LOYOLA COLLEGE (AUTONOMOUS), CHENNAI – 600 034 M.Sc. DEGREE EXAMINATION – PHYSICS
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FIRST SEMESTER – NOV 2006
PH 1810 – STATISTICAL MECHANICS
Date & Time : 26-10-2006/1.00-4.00 Dept. No. Max. : 100 Marks
PART A (20 MARKS)
ANSWER ALL QUESTIONS 10 X 2 = 20
- State the ergodic hypothesis.
- State the principle of conservation of extension in phase space.
- When is the classical limit of the quantum description of a system valid?
- Sketch the Maxwell velocity distribution.
- Why is the super fluid transition in Helium known as the lambda transition?
- What is the significance of the fermi temperature?
- What is the pressure exerted by a Fermi gas at absolute zero?
- How is the super fluidity of Helium-3 explained?
- Give Einstein’s relation for the particle diffusion constant.
- Define spectral density for a randomly fluctuating quantity.
PART B (30 MARKS)
ANSWER ANY FOUR QUESTIONS 4 X 7.5 = 30
- Discuss the quantum picture of a micro canonical ensemble.
- Obtain the distribution for an ideal Fermi gas.
- Apply the Bose Einstein statistics to photons and obtain the Planck law for black body radiation.
- Find the temperature dependence of the chemical potential for an ideal FD gas.
- Discuss the random walk problem in 1-d and apply the results to a system of N particles each having a magnetic moment m.
PART C (50 MARKS)
ANSWER ANY FOUR QUESTIONS. 4 X 12.5 = 50
- Calculate the entropy of an ideal Boltzmann gas using the micro canonical ensemble. Explain the corrections to be made to obtain the Sackur-Tetrode equation.
- (a) Discuss the features of the Gibb’s canonical ensemble.
(b) Discuss the rotational partition function for a system of diatomic molecules.
- Discuss the thermodynamic properties of an ideal Bose-Einstein gas.
- Calculate the pressure exerted by a FD gas of relativistic electrons in the ground state. Use the result to explain t5he existence of Chandrasekhar limit on the mass of a white dwarf.
- (a) Show that the fractional fluctuation in concentration is smaller than the MB case for FD statistics and larger for BE statistics.
(b) Obtain Einstein’s result for the energy fluctuations of black body radiation. What is the implication of the result?
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