A particle of mass m is in a cubical well if side L, corresponding to the
potential energy function

U(r) = 0 if |x|, |y| and |z| < L/2, U(r) = ∞ otherwise.

(a) What is its ground-state energy?

(b) What is the energy of the first excited state? Is this energy
level degenerate or non-degenerate? Explain!

(c) Suppose 20 identical, non-interacting particles of mass m and spin
½
are in this well. What is the ground state energy of this system? Is
this ground state degenerate or non-degenerate? Explain!

Consider a "box" that is a two dimensional square well with sides of length L
x L. Inside the well the potential is U = 0, outside the well the
potential is infinite.

(a) Let the box contain one particle of mass M. Determine (or
write down) the general set of wave functions Φ(x,y),
find the allowed energies for these states and identify the eigenvalues k_{x}
and k_{y} for the particle.

(b) Write down the three lowest energy eigenvalues and note the degeneracies, if any.

(c) Make a plot, as a function of the eigenvalues k_{x} and k_{y}, showing the allowed states. On this plot, consider a
circle of radius k = (k_{x}^{2} + k_{y}^{2})^{½}, with k
large. What is the area of this circle? Approximately how many states are
contained in this circle?

(d) Now suppose that the same box contains N identical,
non-interacting Fermi particles, each with mass M and spin ½. We have N >> 1. Find the energy of the highest occupied state, if the system
is in its ground state.

(e) For the N particle system in part d, calculate its total
energy

Solution:

- Concepts:

The two-dimensional, infinite square well, the Pauli exclusion principle. - Reasoning:

We are asked to find the eigenfunctions and eigenvalues of the two-dimensional, infinite square well. When we consider a system of N non-interacting fermions in that well, we must take into account that each state can only be occupied by one spin up and one spin down particle. -
Details of the calculation:

(a) The eigenfunctions and eigenvalues of the 2D infinite square well are

Φ_{nm}(x,y) = (2/L)sin(k_{x}x)sin(k_{y}y), with k_{x}= πn/L, k_{y}= πm/L, n, m = 1, 2, ... .

The associated eigenvalues are

E_{nm}= (n^{2}+ m^{2})π^{2}ħ^{2}/(2ML^{2}) = (k_{x}^{2}+ k_{y}^{2})ħ^{2}/(2M).(b) The three lowest energy eigenvalues are

E_{11}= π^{2}ħ^{2}/(ML^{2}), E_{12}= E_{21}= 5π^{2}ħ^{2}/(2ML^{2}),

E_{22}= 4π^{2}ħ^{2}/(ML^{2}), E_{13}= E_{31}= 5π^{2}ħ^{2}/(ML^{2}).

The eigenvalue 5π^{2}ħ^{2}/(2ML^{2}) is degenerate.(c) k

_{x}= πn/L, k_{y}= πm/L, ∆k_{x}= ∆k_{y}= π/L.The area of a circle in 2D k-space is A = πk

^{2}.

The number of states in the circle is N_{states}= (A/4)/(π/L)^{2}= k^{2}L^{2}/(4π).

Only positive values of k_{x}and k_{y}are allowed.

The density of states in k-space is n(k) = dN/dk = kL^{2}/(2π).

(d) Each state can be occupied by two particles, one with spin up and one with spin down.

If the system is in its ground state all the lowest energy levels are filled.

The energy of the highest occupied state is E_{max}= ħ^{2}k_{max}^{2}/(2M),

where N_{particles}= (k_{max}^{2}L^{2}/(2π) or k_{max}^{2}= 2πN_{particles}/L^{2}.

(e) The number of states between k and k + dk that can be occupied is 2n(k)dk = (kL^{2}/π)dk.

The total energy of the system is

E_{t }= ∫_{0}^{kmax}(ħ^{2}k'^{2}/(2M))2n(k')dk' = ∫_{0}^{kmax}(ħ^{2}k'^{2}/(2M))(k'L^{2}/π))dk'

= (ħ^{2}L^{2}/(2Mπ)) ∫_{0}^{kmax }k'^{3}dk' = (ħ^{2}k_{max}^{4}L^{2}/(8Mπ)) .

E_{t}= ħ^{2}πN^{2}_{particles}/(2ML^{2})).

Consider an ideal 3D Fermi gas comprising N non-interacting fermions, each
of mass M, in a container of volume V at T = 0

(a) Find the Fermi energy.

(b) Find ρ(E)dE the number of quantum states whose energy lies in the range

E to E + dE.

(c) Find the average energy per fermion at absolute zero by making a direct
calculation of U(0)/N, where U(0) is energy at T = 0 for N fermions. Express
this in terms of the Fermi energy, E_{F}.

Solution:

- Concepts:

The Pauli exclusion principle, the Fermi energy - Reasoning:

The Fermi energy is the energy difference between the highest and lowest occupied single-particle states in a quantum system of non-interacting fermions at T = 0. - Details of the calculation:

(a) The eigenfunctions and eigenvalues of the 3D infinite cubic well are

Φ_{nmp}(x,y,z) = (2/L)^{3/2}sin(k_{x}x)sin(k_{y}y)sin(k_{z}z),

with k_{x}= πn/L, k_{y}= πm/L, k_{z}= πp/L, n, m, p = 1, 2, ... .

The associated eigenvalues are

E_{nmp}= (n^{2}+ m^{2}+ p^{2})π^{2}ħ^{2}/(2ML^{2}) = (k_{x}^{2}+ k_{y}^{2}+ k_{z}^{2})ħ^{2}/(2M)

The spacing between successive allowed values of k_{i}is ∆k_{x}= ∆k_{y}= ∆k_{z}= π/L. Only positive values of k_{x}, k_{y}, and k_{z}are allowed.

If k is large, then the number of states with wave vectors whose magnitudes is less or equal to k is N = (1/8)(4π/3)k^{3}/(π/L)^{3}.

Each state can be occupied by two particles, one with spin up and one with spin down.

The energy of the highest occupied state is E_{F}= ħ^{2}k_{F}^{2}/(2M), with k_{F}^{2}= (3Nπ^{2}/V)^{(2/3)}.

E_{F}= ħ^{2}(3Nπ^{2}/V)^{(2/3)}/(2M) = ħ^{2}(3nπ^{2})^{(2/3)}/(2M), where n is the number of particles per unit volume.

(b) The number of states with wave vectors whose magnitudes lie between k and k + dk is dN = (1/8)*2*4πk^{2}dk/(π/L)^{3}= L^{3}k^{2}dk/π^{2}. dN/dk = L^{3}k^{2}/π^{2}.

The density of states is ρ(E) = dN/dE = (dN/dk)(dk/dE).

With E = ħ^{2}k^{2}/(2M) we have ρ(E) = dN/dE = L^{3}Mk/(πħ^{2}) = 2^{½}M^{3/2}VE^{½}/(π^{2}ħ^{3}).

(c) <E> = (1/N)∫_{0}^{EF}ρ(E) E dE = 2^{½}M^{3/2}/(nπ^{2}ħ^{3}) ∫_{0}^{EF}E^{3/2}dE = (2M)^{3/2}/(nπ^{2}ħ^{3})E_{F}^{5/2}/5.

<E> = [(2M)^{3/2}/(nπ^{2}ħ^{3})/5]E_{F}*E_{F}^{3/2}.

E_{F}^{3/2}= ħ^{3}(3nπ^{2})/(2M)^{3/2}. <E> = (3/5) E_{F}.