Density of states

A system at some energy at most EE has some number N(E)N(E) of quantum states available to it. The density of states is how this number changes with energy

ρ(E)= ⁣dN ⁣dE. \rho(E) = \frac{\d N}{\d E}.

The density of states is related to the multiplicity, since over some energy [E,E+δE][E, E + \delta E] the number of states is Γ= ⁣dN ⁣dEδE\Gamma = \frac{\d N}{\d E} \delta E.

Classically for most systems N(E)=N(E) = \infty. We can approximate the quantum result while still doing mostly classical calculations by assuming that each state has some volume h3h^3 in phase space (pp-vv space), and that states cannot “overlap”.

When energy is quadratic in the parameters of the system (quantum number, momentum, etc), the number of accessible states looks like a ball in some high dimension. The density of states is then its surface area.

The volume of an nn-dimensional ball is

Vn(r)=πn/2Γ(n/2+1)rn. V_n(r) = \frac{\pi^{n/2}}{\Gamma(n/2 + 1)} r^n.

Where Γ(x+1)=x!\Gamma(x + 1) = x! for integer xx.