18
Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container i i In this case h harm onic oscillator Q M w e know that i n i H= h To describe the state of the field, we need to know how many n are in each oscillator hotons are bosons n=0,1,2,3….. 1 2 11 2 2 , ,..., ... Q N,V,T j j j n n n n n n E e e 1 2 11 2 2 0 , ,..., firstw e w antto show that Q N,V,T j j j j j j n nn n j n n n n e e e e

Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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Page 1: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 2: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 3: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 4: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

Monoatomic ideal gases

Page 5: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 6: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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.

Page 7: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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?

Page 8: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 9: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 10: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 11: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 12: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 13: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 14: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

< 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

Page 15: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

<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

Page 16: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 17: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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

Page 18: Example Examples: Photon gas, an electromagnetic field in thermal equilibrium with its container To describe the state of the field, we need to know how

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