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Example
Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container
i
i
In this case h harmonic oscillatorQM we know that i ni
H = h
To describe the state of the field, we need to know how many n are in each oscillator
Photons are bosons n=0,1,2,3…..
1 2
1 1 2 2
, ,...,
... Q N,V,Tj
j j
n n n
n n nEe e
1 2
1 1 2 2
0 , ,...,
first we want to show that
Q N,V,Tj j
j j j j
n n n nj
n nn ne e e e
Cont.
1 1 1 2 2 2
3 3 3
0 1 2 0 1 2
0 1 2
Q N,V,T
e e e e e e
e e e
1 2 1 2 1 2 1 2 1 2
1 2 1 2 1 2 1 2
3 3 3
1 2 1
2 1 2
0 0 0 0 1 0 1
1 2 0 2 1
0 1 2
e e e e
e
e
e e e
e e e
1 2 3 1 2 3 1 2
1 2 3 1 2
1 2
3
3 0 0
1 0 1 1 2 3
1 2 3 1 2 3
1 2
1
1 2 3
1 2 3
0 0 1 00 0 0
0 0 0 1 2
0 2 1 0 2 2 1
0 2
0
0
0 ...
e e
e e
e e
ee
e e e
1 2
1 2 31 2 3
1 1 2 2 3 3
0 0 0
1 2
1 2 3
1 2 3 1 3 32
, ,...,
010 0 1 0
0 0 1 2 0 0 0 2 0
...
jn n n
n n n
e e
e
e
e e e
Cont
j
10 1
where we used1Q N,V,T
1 jj
j j
j xnj j x
nee
The average number of photons in a state j…
1 1 2 2
j
...
n
jjn
E
E
n nn en e
Qe
1 1 2 2 ...
ln , ,1
j j
n
j jn n n n
n neQ N V T
Q
ln , , 1 ln 1 j
j
Q N V T e
ln , ,
1
j
jj
Q N V T e
e
j
1average occupation number is n =
1jePlanck distribution
Monoatomic ideal gases
for the number of states to be N,
32 26
1 12
m
h
kT
To evaluate a monoatomic ideal gas we first see if it can
be represented by the Bolztmann statistics
2
32 2
for 10 , 10 , 300
61 for most gases Boltzmann Stat.
12
m gr a cm T K
kTm
h
,Q N,V,Twe can us
!e
Nq V T
N How do we calculate the molecular partition function q V,T ?
translation electronic nuclearq V,T
we can write thu
=
s
q q q
translation electronic nuclearH H H +H
sum over states sum over levels
q V,Tj
j k
kk
kT kTe e
Nuclear Contribution
for nuclear states ~106 ev to populate an excited state, T>1010 Kwe can consider only the ground state
Nuclear partition function qnuclear
degeneracy
sum over levels
1 2
1 2,nuclear
k
kk
kT kT kTq V T e e e
1
1
we arbitrarily define the ground state as 0
all other energies will be referenced to
12
1 2,nuclear kTq V T e
1
degeneracy is given by spin 2 1I
1
,nuclearq V T
For most chemical problems (not nuclear!), qnuclear is just a const.
Electronic Contribution
Electronic partition function qelectronic
degeneracy
sum over levels
1 2
1 2,electronic
k
kk
kT kT kTq V T e e e
1 we arbitrarily define the ground state as 0
12
1 2,electronic kTq V T e
for electronic states, 400-700 nm (Uv-Vis); 33000–15000 cm-1;
4–1.8 ev; 160 kT – 70 kT; 6.6x10-19J – 3x10-19 J
Most cases
@300K only ground state pop. T>104 K for pop. in excited state
1
,electronicq V T
What is the degeneracy 1 of an electronic energy level?
Electronic degeneracy
What is the degeneracy 1 of an electronic energy level?
