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Chapter 5   Thermodynamic Potentials

5.1   The Potentials - See Handout

5.2   Helmholtz Free Energy

F=U-TS is related to the maximum amount of extractable work in any given system.

Figure 5.1 - System Converting Heat into Work
Let the system perform work W drawing heat Q from the reservoir. The system has the initial and final temperature T0 (but may have T T0 in between). The total entropy satisfies
D S+D S0³ 0
where S is the system and S0 is the reservoir
D S0=-
Q
T0
D S-
Q
T0
³ 0
Q-T0D S£ 0
The first law says D U=Q-W so we can now eliminate Q
Þ D U+W-T0D S£ 0
D (U-T0S)+W£ 0
however F=U-TS so
D F+W£ 0
W£ -D F     (5.1)
For a process with Ti=Tf=T0 the maximum work the system can do which equals the decrease in F . ie. -D F is the work freed by the process

If no work is done, then
D F£ 0     (5.2)
F never increases and is minimized at equilibrium (we recall that for a thermally isolated system D S³ 0 and dS=0 at equilibrium).

So the Minimum Principle of F for a mechanically isolated system, D F£ 0 (if Ti=Tf ), and F is a minimum at equilibrium. Some points about this though are So the explicit solutions for F is:
P= æ
ç
ç
è
F
V
ö
÷
÷
ø
 



T
,  S=- æ
ç
ç
è
F
T
ö
÷
÷
ø
 



V
we could solve the above or
F=U-TS,  U=
3
2
NkT
S=NlnV+
3
2
NklnT+S0  (for an ideal gas)
F=
3
2
NkT-
3
2
NTlnT-NkTlnV-S0T=-NkTlnV+f(T)     (5.3)


Figure 5.2 - An Example of F
The gas in a cylinder and reservoir temp T where the expansion V1® V2
D F=F2-F!=-NTlnV2+NkTlnV1=-NkTln
æ
ç
ç
è
V2
V1
ö
÷
÷
ø
W£ Wmax=-D F
Wmax=NTln
æ
ç
ç
è
V2
V1
ö
÷
÷
ø
this is equal to the work done by a quasistatic isothermal expansion process.

5.3   Chemical Potential - Changing N

There are many situations in which N varies, eg. in chemical reactions, phase transistions such as pourous containers so now
dU¹ TdS-PdV
as U=U(S,V,N) so we use
dU=TdS-PdVdN
µ is the chemical potential
µ = æ
ç
ç
è
U
N
ö
÷
÷
ø
 



S,V
If U=U(S,V,N1,N2,N3,... ) then
dU=TdS-PdV+
 
å
i
µ dNi
this is made more natural in terms of
G=U+PV-TS
dG=VdP-SdTdN
µ = æ
ç
ç
è
G
N
ö
÷
÷
ø
 



P,T
    (5.4)
but G(P,T,N)=Ng(P,T) so
µ =g(P,T)
which is the specific Gibbs functions for one type of particle
dG=gdN+Ndg
dG=VdP-SdTdN
Þ Ndg=VdP-SdT
we now let v=V/N and s=S/N so we obtain
dg=vdP-sdT
and we recall that
G=NkTlnP+N× (function of T)
µ =kTlnP+f(T)     (5.5)
this is the equilibrium condidtion on µ

Figure 5.3 - Pourous Partition
The equilibrium conditions are dS=dS1+dS2=0 , dU1+dU2=0 , dV1+dV2=0 and dN1+dN2=0 . The fundenmental equation for dS1 and dS2 si
1
T1
(dU1+P1dV11dN1)+
1
T2
(dU2+P2dV22dN2)=0
however dU2=-dU1 , P2dV2=-dV1 and -µ2dN2=-dN1 so we obtain
(something)dU1+(something)dV1+(something)dN1=0
Þ T1=T2,  P1=P2,  µ12
see also section 4.5

5.3.1   Example - A Gas in a Gravitational Field

How does P vary with the height z at a given T

Figure 5.4 - Gravitational Effects on a Gas
µ0=kTlnP0+f(T)
µ1=kTlnP1+f(T)+mgz
the condition of equilibrium is µ01 so
kTlnP0=kTlnP1+mgz
lnP0=lnP1+
mgz
kT
P0
P1
=e
-
mgz
kT
 

5.4   Phase Equilibrium


Figure 5.5 - Phase Equilibria (at constant P and T )
we seek a curve in the PT plane
G=Nlgl+Nvgv
N=Nl+Nv=constant
the equilibrium condition is dG=0
Þ gl(T,P)=gv(T,P)
this is true along the curve at ( TP ). ie. also at ( T+dTP+dP )
Þ dgl=dgv
we recall that dg=vdP-sdT so
vldP-sldT=vvdP-svdT
(sv-sl)dT=(vv-vl)dP
dP
dT
=
sv-sl
vv-vl
we now let l=T(sv-sl) which is the latent heat of evapouration (per particle)
dP
dT
=
l
T(sv-sl)
    (5.6)
this is the Clausius Clapeyon Equation. However if vv>>vl we can use PV=NkT instead so that P=kT/V can be solved

Figure 5.6 - Calculating P=kT/V

5.5   The Third Law

What happens to S as T® 0 ? The physical order increases as T® 0 .

D S may be measured, it was Nerrist in 1906 who noted that D S® 0 as T® 0 in many reactions.

So we may choose S® 0 as T® 0
S(T,x)®as T® 0  (for all x)     (5.7)
where x=P or x=V , etc. This is the Third Law. eg. an ideal gas S~lnT . lnT® -¥ as T® 0 , hence the ideal gas behaviour cannot hold as T® 0 .

For paramagnetic systems
S~ -M2,  -
B2
T2
® -¥
so Curie's Law M~B/T must fail as T® 0
dS=
d-6mu'26 Q
T
=Cp(T)
dT
T
S(T,P)= ó
õ
T


0
dT'
T'
Cp(T')
S(T,P)®as T® 0
Þ CP(T)® 0  (faster than T)
for example when CP is a constant S® -¥ . For metals CP=aT+bT3 whilst for other solids is is generally CP=aT3 . Also we let the expansitivity ( b ) by
b =
1
V
æ
ç
ç
è
V
T
ö
÷
÷
ø
 



P
=-
1
V
æ
ç
ç
è
S
T
ö
÷
÷
ø
 



T
  (Maxwell Relation)
S(T,P)® 0 as T® 0 for all P hence S/ P® 0 also there is the unattainablility of T=0 because S(T,x)® 0 as T® 0 is related to the impossibility of cooling to T .

Figure 5.7 - ??
we use cool gas as a reservoir for another cyclinder and repeat many times

Figure 5.8 - ??
because S(T,V0) and S(T,V1) are convergeal at T=0 , so we need an infinite number of steps to reach T=0 .
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