/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q57E Exercise 54 calculates the three... [FREE SOLUTION] | 91影视

91影视

Exercise 54 calculates the three oscillator distributions'E=0values in the special case wherekBTis15. Using a very common approximation technique. show that in the more general low-temperature limit,kBT,theoccupation numbers become/kBT,e5/kBT, and 1, for the distinguishable. boson. and fermion cases, respectively. Comment on these results. (Note: Although we assume thatkBTN0/(2s+1). we also still assume that levels are closely spaced-that is kBh0.),

Short Answer

Expert verified

For the three distributions, the results are as expected in terms of their relationship to the Pauli Exclusion Principle. Because fermions resist being clumped together in the same state (because Pauli stated that no two fermions can share the same state), a very low temperature is required to view an entire oscillator in the ground state. The bosons, on the other hand, have no such constraints and can pack a large number of oscillators into the ground state. And, ignoring spin, the Boltzmann conclusion is simply another way of saying that the average number of oscillators is equal to the total energy of the oscillators divided by the energy of each oscillator

Step by step solution

01

Formula used

The equations for the distributions will be needed;

NBoltz(E)=EkBT1eE/kBT 鈥︹. (1)

NBE(E)=1eE/kBT1eE/kBT1 鈥︹. (2)

NFD(E)=1eEkBTeEkBT1+1 鈥︹. (3)

Here,

EEnergy

kBBoltzmann's constant

TTemperature

E=N02s+1 鈥︹. (4)

Here,

NNumber of oscillators

Planck's reduced constant

0Fundamental angular frequency

sSpin

02

Check the Boltzmann distribution of equation (2)

The Boltzmann distribution of equation (2) is checked first, using that Ewill be 0:

NBoltz(E)=EkBT1eEkBTNBoltz(0)=EkBT1e(0/VBT=EkBT1e0=EkBT

So, the number of oscillators expected in the ground state if they were classically distinguishable would be .

NBoltz(0)=EkBT

03

Check the Bose-Einstein distribution of equation (3)

The Bose-Einstein distribution of equation (3) is checked with

being 0.

NBE(E)=1eEkBT1eEkBT1

At E=0,

NBE(0)=1e[0/KBT1eEkBT1=1e01eE/KBT1=1e01eE///BT1=111eE/kBT1

NBE(0)=111eEkBT1eEkBT1eEkBT=11(1eEkBT)1eEkBT=1eEkBTeEkBT

NBE(0)=1eEkBTeEkBT=1eEkBTeEkBTeEkBT=eEkBT1

Since kBTis very small, that/kBTmeans that will be very large, and consequently, soeE/kBT. Thus subtracting 1 from it won't significantly affect it, and can be ignored:

NBE(0)=eE/kBT1NBE(0)eE/kBT

So, the number of oscillators expected in the ground state if they were bosons would beNBE(0)eE/kBT and matches the expected value for the Bose-Einstein distribution, thus verifying it.

04

Check for the Fermi-Dirac distribution of equation (4)

The Fermi-Dirac distribution of equation (4) is checked for an Eof 0.

NFD(E)=1EEkBTeEkBT1+1NFD(0)=1e(0)/kBTeE/kBT+1=1c0eE/kBT+1=11eE/kBT+1=11eEkBT+1

NFD(0)=11eEkBT+eEkBTeEkBT=1[1+eEkBTeEkBT]=eEkBT1+eEkBT

Since kBTis very small, that means that /kBTwill be very large, and consequently, so will eE/kBT. Thus adding 1 to it won't significantly affect it, and can be ignored

NFD(0)=eEkBT1+eEkBTeEkBTeEkBT1

So, the number of oscillators expected in the ground state if they were fermions would beNFD(0)1 and matches the expected value from equation (1) for the Fermi-Dirac distribution thus verifying it.

05

Conclusion

For the three distributions, the results are as expected in terms of their relationship to the Pauli Exclusion Principle. Because fermions resist being clumped together in the same state (because Pauli stated that no two fermions can share the same state), a very low temperature is required to view an entire oscillator in the ground state. The bosons, on the other hand, have no such constraints and can pack a large number of oscillators into the ground state. And, ignoring spin, the Boltzmann conclusion is simply another way of saying that the average number of oscillators is equal to the total energy of the oscillators divided by the energy of each oscillator.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91影视!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Discusses the energy balance in a white dwarf. The tendency to contract due to gravitational attraction is balanced by a kind of incompressibility of the electrons due to the exclusion principle.

(a) Matter contains protons and neutrons, which are also fanions. Why do the electrons become a hindrance to compression before the protons and neutrons do?

(b) Stars several times our Sun's mass has sufficient gravitational potential energy to collapse further than a white dwarf; they can force essentially all their matter to become neutrons (formed when electrons and protons combine). When they cool off, an energy balance is reached like that in the white dwarf but with the neutrons filling the role of the incompressible fermions. The result is a neutron star. Repeat the process of Exercise 89. but assume a body consisting solely of neutrons. Show that the equilibrium radius is given by

R=322G(322mn8M)1/3

(c) Show that the radius of a neutron star whose mass is twice that of our Sun is only about10km .

When would a density of states be needed: in a sum over states? in a sum over energies? in an integral over energies? in an integral over states?

At high temperature, the average energy of a classical one-dimensional oscillator is kBT, and for an atom in a monatomic ideal gas. it is 12kBT. Explain the difference. using the equipartition theorem.

The temperature of our Sun鈥檚 surface is ~6000K.(a) At what wavelength is the spectral emission of the Sun is maximum? (Refer to Exercise 79.) (b) Is there something conspicuous about this wavelength?

In Exercise 35, a simple two-state system is studied. Assume that the particles are distinguishable. Determine the molar specific heat Cvof this material and plot it versus T. Explain qualitatively why it should behave as it does.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.