Thursday, August 29, 2019

thermodynamics - Why can't a reaction go to completion?


What is the reason for why an exergonic reaction would still have some remaining reactants (or an endergonic reaction to have any products)? The explanation given on this page (see Chemical reactions and mixing) is that there is a Gibbs free energy change caused by the entropy change by mixing; therefore, it is always energetically favorable to have at least some of each.


At another page (see Dissociation of weak acids) on the site, the explanation as to why weak acids (with positive ΔG for reaction with water) dissociate at all seems to be that some molecules do have the energy required for the reaction, analogous to molecules overcoming activation energy in the context of kinetics.


Are these two explanations equivalent? The first one is a macroscopic view that involves entropy of the whole system; the second one involves the distribution of speeds of the molecules themselves.



Answer



You alluded to the answer when you mention activation energy. Kinetically the equilibrium constant is Ke=kf/kb where kf and kb are the forward are reverse reaction rate constants in the reaction AB. The reason that there is a finite and not zero back reaction rate constant, is that the activation barrier going B to A is not infinitely high. Quite the opposite in fact and while larger than the barrier A to B, (if the reaction is exothermic), may nevertheless be of such a magnitude that the products can return to reactants and thus an equilibrium is established. In this case molecules are continually transforming between one another. The ratio of concentrations at equilibrium is the equilibrium constant.



The reason that the activation barrier can be surmounted is that there is a Boltzmann distribution of energies in all molecules and this means that the number of molecules in either A or B with energy Ei is given by ni=n0exp(Ei/(kBT)). This is the Boltzmann distribution for molecules with energy Ei and kB is the Boltzmann constant.


The total number of molecules of type A is given by the sum of those in each level Ei from level 0 to the maximum energy level, which is nAn0=iexp(EAi/(kBT))


The equation for molecules of type B with energy EBi is nBn0=iexp((EBi+ΔE0)/(kBT))=iexp(EBi/(kBT))exp(ΔE0/(kBT))


where ΔE0 is the difference in energy between the lowest levels of A and B.


At equilibrium the constant K is the ratio of the two concentrations which is therefore the same as the ratio of the two populations and is


K=ZAZBexp(ΔE0/(kBT))

where Z represents the summations and are called the partition functions. This equation represents the equilibrium constant in terms of the molecules energy levels.


The reason that there is a Boltzmann distribution, but a fixed energy at a give temperature, is that by far the the most likely way of populating a range of energy levels is according to the Boltzmann distribution. In fact the chance of having a Boltzmann distribution is greater than all other possible ways added together.


In classical thermodynamic terms, a plot of free energy G vs extent of reaction ζ (zeta) which ranges from 0 (entirely A) to 1 (entirely B), has a minimum at some intermediate value of ζ and this value naturally depends on the particular reaction. The minimum value is where the reaction is at equilibrium and at the minimum the slope of G vs. ζ is zero which is also when (G/ζ)T,P=0.


The minimum in G occurs because the entropy term TS has a minimum as the mole fraction of B increases (at constant T). Initially it is the entropy of A alone in solution, but at equilibrium is a mixture of A and B. If the reaction goes entirely to B then the entropy is that of B alone. The entropy of a mixture is naturally greater than that of one species thus TS has a minimum vs. ζ.


If dnA and dnB of A and B molecules react the the infinitesimal change in zeta is dζ=dnAdnB. The total change in free energy is dG=μAdnA+μBdnB where μ is the chemical potential or the free energy / mole. From these two equations the change in free energy of the reaction is dG=(μbμA)dζ

The reaction proceeds until (G/ζ)T,P=0 and thus to proceed further expressions for the chemical potential are needed. For a perfect gas μ=μ0+RTln(p) thus (G/ζ)T,P=μ0Bμ0A+RTlnpBpA
which can be recast as (G/ζ)T,P=ΔG0+RTlnpBpA
and at equilibrium as the derivative is zero ΔG0=RTlnpBpA=RTlnKp
which connect the equilibrium constant (KP for the gas phase reaction), with the free energy.





Edit:


Notes: The shape of the plot of G vs. extent of reaction can be shown by considering a general reaction of the form A+B2C . The Gibbs function is then G=naμa+nbμb+ncμc

for ni moles of species i with chemical potential μi. If we assume that the reaction is one of perfect gases then at total pressure P and with mole fraction x, the chemical potential of species i is μi=μ0i+RTln(P)+RTln(xi)
where μ0i is a function of temperature only. G can now be written as G=naμ0a+nbμ0b+ncμ0c+RTln(P)+RT(naln(xa)+nbln(xb)+ncln(xc))
If we assume that the total pressure is 1 atm. then the RTln(P)=0 and can be removed from the equation. Using the relationship between number of moles na=nb and nc=2(1na) gives G=na(μ0a+μ0b2μ0c)+2μ0c+2RT(naln(na/2)+(1na)ln(1na))
The μ0 are the properties of the pure components so do not change during the course of the reaction which means that G is a function of na only.


A plot of G(na)G(0) vs. na is shown below.


Gvsn


Plotting this way gives a value of zero when n=0, which is the condition should all reactants be converted into product, point S. The equilibrium value is at point E. The energy T-R is that due to mixing reactants and R-E that extra energy of mixing when C is formed. The dashed diagonal line is na(μ0a+μ0b2μ0c) which is how the reaction would behave if no entropy of mixing is included.


The important point is that there is a minimum in the free energy curve because the creation of a mixture is an irreversible process and this mixing produces a decrease in free energy.


The equilibrium constant is calculated using RTln(Kp)=2μ0cμ0aμ0b


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