa, and R is the universal gas constant, 8.3144598 m2.kg.s−2.K−1.mol−1. Sips 68 also proposed the following expression for determining the isosteric heat:
(89)
The value of Qst can be derived from the slope of the ln(C) versus 1/T curve at a constant charge or from the best-fitting adsorption isotherm67. Therefore, the detailed thermodynamic functions are available in the Supplementary Table 1.
Entropy
The entropy measures the configurational disorder in an adsorption system. It can be calculated using equations from statistical physics based on the model parameters63,72,74:
(90)
(91)
Combining these relationships gives the entropy in the form:
(92)
At low adsorbate concentrations, entropy increases prior to half-saturation due to the available configurations31. Close to C1/2, a high site occupation rate maximizes entropy, but after this value, the decrease in the number of vacant sites reduces the number of possible molecular configurations, leading to a decrease in entropy toward zero at saturation70.
Gibbs free energy
The free enthalpy, used to evaluate whether adsorption is spontaneous and feasible, is generally expressed as74,75,76,77,78,79:
(93)
The corresponding chemical potential is written as:
(94)
At a fixed temperature, negative values of free enthalpy indicate a thermodynamically favorable removal of the adsorbed species.
Internal energy
Internal energy accounts for the energetic contributions associated with uptake of the transferred species and is expressed as72,73,74,75,76,78,79,80:
(95)
Negative internal energy is consistent with spontaneous retention of the species by the adsorbent surface. From the grand canonical partition function, the thermodynamic functions considered in this section are therefore obtained as follows:
Site energy distribution
The energy distribution per site (SED) provides a correlation between equilibrium parameters and the energy heterogeneity of adsorbents, indicating variations in energy per site F(ε) and interactions with solutes θt(ε,C)81:
(96)
Here, ε represents the energetic difference between the adsorption of the solute and the adsorption of the solvent at a given site. The direct solution of this integral is not straightforward. For this reason, Cerofolini introduced the condensation approximation82, in which adsorption on low-energy sites is considered negligible (θt(ε,C) = 0), whereas adsorption on high-energy sites is considered complete (θt(ε,C) = 1). Under this assumption, the lower limit of integration is replaced by a concentration-dependent threshold energy ε*81,83,84,85:
(97)
In this equation, Cs is the adsorbate maximum solubility in the solvent, εs denotes the minimum accessible adsorption energy associated with Ce = Cs, R is the ideal gas constant, T is the absolute temperature, and C is the standard adsorbate concentration in the liquid phase. The exponent m describes surface heterogeneity and is obtained from the Freundlich model, which is frequently used to construct the SED for heterogeneous adsorbents82,83,84,85.
(98)
The integral in Eq. 93 corresponds to the area below the SED curve and is equal to the saturation adsorption capacity, Qsat36,86:
(99)
When the SED profile contains a maximum, defined by ε*m and F(ε*m), the surface can be interpreted as containing sites of different energetic classes. Sites with ε* > ε*m are considered high-energy sites, whereas those with ε* < ε*m are considered low-energy sites. The energy associated with the maximum is given by:
(100)
The SED profile also provides the relative abundance of adsorption sites at a given energy. The spread of this profile, referred to as the site-energy variability of the adsorbent, σe*, represents the distribution width and is calculated as:
(101)
With
(102)
(103)
In these expressions, EP(ε*) is the expectation value of ε* and corresponds to the mean adsorption-site energy for a specific adsorbate87, whereas EP(ε*2) is the expectation value of ε*2. The critical energies ε*1 and ε*2 delimit the interval over which the SED is evaluated. When the distribution is Gaussian, σe* is equivalent to the standard deviation. Joint analysis of σe* and EP(ε*) therefore supports evaluation of surface energetic heterogeneity and identification of the energy domain most favorable for adsorbate retention.
The mean SED, EP(ε*), also reflects the strength of adsorbate-surface association. Larger EP(ε*) values indicate stronger adsorbent-adsorbate affinity and, consequently, a more favorable uptake process. After adsorption, variations in EP(ε*) describe how adsorbate molecules are redistributed among sites of different energies and help delimit the energy interval responsible for the most efficient retention.