We have to go back to atomic electronic structure and Spectroscopic Term Symbols 2S+1Lj (for light atoms with RS S-L coupling)
1 =2j +1
212
10 1
12
1
32
1H 2 1 2
2
He 2 0 1 1
3F 2
2
1
1 42
4
electronic
electronic
electronic
q
q
q
S
S
P
Fraction of population in excited states
12For heavy atoms,
12
1 2sometimes we have to consider
kT ,
,
electronic kTq V T e
st
to know whether we have to consider an additional electronic
state, we calculate the fraction of atoms in the 1 excited state
2
12
2
12
1 2
kT
kT
ef
e
312 1
7652
19.80.0259
19.80.00259
He 19.8
3
1
3 10
3
S
ef
ev
e
1
2
212
2
0.050.0259
0.050.00259
F 0.05
2
4 2
0.068f
ev P
e
e
for 300
25.9
T K
kT mev
Translation Contribution by levelTranslation partition function qtranslation
A single particle translation energy is given by 2
2 2 2
2,
8
x y zn n n x y z
hn n n
ma
sum over level
degeneracy
s
,translationk
kk
kTq V T e
2 2 2x y z
3
2 3
2
where we consider again a sphere
of radius R= n n n
8 and
4
k
ma d
h
because the between 2 consecutive states 0
we can consider a continuos change in energy
3
2 3
20 0
8,
4translation kT kTm
q V T e d a e dh
3
2
2
2,translation mkT
q V T Vh
Translation Contribution by stateTranslation partition function qtranslation
sum over states
,
,
,translation
n n nx y z
n n nx y z
kTq V T e
22 2 2
2 2
2
23
88
,
,
x y z h n
transla
hn n n
tion kma
T
n
k maT
n n nx y z
q V T ee
2 2
2
2
2
11 32
3
8
8
1,
2
h n
translation kT ma
h
kT ma
q V T e dn
because the between 2 consecutive states 0 we can
consider a continuos change in energy
n
3
2
2
2,translation kT m
q V T Vh
Q of ideal gas
combining all these information we obtain Q N,V,T
123
2
2 2 11
1Q V,
!
2N, T kT
elec ele ucc
N
n
mkTV
hNe
2
and for the thermodynamic properties...
, , - ln , ,
lnQ N,V,TE
lnQ N,V,Tp
lnQ N,V,TS ln , ,
lnQ N,V,T, ln
A N V T kT Q N V T
kTT
kTV
k Q N V T kTT
T P kTN
12
1 2
3
2
2 1
21A= ln
!kT
elec elec uc
N
n
mkTVkT
he
N
1ln ln ln 1 ln
N!
N
eN N N N N N
1nuclear contributions is constantusually omittedln nucNkT
123
2
1 22
2 A= ln ln kT
elec elec
mkT eVNkT NkT e
Nh
12
2
2
1
3
2
2 kTelec elec e
m
N
T
h
ekV 54@ room T 4 10 1
3
2
2
the only significant contributionis from the translations A=
2ln
mkT eVNkT
Nh
Helmholtz energy, A N,V,T - ln , ,kT Q N V T
< E>for an ideal monoatomic gas
12
1 2
3
2
2
2
1
!ln
E =
2elec elec
kT
N
N
mkTV
h
kT
e
T
12
2 12 at low T, the electronicterm is neglegible
3
2E =
kTelec
electronic
Nke
TN
q
12
2
1
3
22 2
3
2
2
2
1
!
lnln
E =
2ln
elec
elec
N
kTN
N
N
eT
kT kTT T
mkV
h
kTT
Internal energy <E>
2 lnQ N,V,T
kTT
<p> for a monoatomic gas
12
1 2
3
2
2
1
!p
2ln elec elec
k
N
T
N
mkTV
hkT
e
V
Pressure <p>
all contributions from translationp
NkT
V
12
1 2
3
2
2
1
!
2ln
lnp
elec eleckT
N
mkTe
hVkTN kTN
V V
lnQ N,V,T
kTV
S for a monoatomic gas
Entropy S(N,V,T)
12
12
3
2
1 22
2 12
2ln ln
1 3
2
kTelec elec
kTelec
electronic
mkT eVS Nk Nk e
Nh
N eNkT
T q
translation electronicS S S
5322
. 2
2lntrans
mkT e VS Nk
Nh
12
12
2 12. 1 2ln
kTeleckT
elec elec elecelectronic
eS Nk e
kTq
lnQ N,V,Tln , ,k Q N V T kT
T
for a monoatomic ideal gas
Chemical potential (T,P)
12
1 2
3
2
2
1
!n
=
2l
, -
elec eleckT
N
N
mk
T p kT
TeV
h
N
12
1 2
3
2
2
ln
2ln
=+
elec eleckT
N N NkT
N
mkTN V e
hkT
N
12
1 2
3
2
2 02
= ln 1 ln elec eleckTkT
N mkTkT N V e
N h
lnQ N,V,T
lnkTN
Reference
3
2
2 .
2ln ln eleckT
mkT qk
T V
Nh
3
.
2
2
2, ln ln lnelec kT
mkTkT
hqT P kT kT p
, lnoT p T kT p
12
1 2
3
2
2
2
ln
elec eleckT
kT
mkTV
he
N