Chapter 7: Q. 7.31 (page 285)
In Problem
Short Answer
The heat capacity of the gas in the limit is
The graph of heat capacity as a function of temperature is
Chapter 7: Q. 7.31 (page 285)
In Problem
The heat capacity of the gas in the limit is
The graph of heat capacity as a function of temperature is
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Get started for freeAlthough the integrals (
carried out analytically for all T, it's not difficult to evaluate them numerically
using a computer. This calculation has little relevance for electrons in metals (for
which the limit
for astrophysical systems like the electrons at the center of the sun.
(a) As a warm-up exercise, evaluate the
and
above. (Hint: As always when solving a problem on a computer, it's best to
first put everything in terms of dimensionless variables. So let
, and
and then put it on the computer.)
(b) The next step is to vary
the desired value,
and plot the results to reproduce Figure
to try to use numerical methods when
you can start getting overflow errors from exponentiating large numbers.
But this is the region where we've already solved the problem analytically.)
(c) Plug your calculated values ofµ into the energy integral (
that integral numerically to obtain the energy as a function of temperature
for
heat capacity. Check that the heat capacity has the expected behavior at
both low and high temperatures.
For a system of bosons at room temperature, compute the average occupancy of a single-particle state and the probability of the state containing
(a)
(b)
(c)
(d)
The sun is the only star whose size we can easily measure directly; astronomers therefore estimate the sizes of other stars using Stefan's law.
(a) The spectrum of Sirius A, plotted as a function of energy, peaks at a photon energy of
(b) Sirius B, the companion of Sirius A (see Figure 7.12), is only role="math" localid="1647765883396"
(c) The spectrum of the star Betelgeuse, plotted as a function of energy, peaks at a photon energy of
Consider a Bose gas confined in an isotropic harmonic trap, as in the previous problem. For this system, because the energy level structure is much simpler than that of a three-dimensional box, it is feasible to carry out the sum in equation 7.121 numerically, without approximating it as an integral.*
(a) Write equation 7.121 for this system as a sum over energy levels, taking degeneracy into account. Replace
(b) Program a computer to calculate this sum for any given values of
(c) For the same parameters as in part (b), plot the number of particles in each energy level as a function of energy.
(d) Now reduce
(e) Repeat part (d) for
The tungsten filament of an incandescent light bulb has a temperature of approximately
(a) If the bulb gives off a total of
(b) At what value of the photon energy does the peak in the bulb's spectrum occur? What is the wavelength corresponding to this photon energy?
(c) Sketch (or use a computer to plot) the spectrum of light given off by the filament. Indicate the region on the graph that corresponds to visible wavelengths, between
(d) Calculate the fraction of the bulb's energy that comes out as visible light. (Do the integral numerically on a calculator or computer.) Check your result qualitatively from the graph of part (c).
( e) To increase the efficiency of an incandescent bulb, would you want to raise or lower the temperature? (Some incandescent bulbs do attain slightly higher efficiency by using a different temperature.)
(f) Estimate the maximum possible efficiency (i.e., fraction of energy in the visible spectrum) of an incandescent bulb, and the corresponding filament temperature. Neglect the fact that tungsten melts at
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