The adsorption of gases and solutes is usually described through isotherms, that is, the amount of adsorbate on the adsorbent as a function of its pressure (if gas) or concentration (for liquid phase solutes) at constant temperature. The quantity adsorbed is nearly always normalized by the mass of the adsorbent to allow comparison of different materials. A number of different isotherm models have been developed.
Freundlich The first mathematical fit to an isotherm was published by Freundlich and Kuster (1906) and is a purely empirical formula for gaseous adsorbates: :\frac{x}{m} = kP^{1/n}, where x is the mass of adsorbate adsorbed, m is the mass of the adsorbent, P is the pressure of adsorbate (this can be changed to concentration if investigating solution rather than gas), and k and n are empirical constants for each adsorbent–adsorbate pair at a given temperature. The function is not adequate at very high pressure because in reality x/m has an asymptotic maximum as pressure increases without bound. As the temperature increases, the constants k and n change to reflect the empirical observation that the quantity adsorbed rises more slowly and higher pressures are required to saturate the surface.
Langmuir Irving Langmuir was the first to derive a scientifically based adsorption isotherm in 1918. While the Langmuir model assumes that the energy of adsorption remains constant with surface occupancy, the Freundlich equation is derived with the assumption that the heat of adsorption continually decrease as the binding sites are occupied. The choice of the model based on best fitting of the data is a common misconception. To compensate for the increased probability of adsorption occurring around molecules present on the substrate surface, Kisliuk developed the precursor state theory, whereby molecules would enter a precursor state at the interface between the solid adsorbent and adsorbate in the gaseous phase. From here, adsorbate molecules would either adsorb to the adsorbent or desorb into the gaseous phase. The probability of adsorption occurring from the precursor state is dependent on the adsorbate's proximity to other adsorbate molecules that have already been adsorbed. If the adsorbate molecule in the precursor state is in close proximity to an adsorbate molecule that has already formed on the surface, it has a sticking probability reflected by the size of the SE constant and will either be adsorbed from the precursor state at a rate of
kEC or will desorb into the gaseous phase at a rate of
kES. If an adsorbate molecule enters the precursor state at a location that is remote from any other previously adsorbed adsorbate molecules, the sticking probability is reflected by the size of the SD constant. These factors were included as part of a single constant termed a "sticking coefficient",
kE, described below: :k_\text{E} = \frac{S_\text{E}}{k_\text{ES} S_\text{D}}. As SD is dictated by factors that are taken into account by the Langmuir model, SD can be assumed to be the adsorption rate constant. However, the rate constant for the Kisliuk model (
R') is different from that of the Langmuir model, as
R' is used to represent the impact of diffusion on monolayer formation and is proportional to the square root of the system's diffusion coefficient. The Kisliuk adsorption isotherm is written as follows, where θ(
t) is fractional coverage of the adsorbent with adsorbate, and
t is immersion time: :\frac{d\theta_{(t)}}{dt} = R'(1 - \theta)(1 + k_\text{E}\theta). Solving for θ(
t) yields: :\theta_{(t)} = \frac{1 - e^{-R'(1 + k_\text{E})t}}{1 + k_\text{E} e^{-R'(1 + k_\text{E})t}}.
Adsorption enthalpy Adsorption constants are
equilibrium constants, therefore they obey the
Van 't Hoff equation: :\left( \frac{\partial \ln K}{\partial \frac{1}{T}} \right)_\theta = -\frac{\Delta H}{R}. As can be seen in the formula, the variation of
K must be isosteric, that is, at constant coverage. If we start from the BET isotherm and assume that the entropy change is the same for liquefaction and adsorption, we obtain :\Delta H_\text{ads} = \Delta H_\text{liq} - RT\ln c, that is to say, adsorption is more exothermic than liquefaction.
Single-molecule explanation The adsorption of ensemble molecules on a surface or interface can be divided into two processes: adsorption and desorption. If the adsorption rate wins the desorption rate, the molecules will accumulate over time giving the adsorption curve over time. If the desorption rate is larger, the number of molecules on the surface will decrease over time. The adsorption rate is dependent on the temperature, the diffusion rate of the solute (related to
mean free path for pure gas), and the
energy barrier between the molecule and the surface. The diffusion and key elements of the adsorption rate can be calculated using
Fick's laws of diffusion and the
Einstein relation (kinetic theory). Under ideal conditions, when there is no energy barrier and all molecules that diffuse and collide with the surface get adsorbed, the number of molecules adsorbed \Gamma at a surface of area A on an infinite area surface can be directly integrated from
Fick's second law differential equation to be: :\Gamma = 2AC\sqrt{\frac{Dt}{\pi}} where A is the surface area (unit m2), C is the number concentration of the molecule in the bulk solution (unit #/m3), D is the diffusion constant (unit m2/s), and t is time (unit s). Further simulations and analysis of this equation show that the square root dependence on the time is originated from the decrease of the concentrations near the surface under ideal adsorption conditions. Also, this equation only works for the beginning of the adsorption when a well-behaved concentration gradient forms near the surface. Correction on the reduction of the adsorption area and slowing down of the concentration gradient evolution have to be considered over a longer time. Under real experimental conditions, the flow and the small adsorption area always make the adsorption rate faster than what this equation predicted, and the energy barrier will either accelerate this rate by surface attraction or slow it down by surface repulsion. Thus, the prediction from this equation is often a few to several orders of magnitude away from the experimental results. Under special cases, such as a very small adsorption area on a large surface, and under
chemical equilibrium when there is no concentration gradience near the surface, this equation becomes useful to predict the adsorption rate with debatable special care to determine a specific value of t in a particular measurement. The desorption of a molecule from the surface depends on the binding energy of the molecule to the surface and the temperature. The typical overall adsorption rate is thus often a combined result of the adsorption and desorption. ==Quantum mechanical – thermodynamic modelling for surface area and porosity==