Introduction To Quantum Mechanics
Introduction To Quantum Mechanics
3rd Edition
ISBN: 9781107189638
Author: Griffiths, David J., Schroeter, Darrell F.
Publisher: Cambridge University Press
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Chapter 5.3, Problem 5.22P
To determine

The Fermi temperature of helium-3.

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Problem 1: Fermi temperature of the sun At the center of the sun, the temperature is approximately 107K and the concentration of electrons is approximately 1032 per cubic meter. Would it be (approximately) valid to treat these electrons as a classical gas (using Boltzmann statistics), or as a degenerate Fermi gas (with T × 0), or neither?
A system containing a single particle in a rigid container at temperature 100 K has a translational partition function of Ztrans = 1.5 × 1012. (a) If the mass of the particle is doubled, what is the new value for ztrans? Report your answer in scientific notation (in Blackboard, 1.23 x 1045 is written 1.23E45).
Problem 1: This problem concerns a collection of N identical harmonic oscillators (perhaps an Einstein solid) at temperature T. The allowed energies of each oscillator are 0, hf, 2hf, and so on. a) Prove =1+x + x² + x³ + .... Ignore Schroeder's comment about proving 1-x the formula by long division. Prove it by first multiplying both sides of the equation by (1 – x), and then thinking about the right-hand side of the resulting expression. b) Evaluate the partition function for a single harmonic oscillator. Use the result of (a) to simplify your answer as much as possible. c) Use E = - дz to find an expression for the average energy of a single oscillator. z aB Simplify as much as possible. d) What is the total energy of the system of N oscillators at temperature T?
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