Chapter 9: Q28E (page 404)
In a large system of distinguishable harmonic oscillators, how high does the temperature have to be for the probability of occupying the ground state to be less than?
Short Answer
The temperature is
Chapter 9: Q28E (page 404)
In a large system of distinguishable harmonic oscillators, how high does the temperature have to be for the probability of occupying the ground state to be less than?
The temperature is
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Get started for freeA "cold" subject,, is briefly put in contact with s "hut" object,, andof heat flows frum the hot object io the cold use. The objects are then spiralled. their temperatures having changed negligibly due ko their large sizes. (a) What are the changes in entropy of each object and the system as a whole?
(b) Knowing only this these objects are in contact and at the given temperatures, what is the ratio of the probabilities of their being found in the second (final) state for that of their being found in the first (initial) state? What dies chis result suggest?
When a star has nearly bumped up its intimal fuel, it may become a white dwarf. It is crushed under its own enormous gravitational forces to the point at which the exclusion principle for the electrons becomes a factor. A smaller size would decrease the gravitational potential energy, but assuming the electrons to be packed into the lowest energy states consistent with the exclusion principle, "squeezing" the potential well necessarily increases the energies of all the electrons (by shortening their wavelengths). If gravitation and the electron exclusion principle are the only factors, there is minimum total energy and corresponding equilibrium radius.
(a) Treat the electrons in a white dwarf as a quantum gas. The minimum energy allowed by the exclusion principle (see Exercise 67) is
Note that as the volume Vis decreased, the energy does increase. For a neutral star. the number of electrons, N, equals the number of protons. If protons account for half of the white dwarf's mass M (neutrons accounting for the other half). Show that the minimum electron energy may be written
Where, R is the star's radius?
(b) The gravitational potential energy of a sphere of mass Mand radius Ris given by
Taking both factors into account, show that the minimum total energy occurs when
(c) Evaluate this radius for a star whose mass is equal to that of our Sun 2x1030kg.
(d) White dwarfs are comparable to the size of Earth. Does the value in part (c) agree?
Show that the rms speed of a gas molecule, defined as , is given by.
The diagram shows two systems that may exchange both thermal and mechanical energy via a movable, heat-conducting partition. Because both Eand Vmay change. We consider the entropy of each system to be a function of both:. Considering the exchange of thermal energy only, we argued in Section 9.2 that was reasonable to defineas. In the more general case, is also defined as something.
a) Why should pressure come into play, and to what mightbe equated.
b) Given this relationship, show that(Remember the first law of thermodynamics.)
Equation (9-27) gives the density of states for a system of oscillators but ignores spin. The result, simply one state per energy change ofbetween levels, is incorrect if particles are allowed different spin states at each level, but modification to include spin is easy. From Chapter 8, we know that a particle of spinis allowedspin orientations, so the number of states at each level is simply multiplied by this factor. Thus,
.
(a) Using this density of states, the definition, and
calculate the parameterin the Boltzmann distribution (9-31) and show that the distribution can thus be rewritten as
(b) Argue that if,the occupation number is much less than 1 for all E.
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