For bosons, the average occupation of a single-particle state of energy ε is
⟨nε⟩=eβ(ε−μ)−11
The chemical potential must satisfy μ≤ε0 (the lowest single-particle energy) to prevent negative occupation numbers.
5.2 Density of States and Critical Temperature
For a 3D free Bose gas with ε=ℏ2k2/(2m)The density of states is g(ε)=(V/4π2)(2m/ℏ2)3/2ε. The number of particles in excited states (ε>0) is
Nex=∫0∞eβε−1g(ε)dε=V(2πℏ2mkBT)3/2ζ(23)
Where ζ(3/2)≈2.612 is the Riemann zeta function.
Theorem 5.1 (BEC critical temperature). The maximum number of particles that can be accommodated in excited states is achieved at μ=0. When N exceeds this maximum, the excess condenses into the ground state. The critical temperature is
Tc=mkB2πℏ2(ζ(3/2)n)2/3
Where n=N/V.
Proof. Setting N=Nexmax at μ=0 and solving for T:
This contrasts with the constant CV=23NkB above Tc (equipartition). There is a cusp (discontinuity in the derivative) at TcCharacteristic of a phase transition.
5.5 Worked Example: BEC in Rubidium-87
Problem. Estimate Tc for a gas of N=104 rubidium-87 atoms confined in a harmonic trap with frequency ωho=2π×100 Hz.
Solution
For a harmonic trap, the effective density of states is g(ε)=ε2/(2ℏ3ωho3). The critical temperature in a harmonic trap is:
kBTc=ℏωho(ζ(3)N)1/3
kBTc=(1.055×10−34)(2π×100)(1.202104)1/3
=(6.63×10−32)(20.1)=1.33×10−30J
Tc=1.381×10−231.33×10−30≈9.6×10−8K≈96nK
This is consistent with the 1995 BEC experiments by Cornell and Wieman (JILA) and Ketterle (MIT), who achieved BEC at temperatures of a few hundred nanokelvin. ■