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PHY 418: Statistical Mechanics I
Prof. S. Teitel: stte@pas.rochester.edu ---- Spring 2021

Problem Set 4

Since Wednesday, March 3, is a University study break day, we will have no Discussion Session this week, and hence there will be no Discussion Question this week.


Problems -- Due Thursday, March 4, by 5pm.

Upload your solutions to Blackboard at this link: PS4

  • Problem 1 [25 points total]

    Consider a system of N distinguishable non-interacting objects, each of which can be in one of two possible states, "up" and "down", with energies +ε and −ε. Assume that N is large.

    (a) Working in the microcanonical ensemble, find the number of states Ω(E,N), and then the entropy of the system S(E, N), as a function of fixed total energy E and number N (Hint: it may be useful to consider the numbers N+ and N of up and down objects). Sketch S(E,N) as a function of E for fixed N, and show that it is not a monotonic increasing function of E. What is the key feature of this system that causes the dependence of S on E to be so qualitatively different from that of an ideal gas? [10 points]

    (b) Using your result from (a) find the temperature T as a function of energy E and number N. Show that T will be negative if E>0. Sketch T vs E for fixed N. [7 points]

    (c) What happens if such a system (1) with T1<0 comes into thermal contact with another such system (2) with T2>0? Does T1 increase or decrease? Does T2 increase or decrease? In which direction does the heat flow? [8 points]

  • Problem 2 [10 points total]

    In Notes Eq. (2.4.14) we derived the number of states Ω(E,V,N) for the idea gas of N point particles, which can be written as given below,
    Ω(E,V,N) = [ V
    h3
    (2πmE)3/2 ]N             1            
    [(3N/2) - 1]!  N!
    (ΔE/E)

    Note, compared to Eq. (2.4.14) the above expression has the factor N! in the denominator, as needed for indistinguishable particles, as described in Notes 2-7.

    By taking the Laplace transform of Ω(E,V,N), directly compute the canonical partition function, as in Notes Eq. (2.8.6),

    QN(T,V) =

    0
    dE
    ΔE
    Ω(E,V,N)e-βE

    Using the resulting canonical partition function, compute the Helmholtz free energy A(T,V,N) and compare it to what was found in Problem Set 1.