Chapter 11: Problem 16
List similarities and differences between phonons and photons.
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Chapter 11: Problem 16
List similarities and differences between phonons and photons.
These are the key concepts you need to understand to accurately answer the question.
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Consider the relation \(n_{1} / n_{2}=e^{\left(\mathcal{E}_{2}-\mathscr{E}_{1}\right) / k T}\), the Boltzmann factor for nondegenerate states for systems in equilibrium, where \(\mathscr{E}_{2}>\mathscr{E}_{1}\). (a) Show that \(n_{2}=0\) at \(T=0\). (b) Show that \(n_{1}=n_{2}\) at \(T=\infty\) or \(T=-\infty\). (c) Show that \(n_{2}>n_{1}\) at finite negative temperature \(T\). (d) Show that \(n_{1} \rightarrow 0\) as \(T \rightarrow-0\). (e) Hence, explain the statements, "Negative absolute temperatures are not colder than absolute zero but hotter than infinite temperature," and "One approaches negative temperatures through infinity, not through zero." (f) Can you suggest a change in temperature scale that would avoid temperatures that are negative in this sense?
What examples of a Fermi gas are there other than an electron gas and a gas of \(\mathrm{He}^{3}\) atoms?
(a) By combining \(n(\mathscr{E})\) of (11-21) and \(N(\mathscr{E})\) of (11-49) for an ideal gas of classical particles, with $$ A=e^{-\alpha}=\frac{N h^{3}}{(2 \pi m k T)^{3 / 2} V} $$ show that $$ n(\mathscr{E}) N(\mathscr{E}) d \mathscr{E}=\frac{2 N}{(k T)^{3 / 2} \pi^{1 / 2}} \mathscr{E}^{1 / 2} e^{-\mathscr{E} / k T} d \mathscr{E} $$ is the energy distribution of particles in an ideal gas. (b) Show that Maxwell's speed distribution of molecules in a gas, which has the form \(n(v) d v=C v^{2} e^{-m v^{2} / 2 k T} d v\), where \(C\) is a constant, follows directly from this.
Can you devise a cycle of transitions between three states which would maintain an equilibrium in the populations of these states, with transitions that violate detailed balancing? Does it seem reasonable to extend this to a system with many states?
How can the ordered state of the He II explain its lack of resistance to heat conduction?
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