NOTE: acceptable formats for turning in your homework are as follows:-
(1) handwritten clearly in blue or black ink
(2) handwritten clearly in 2B or darker pencil
(3) typewritten.
NO other types of work will be marked. In addition, if any of your
working / logic is unclear, points will be docked -- in physics, it's
not only getting the right answer, it's knowing how to get it using
the correct method that matters.
[10] Q1: If equations 6.12, 6.14, and 6.18 in Kittel and Kroemer, concerning a classical ideal gas, are to be self-consistent, what can you say about the sign and the size of the chemical potential relative to the temperature (in energy units)? what strong inequality must hold among the total number of particles in the gas, its volume, the mass of the particles, and the temperature? To what extent would the inclusion of the spin of the particles (see comment (b) at the bottom of p. 162) affect your results?
[10] Q2: Kittel and Kroemer, problem 7-2.
[10] Q3: Kittel and Kroemer, problem 7-6. In part (b), you can assume that there are as many protons as neutrons in a white dwarf, in order to relate the number of electrons in the star to its mass. You might want to try 7--10 as well, but do not hand it in.
[10] Q4: In our derivation of the ground-state energy, U0, of a fermion gas, we assumed that there is no interaction between the fermions. Yet, at fixed volume, U0 is not directly proportional to the number of particles, N, in the gas. In a few lines, account for this seemingly counter-intuitive result.
[10] Q5: The second experiment that produced a Bose-Einstein condensate used sodium atoms with concentration n=1020 atoms/m3. The mass of a sodium-23 atom is M=3.82 x 10-26 kg. Only one spin state was populated.
[10] Q6: Kittel and Kroemer, problem 7-12.