Physics 413: Statistical Mechanics - Homework Solutions...
Transcript of Physics 413: Statistical Mechanics - Homework Solutions...
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
Problem 2: Bose-Einstein temperature of Helium