Introduction
The motivation for discussing the ideal Bose gas is that it exhibits Bose-Einstein condensation. The original prediction of Bose-Einstein condensation by Satyendra Nath Bose and Albert Einstein in 1924 was considered by some to be a mathematical artifact. In the 1930s Fritz London realized that superfluid liquid helium could be understood in terms of Bose-Einstein condensation. However, the analysis of superfluid liquid helium is complicated by the fact that the helium atoms in a liquid strongly interact with one another. In 1995 several groups used laser and magnetic traps to create a Bose-Einstein condensate of alkali atoms at approximately 10-6K. In these systems the interaction between the atoms is very weak so that the ideal Bose gas is a good approximation and is no longer only a textbook example.
The behavior of an ideal Bose gas can be understood by calculating N(T,V,μ), the mean number of particles for given values of the temperature T, volume V, and chemical potential μ. In the grand canonical ensemble N is given by
,
where n(ε) is the mean number of particles with energy ε and g(ε) is the density of states. For a system of particles in three dimensions we know that g(ε) ∝ ε1/2. We substitute the form of g(ε) for bosons and the form of n(ε) and write N(T,V,μ) as
,
where D = 2(2m)3/2π/h3.
To understand the nature of an ideal Bose gas at low temperatures, suppose that the mean density of the system is fixed and consider the effect of lowering the temperature. The correct choice of μ gives the desired value of ρ when substituted into
.
Let us define ρ* = ρ/D so that
.
We will study the behavior of μ as a function of the temperature T for a particular value of ρ*.
Problems
References
Updated 2 May 2007.