CHM 5414 Lecture Notes
17 October 1996
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Statistical Equilibrium
God plays dice if not with the Universe then at least with Thermodynamics.
But Thermodynamics governs the Universe! So our most probable microstate gives rise
to energy state populations and partition functions which we'll show here not only
yield thermochemical equilibrium but also speak to pedestrian concepts like heat
and work. "Maximization of statistical entropy: it's not just a bright idea; it's
the (2nd) Law."
Energy, entropy, work function...piffle. What we as chemists really want is the
Gibb's Free Energy so we can predict the (thermodynamic) outcome of
chemical reactions. Well, if we weren't so picky, we'd already have it. Our physicist
colleagues have been using A, the work function, for this
purpose. While G points at equilibrium
(G ° = 0)
at constant pressure,
A ° = 0
points at equilibrium at constant volume. Cold comfort for a gas reaction at
atmospheric pressure...which is why we yearn for G. OK...we shall have it.
dE = qrev, in + won = TdS - PdV
H = E + PV so that
dH = dE + PdV + VdP = TdS - PdV + PdV + VdP = TdS + VdP
measures reversible q transfer when dP=0, a great convenience.
and G = H - TS so that
dG = dH - TdS - SdT = TdS + Vdp - TdS - SdT = VdP - SdT
has fixed P and T as its experimental handles, a great convenience.
We'll return to these total differentials (State Functions) in a
moment, but right now it's the function definitions themselves which interest.
Since the physicists want to control equilibrium at fixed T and V,
they would naturally prefer
A = E - TS so that
dA = dE - TdS - SdT = TdS - PdV - TdS - SdT = - SdT - PdV.
But if A = E - TS and E = H - PV and H = G + TS then simple substitution shows us
A = G - PV or G = A + PV.
That's what I really wanted all along because I have simple statistical
mechanical expressions for both A and P. Indeed, harkening back a lecture,
A = - kT ln zN = - nRT ln z
and P = nRT/V ... well, of course that's just the ideal gas equation which evolved
from that "independent particle-in-the-box" ztrans. If we turned on non-idealities,
P would've had a different form. Let's let sleeping dogs lie on this one, and accept PV=nRT.
So that G = A + PV becomes
G = - nRT ln z + nRT = - nRT [ ln(z) - 1 ] = - nRT [ ln(z) - ln(e) ]
or
G = - nRT ln (z/e) = - RT ln (z/e)n
which is, mercifully, as simple as the expression for A; indeed it differs from it only by
the denominator e, the natural number, 2.7182818... (aren't calculators a blessing?).
One of the satisfying features to point out is the continued dependence of these extensive
variables (additive) like G upon the logarithm of the (multiplicative) partition functions.
Even the power n implies multiplicative partition functions due to
moles of material becoming additive components of G.
Thus when we relate the Gibbs Free Energy of the many molecules in a reaction:
a A + b B c C + d D,
the stoichiometric coefficients, = a,b,c,d
replace the power n as moles of material in the reaction as written. Thus
G° = prod G°prod - react G°react
or
G° = - RT [ prod ln(z/e)prod - react ln(z/e)react ]
or
G° = - RT [ ln(z/e)prod - ln(z/e)react ]
or
G° = - RT ln [ (z/e)prod / (z/e)react ]
All of this is recalls the defining moment of 1st semester PChem when it was revealed that G° = - RT ln Keq,
where Keq is the equilibrium constant of the reaction. Thus, we can use with
confidence the intuitive expression:
Keq = (z/e)prod / (z/e)react
It's intuitive because (gee, if it's intuitive, I shouldn't have to say why!) it tells
us that compounds with more states available to them are going to shift equilibrium
their way. Why are we not surprised?
Only a couple of caveats to toss out here: the first is to remind you that although z
is a product of ztrans zrot zvib zel,
there's still only one factor of e in that z/e expression...rather
like there's only one factor of 1/N! in the indistinguishable Z = zN/N!.
The second caveat has to do with z's all being measured from the same origin. That
leads to a factor of exp(-o/kT)
appearing before every z vib. But since each z vib appears with its
own stoichiometric coefficient as a power, zvib,
the zeropoint correction factor becomes
exp( - o / kT)
and the z product and quotients in Keq gather those terms into
exp( - Do / kT )
where
Do = o(products) - o(reactants)
(assuming we measure o as
molecular zeropoint energies. If we used molar zeropoint energies instead, the kT becomes RT.
(Try not to be off by a factor of NAv ; it tends to get noticed.)
Seque to Traditional Thermo
So there's Good News and Bad News.
The Good News is that we're moving now to things less jarringly unfamiliar.
The Bad News is that we're moving to topics too boringly familiar. Win a few;
lose a few.
