Physics 413: Statistical Mechanics - Homework Solutions...

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Physics 413: Statistical Mechanics - Homework Solutions 8 Problem 1: Quantum corrections to classical ideal gas The classical (Boltzmann) limit corresponds to n= 1 e β(ϵ-μ) + δ 1 Expanding the denominator gives n= e -β(ϵ-μ) (1 - δe -β(ϵ-μ) )+ O[(e -β(ϵ-μ) ) 3 ] Average particle number and internal energy read N = dϵ a(ϵ) e -β(ϵ-μ) (1 - δe -β(ϵ-μ) ) U = dϵ ϵ a(ϵ) e -β(ϵ-μ) (1 - δe -β(ϵ-μ) ) with a(ϵ)= V 2π 2 ( m ¯ h 2 ) 3/2 2ϵ The energy per particle is U N = dϵ ϵ 3/2 e -βϵ (1 - δe -β(ϵ-μ) ) dϵ ϵ 1/2 e -βϵ (1 - δe -β(ϵ-μ) ) = k B T (3/4) π (1 - δe βμ /2 5/2 ) (1/2) π (1 - δe βμ /2 3/2 ) = 3 2 k B T (1 + δe βμ 2/8) The factor e βμ in the correction term can be calculated in lowest order, i.e. for the classical ideal gas. e βμ = N V ( 2π¯ h 2 mk B T ) 3/2 = N V λ 3 where λ is the thermal wave length. Therefore U N = 3 2 k B T (1 + δNλ 3 2/(8V )) The corrections to the pressure most easily follow from the general relation p = (2U )/(3V ) which can be proven as follows: p = - ( ∂V ) T,μ = - V = k B T V ln Z μ = k B T V 1 δ dϵ a(ϵ) ln[1 + δe -β(ϵ-μ) ] partial integration = 2 3 k B T V 1 δ dϵ a(ϵ)ϵ βδe -β(ϵ-μ) 1+ δe -β(ϵ-μ) = 2 3 U V

Transcript of Physics 413: Statistical Mechanics - Homework Solutions...

Page 1: Physics 413: Statistical Mechanics - Homework Solutions 8web.mst.edu/~vojtat/class_6311/solution8.pdf · Physics 413: Statistical Mechanics - Homework Solutions 8 Problem 1: Quantum

Physics 413: Statistical Mechanics - Homework Solutions 8

Problem 1: Quantum corrections to classical ideal gas

The classical (Boltzmann) limit corresponds to

⟨n⟩ = 1

eβ(ϵ−µ) + δ≪ 1

Expanding the denominator gives

⟨n⟩ = e−β(ϵ−µ)(1− δe−β(ϵ−µ)) +O[(e−β(ϵ−µ))3]

Average particle number and internal energy read

N =

∫dϵ a(ϵ) e−β(ϵ−µ)(1− δe−β(ϵ−µ))

U =

∫dϵ ϵ a(ϵ) e−β(ϵ−µ)(1− δe−β(ϵ−µ))

with

a(ϵ) =V

2π2

(m

h2

)3/2√2ϵ

The energy per particle is

U

N=

∫dϵ ϵ3/2 e−βϵ(1− δe−β(ϵ−µ))∫dϵ ϵ1/2 e−βϵ(1− δe−β(ϵ−µ))

= kBT(3/4)

√π (1− δeβµ/25/2)

(1/2)√π (1− δeβµ/23/2)

=3

2kBT (1 + δeβµ

√2/8)

The factor eβµ in the correction term can be calculated in lowest order, i.e. for the classical idealgas.

eβµ =N

V

(2πh2

mkBT

)3/2

=N

Vλ3

where λ is the thermal wave length. Therefore

U

N=

3

2kBT (1 + δNλ3

√2/(8V ))

The corrections to the pressure most easily follow from the general relation p = (2U)/(3V ) whichcan be proven as follows:

p = −(∂Ω

∂V

)T,µ

= −Ω

V

=kBT

VlnZµ =

kBT

V

1

δ

∫dϵ a(ϵ) ln[1 + δe−β(ϵ−µ)]

partial integration

=2

3

kBT

V

1

δ

∫dϵ a(ϵ)ϵ

βδe−β(ϵ−µ)

1 + δe−β(ϵ−µ)=

2

3

U

V

Page 2: Physics 413: Statistical Mechanics - Homework Solutions 8web.mst.edu/~vojtat/class_6311/solution8.pdf · Physics 413: Statistical Mechanics - Homework Solutions 8 Problem 1: Quantum

Problem 2: Bose-Einstein temperature of Helium

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