Utilization of statistical mechanics in the adsorption phenomenon
The field of statistical physics supports research on adsorption by establishing a relation between the equilibrium isotherms and the microscopic properties, which makes it possible to obtain steric and energetic parameters that describe the adsorption mechanism at the molecular level, the site density, the number of adsorbed species, the layers, and the adsorption energy19,22.
Steric characteristics
The steric parameters highlight the interactions and arrangement of species adsorbed on surfaces, which affect the interpretation of the adsorption equilibrium.
Parameter n
The parameter n denotes the number of adsorbed species bound by an adsorption site at the equilibrium state. It indicates the molecular orientation and the mode of attachment, and is also termed the aggregation parameter. Below 1: A single adsorbate is distributed over more than one adsorption site, with no clustering. This situation is assigned to a multi-anchorage mechanism88,89,90. The functional groups of the adsorbates are attached to distinct sites, making both horizontal and parallel adsorption possible91. Equal to 1: One adsorbate species is associated with one adsorption site. This configuration is generally interpreted as non-parallel orientation, mono-adsorbate retention, and monomer formation92,93. Greater than 1: Several adsorbate species are retained by the same site, usually in inclined or perpendicular arrangements. This condition may generate 2-aggregated (n = 2), 3-aggregated (n = 3), or 4-aggregated (n = 4) species 17, indicating that adsorption proceeds through a multi-adsorbate mechanism22,93.
Parameter NM
NM denotes the density of occupied adsorption sites per unit mass of adsorbent91. It is inverse to n; values of n that are high reduce the number of accessible sites due to aggregation, while values of n that are low increase the availability of sites, which affects adsorption capacity92.
Number of layers formed
The number of adsorbed molecules is a steric parameter governed by steric hindrance and adsorbate-adsorbent/adsorbate-adsorbate interactions. Sellaoui et al.17 attributed the limited number of ibuprofen layers to pore-related constraints, while Yazidi et al.19 attributed the differences in the number of layers to intermolecular interactions. Atrous et al.17 reported 2.349 layers for Acid Red 1 on clay, applying the equation 2.349 = 2×y + 3×(1−y) to obtain the following fractions: 65.1% double layers and 32.9% triple layers. The concept of "layer-by-layer" (LBL) describes adsorption driven by electrostatic charge compensation, with alternating layers of cations and anions (double layer, finite or infinite multilayer), as shown in Figure 663,94,95. Ben Yahia et al.62 demonstrated the formation of such an alternating Mg2+/NO3- multilayer on porphyrin, although higher temperatures and reduced surface effects limited its growth.
Parameter Qsat
The Qsat, a steric parameter governed by several steric factors, is related to the number of species per site, the site density, and/or the number of layers in the best-fit model, making it useful for comparing adsorbent performance. In binary adsorption, the interactions between species A and B are inferred by comparing the binary Qsat to the value associated with a single solution, with three extreme cases taken into calculation27. If Qsat is lower in the binary system than in the single-solute system, species A and B compete and mutually reduce adsorption. If Qsat is higher in the binary system, the presence of B enhances retention of A, and the reciprocal effect may also occur. If Qsat is unchanged, no significant interaction between A and B is detected.
Energetic parameter
The adsorption energy is the primary characteristic used to describe interactions, affinity, and mechanism65. The values below 40 kJ·mol-1 indicate physisorption (van der Waals, hydrophobic, electrostatic, etc.), while values above 80 kJ·mol-1 indicate chemisorption91,96. The negative and positive signs denote exothermic and endothermic processes, respectively91. The first layer has a stronger binding than the other layers, so that |the first layer's energy| exceeds that of the subsequent layers19,28,88,96,97.
Van der Waals coefficients
In advanced statistical physics models that describe solutions as real gases, the Van der Waals coefficients (cohesion pressure and co-volume b) reflect lateral interactions between adsorbates and help explain the reductions in adsorption after saturation98,99,100. A higher value of a indicates a stronger attraction, which weakens the bond between the adsorbate and the site and promotes solution retention, thereby reducing adsorption52. In contrast, a higher value of b increases the distance between particles, thereby promoting adsorption101. The effects of temperature depend on the system: Souissi et al.23 found that higher temperatures reduced a (weaker attraction) and increased b (increased repulsion), thereby favoring the adsorption of silver ions onto hexahelicene (an endothermic process). In comparison, Alyousef et al.15 observed a higher value of a at high temperatures, suggesting stronger lateral interactions that hindered water vapor adsorption on date pits (an exothermic process).
