Consider a gaseous state elementary reaction aA(g)+bB(g)kf−⇀↽−kbcC(g)+dD(g)
I know that for this reaction, ΔG=ΔG∘+RTln(PcCPdDPaAPbB)
Now, if K=(PcCPdDPaAPbB),
then ΔG=ΔG∘+RTlnK.
Now, how can we say that K=kbkf
and rf=kf⋅PaA⋅PbB and rb=kf⋅PcC⋅PdD where rf and rb are rates of forward and backward reaction as assumed in this answer.
I want that to know that how can one prove rigorously that rf=kf⋅PaA⋅PbB and rb=kb⋅PcC⋅PdD.
Answer
I want that to know that how can one prove rigorously that rf=kf⋅PaA⋅PbB and rb=kb⋅PcC⋅PdD.
I might try to give you some intuition to back up that, for a given (elementary) reaction Ak→B, the reaction rate r can be written as
r=dPBdt=−dPAdt∝PA.
(Observe that the second equality above is true due to PA+PB=constant.) First, for an ideal gas, PA=nAVRT. This means that PA∝n for fixed temperature and volume.
Let's say the reaction happens as a random process. That is to say that, for every time interval Δt, we have a probability per unit time p of having a single molecule A turning into B. If we wait longer, proportionally more molecules will turn. We'll thus have, for initially nA molecules of A, after Δt seconds,
ΔnB=pnAΔt.
This means that, in the time interval Δt, the population of B goes from 0 to ΔnB (assuming no B initially). From the stoichiometry of the reaction, ΔnB=−ΔnA (i.e., there's conservation of moles).
Thus,
ΔnBΔt=−ΔnAΔt=pnA.
After taking the limit of Δt→0 and multiplying by 1V (i.e., dividing by volume), we get
dnBVdt=d[B]dt=pnAV=p[A],
where [A] and [B] stand for the concentrations of A and B, respectively. Since, again for an ideal gas, [A]=PART, we get
r=dPBdt=−dPAdt=pPA,
where the proportionality constant is the probability of reaction per unit time.
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