Average Energy - Solid State Physics - Solved Paper, Exams of Solid State Physics

These are the notes of Solved Paper of Solid State Physics. Key important points are: Average Energy, Free Energy, Boltzmann Factor, Consecutive Atoms, Total Multiplicity for Domains, Definition of Temperature, Orientation Flips

Typology: Exams

2012/2013

Uploaded on 02/11/2013

pannaaaa
pannaaaa 🇮🇳

4.8

(6)

68 documents

1 / 3

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
Physics 112 Spring 2010
Professor William Holzapfel
Midterm 1 Solutions
Problem 1
a) Since Zis a sum over microstates, not macrostates, we must include multiplic-
ities (degeneracies). This gives
Z=eE0 (1 + 2e/τ +e2/τ )
=eE0 (1 + e/τ )2.
b) The average energy is given by
U=τ2ln Z
∂τ
=τ2
∂τ hE0 + 2 ln(1 + e/τ )i
=E0+2e/τ
1 + e/τ
=E0+2
1 + e/τ .
c) The free energy is
F=τln Z
=τ[E0 + 2 ln(1 + e/τ)]
=E02τln(1 + e/τ )
and so the entropy is then
σ=∂F
∂τ
= 2 ln(1 + e/τ ) + 2
τ
1
1 + e/τ .
d) Let’s take the τ limits first, since in this case the exponentials e±/τ can
be Taylor expanded:
lim
τ→∞ U(τ)E0+2
1+(1+/τ)
=E0+
1 + /2τ
=E0+(1 /2τ).
1
pf3

Partial preview of the text

Download Average Energy - Solid State Physics - Solved Paper and more Exams Solid State Physics in PDF only on Docsity!

Physics 112 Spring 2010

Professor William Holzapfel

Midterm 1 Solutions

Problem 1

a) Since Z is a sum over microstates, not macrostates, we must include multiplic- ities (degeneracies). This gives Z = e−E^0 /τ^ (1 + 2e−/τ^ + e−^2 /τ^ ) = e−E^0 /τ^ (1 + e−/τ^ )^2.

b) The average energy is given by

U = τ 2 ∂^ ln^ Z ∂τ = τ 2

∂τ

[

−E 0 /τ + 2 ln(1 + e−/τ^ )

]

= E 0 + 2 e

−/τ 1 + e−/τ = E 0 +

1 + e/τ^

c) The free energy is F = −τ ln Z = −τ [−E 0 /τ + 2 ln(1 + e−/τ^ )] = E 0 − 2 τ ln(1 + e−/τ^ ) and so the entropy is then

σ = − ∂F ∂τ = 2 ln(1 + e−/τ^ ) +^2 τ^1 1 + e/τ^

d) Let’s take the τ → ∞ limits first, since in this case the exponentials e±/τ^ can be Taylor expanded:

τlim →∞ U^ (τ^ )^ ≈^ E^0 +^

1 + (1 + /τ ) = E 0 +  1 + / 2 τ = E 0 + (1 − / 2 τ ).

This has limiting value E 0 + , which is what we expect: in the large τ limit all microstates are equally probable, so the average energy should just be the average of all the possible values (weighted by multiplicity), which is E 0 + . Similarly for the entropy (we carefully expand to second order here):

τlim →∞ σ(τ^ )^ ≈^ 2 ln

[

2 − /τ + 

2 2 τ 2

]

+^2 

τ

2 + /τ

≈ 2 ln 2 + 2 ln

[

/ 2 τ −

^2

4 τ 2

)]

τ

2 τ

≈ ln 4 + 2

[

−/ 2 τ +

^2

4 τ 2 −^

2 (/^2 τ^ )

2

]

τ

2 τ

= ln 4 − 1 4

(/τ )^2.

Again, this has the limiting value that we expect at τ → ∞ since there are four possible microstates, all of which are equally likely in this limit. For the low temperature limits, the exponentials cannot be Taylor expanded but the Boltzmann factor itself is small so that allows some simplifications:

τlim → 0 U^ (τ^ )^ =^ E^0 +^2 e

−/τ 1 + e−/τ ≈ E 0 + 2e−/τ^. Likewise,

τlim → 0 σ(τ^ )^ =^ 2 ln(1 +^ e−/τ^ ) +

τ

e−/τ 1 + e−/τ ≈ (^2) τ e−/τ^.

Problem 2

a) Say we start with the first atom spin up. Then we’ll have all consecutive atoms spin up until we hit the first domain wall, where the next atom is spin down. The n domain walls are thus determined by choosing n atoms where the spin orientation flips. Thus if we start with the first domain spin up then choosing n out of N atoms completely specifies a microstate (we don’t choose out of N + 1 because we can’t have a domain wall at the first atom). This then gives a multiplicity of

(N

n

. However, we could also have started with the first domain spin down, so the total multiplicity for n domains is

g(N + 1, n) = 2

N

n

= 2 N^!

N !(N − n)!