Recent studies on adsorption isotherm calculations using statistical physics models.
Organic pollutants: Dyes and pharmaceuticals
Statistical physics models have become essential for interpreting equilibrium adsorption data, with Table 2, the result of maximum adsorption capacities and fitted parameters for dye/adsorbent systems.
An important study of dyes has shown that temperature increases site density and saturation capacity (Qsat) while confirming physisorption mechanisms64,97,102. The inverse relationship between molecules per site (n) and site density (NM) revealed that higher n increases steric hindrance, reducing accessible sites64. Real-gas monolayer models enabled isosteric heat analysis, identifying three concentration regions that reflect molecular interactions51.
For pharmaceuticals, single-solute systems followed the two-energy double-layer model, while ternary systems required designated-site models (Table 3)103,104. Diclofenac showed dimer formation (n varies from 1.13 to 2.06), while acetaminophen aggregation decreased with temperature103. Norfloxacin on graphene oxide revealed two site classes: 59% monomers/41% dimers at primary sites and 88% monomers/11% dimers at secondary sites105. Binary systems showed competitive exothermic physisorption106 and antagonistic effects from site competition107. Additional studies on activated carbons, modified clays, and biochars confirmed multimolecular physisorption108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125, with energies below 40 kJ·mol-1 confirming physisorption91,96. Negative values indicated exothermic processes while positive values indicated endothermic behavior. First-layer energies consistently exceeded subsequent layers due to stronger direct site binding19,28,88,96,97. For pharmaceutical systems, adsorption energies of ΔE1 = 12.73 kJ·mol-1 and ΔE2=18.85 kJ·mol-1 confirmed physical adsorption, suggesting feasible adsorbent regeneration. Statistical physics has proven essential for interpreting molecular orientations, aggregation states, interaction energies, and thermodynamic parameters across diverse adsorbate-adsorbent systems.
Inorganic pollutants and heavy metals
Pollution from heavy metals in industrial activities (such as tanning, mineral extraction, galvanoplasty, paint, and heating element production) releases toxic metal ions into water, harming ecosystems and organisms. Adsorption modeling using isotherms is an essential tool for evaluating removal performance126 (Table 4).
The entropy profiles of Ni(II) on four biosorbents showed two maxima at C1 and C2, corresponding to the first and second adsorbed layers, respectively. Three regimes were identified for each layer: (i) C < Ci: entropy increased due to the abundance of vacant sites allowing greater ion mobility; (ii) C = Ci: entropy reached a maximum, indicating the highest probability of adsorption; (iii) C > Ci: entropy decreased as the progressive occupation of sites restricted movement and reduced disorder. Ben Yahia et al.103 studied Ag+ species (silver chloride, silver nitrate, silver sulfide) on hexahelicene using QCM isotherms. The type of adsorbate governed the interactions, with higher temperatures favoring binding (endothermic adsorption). The silver chloride exhibited the strongest adsorption with stable saturation, which could be successfully fitted using the advanced single-layer model based on the ideal gas approach127,128,129,130.
Multicomponent and competitive adsorption systems
For AgNO3, descending isotherms indicated unstable saturation due to strong lateral interactions in solution competing with surface binding (Table 4). Dotto et al.130 studied Ni(II) on four biosorbents using the two-energy double-layer model; temperature increased aggregation (n) but decreased capacity, confirming exothermic physisorption, with surface interactions stronger than Ni(II)-Ni(II) interactions. Ben Yahia et al.103 found Ag2S showed the lowest n values due to sulfur-layer interference.
Selim et al.22 examined Cu2+/Zn2+ on cancrinite; in binary systems, both capacities decreased with nCu2+>nZn2+ and higher adsorption energy for Cu2+, confirming antagonism with spontaneous endothermic behavior. Sellaoui et al.48 evaluated ternary Cu2+, Cd2+, and Zn2+ on bone char; Cu2+ uptake was highest and unaffected by the other ions, whereas Cd2+ and Zn2+ showed parallel orientations, with Cu2+ showing non-parallel alignment. Quaternary adsorption on sludge-derived adsorbent49 showed endothermic behavior for Cu2+, Co2+, Ni2+, but exothermic for Ag+.