Chapter 7: Q. 7.57 (page 313)
Fill in the steps to derive equations and.
Short Answer
The derived equations are and.
Chapter 7: Q. 7.57 (page 313)
Fill in the steps to derive equations and.
The derived equations are and.
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Get started for freeConsider a free Fermi gas in two dimensions, confined to a square area •
(a) Find the Fermi energy (in terms of and ), and show that the average energy of the particles is .
(b) Derive a formula for the density of states. You should find that it is a constant, independent of .
(c) Explain how the chemical potential of this system should behave as a function of temperature, both when role="math" localid="1650186338941" and when is much higher.
(d) Because is a constant for this system, it is possible to carry out the integral 7.53 for the number of particles analytically. Do so, and solve for as a function of . Show that the resulting formula has the expected qualitative behavior.
(e) Show that in the high-temperature limit, , the chemical potential of this system is the same as that of an ordinary ideal gas.
In the text I claimed that the universe was filled with ionised gas until its temperature cooled to about 3000 K. To see why, assume that the universe contains only photons and hydrogen atoms, with a constant ratio of 109 photons per hydrogen atom. Calculate and plot the fraction of atoms that were ionised as a function of temperature, for temperatures between 0 and 6000 K. How does the result change if the ratio of photons to atoms is 108 or 1010? (Hint: Write everything in terms of dimensionless variables such as t = kT/I, where I is the ionisation energy of hydrogen.)
Explain in some detail why the three graphs in Figure all intercept the vertical axis in about the same place, whereas their slopes differ considerably.
Consider a degenerate electron gas in which essentially all of the electrons are highly relativistic so that their energies are (where p is the magnitude of the momentum vector).
(a) Modify the derivation given above to show that for a relativistic electron gas at zero temperature, the chemical potential (or Fermi energy) is given by =
(b) Find a formula for the total energy of this system in terms of N and .
Starting from the formula for derived in Problem 7.70(b), calculate the entropy, Helmholtz free energy, and pressure of a Bose gas for . Notice that the pressure is independent of volume; how can this be the case?
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