The thrust of this course (somewhat tardy to mention it here, no?) is to leave you
as comfortable making intuitive conclusions about the world of chemistry using
both your statistical mechanical understanding of the role of availability
of states (when that's informative) and your knowledge of the macroscopic relationships
of thermodynamical variables and their applications. In other words, we want you
to be "switch-hitters," capable of analysing a problem from both the microscopic
and the macroscopic view, emphasizing the one most instructive to the problem at hand.
So having explored the one, we now turn to the other, unafraid to have either view
inform the discussion of the other! For example, we'll speak of heating as the
population of higher energy levels and of work as the retention of populations in
levels which separate from one (another along the energy axis). In either
case, the average energy rises, but they're due to fundamentally different causes,
most easily seen in microscopic arguments.
But we really "see" them through our observation of thermometers and physical
compressions of heat/work experiments. Being a theoretical course, we take on faith
those experiments and draw on the collective wisdom of their collectors.
So we "know" we can raise the energy of a system by flooding heat into it, +qrev., in,
and by working on it, +won. It may come of something of a surprise that
work doesn't always have the same "sense;" that is, collapse doesn't always increase
the energy as it does in a gaseous system. For example,
Gravitational work = h1h2 mg dh = mg h
is an expansive work; we increase the energy of systems (rockets, say) by
"expanding" them away from the gravitational center. This work is the result of
one-dimensional motion in opposition to a one-dimensional force, mass x gravitational
acceleration. (We're trusting that h isn't so large
that g starts falling off...as distance squared from Earth's center.)
The same thing is observed in two-dimensional work such as that done stretching
a balloon or in filling a glass of water slightly more than its capacity. In the
latter case, one we'll explore later in the course, water's surface tension, ,
acts to increase the energy of surface under expansion,
Surface work = a1a2 da = a
In contrast, three-dimensional expansion against external pressure is the way to
decrease the energy of a gaseous system. To increase the system energy, one
compresses it, contracting the volume:
Pressure/Volume work = V1V2 - P dV
Also, in contrast to the near constancy of mg and , Pressure may
well vary during the compression (or expansion). For example, the familiar case
of isothermal expansion of an ideal gas requires substitution of P by nRT/V where
the constants nRT come out of the integral, rendering
Pressure/Volume work = nRT V1V2 - (1/V) dV = - nRT V1V2 d ln(V) = nRT ln (V1/V2)
(We'll discover that there are "ideal surface films" as well as ideal gases.)
We've fixated on the work half of the energy change expression but only identified
a paltry 3 kinds of work; there are as many kinds as there are forces against or along
which to contend. But the other half, heat, we've visited earlier in this course.
Then we identified reversible heat, at least, with our fundamental thermodynamic
variable, entropy, but for a temperature scaling,
dS = qreversible / T
which allows us to complete the fundamental expression of thermodynamics as
dE = TdS - PdV.
In PChem, we recall that while neither heat, TdS, nor work, -PdV, were State
Variables, T, S, P, V, and E were! These individual quantities were completely
characterized by the state of a thermodynamic system but not dependent at all on
the path to that system from any other (including itself). However, different paths
between two states of the system (or away and back to the same one) would involve
varying heat transfers and work done on the system. (Were work and heat transfers
independent of path, cyclic engines could generate no overall work.)
Mathematicians would speak of dE as a perfect differential rather than as a
state function, but the property is the same. They would remind us that any
perfect differential like dE can be evaluated (in the limit of infinitesimal changes) as
dE = (E/S)VdS + (E/V)SdV
where the crux of the differential's "perfection" lay in the Cauchy-Riemann conditions
(which we chemists call "Maxwell's Relations") which require that
[(E/S)V / V]S = 2E/SV = [(E/V)S / S ]V
Well, that isn't the way Maxwell would have you read it; instead from the perfect
differential expression, the partial differentials are easily identified as
(E/S)V = T
and
(E/V)S = - P
So the Cauchy-Riemann condition above becomes the first Maxwell Relation as
(T/V)S = - (P/S)V
admittedly not terrifically illuminating. But wait; there's more! Indeed, there is
one Maxwell relation for each perfect differential we can write: dE, dH, dG, and dA
so far. Some of them are more useful than others, but all are easily found...and
inverted for that matter!
You should be able to show with no difficulty from dG=VdP-SdT that the isothermal
sensitivity of entropy to pressure change can be found from the equation of state
(the gas law, if the system is a gas) as
(S/P)T = - (V/T)P
not a result divined as easily any other way.
Return to the CHM 5414 Lecture Notes or Go To Next or Previous Lectures.
Chris Parr
University of Texas at Dallas
Programs in Chemistry, Room BE3.506
P.O. Box 830688 M/S BE2.6 (for snailmail)
Richardson, TX 75083-0688
Voice: (972) 883-2485
Fax: (972) 883-2925
BBS: (972) 883-2168 (HST) or -2932 (V.32bis)
Internet: parr@utdallas.edu (Click on that address to send Chris e-mail.)
Last modified 28 October 1996.