/*! 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} Q18CQ At high temperature, the average... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

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.

Short Answer

Expert verified

Average energy from to the equipartition theorem=32kBT

Step by step solution

01

The equipartition theorem.

The equipartition theorem says that any quadratic term in the expression for the total energy E of a particle contributes to the average energy E¯by an amount12kBT, wherekBis the Boltzmann constant, and T is temperature.

02

The total energy of 1-D harmonic oscillator.

First consider the 1-D harmonic oscillator. Its total energy writes:

E=12mvx2+12kx2

whereVx is speed,x is position, mis mass, andk is the force constant.

03

The average energy in a harmonic oscillator 

The two quadratic terms pop up. Use the equipartition theorem, each degree of freedom namelyvx2 and X2contributes to the average energy by an amount 12kBT. Thus, the average energy in a harmonic oscillator must be:

E¯=12kBT+12kBT=kBT

04

Total energy must simply be its kinetic energy in 3-D 

Now for an atom in a monatomic ideal gas, the atom possesses three degrees of freedom in its velocity as it freely moves in 3-D space. Since it is not acted on by a conservative force, then its total energy must simply be its kinetic energy in 3-D:

E=12mvx2+12mvy2+12mvz2

05

Average energy from to the equipartition theorem.

Since the atom has three degrees of freedom, then its average energy from to the equipartition theorem must be:

E¯=12kBT+12kBT+12kBT=32kBT

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 91Ó°ÊÓ!

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

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
Uclocimns=310(3Ï€2h3me32V)23N53

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

Uelectrons=9h280me(3Ï€2M5mp5)131R2

Where, R is the star's radius?

(b) The gravitational potential energy of a sphere of mass Mand radius Ris given by

Ugray=-35GM2R

Taking both factors into account, show that the minimum total energy occurs when

R=3h28G(3Ï€2me3mp5M)13

(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?

Figure 9.8 cannot do justice to values at the very highspeed end of the plot. This exercise investigates how small it really gets. However, although integrating the Maxwell speed distribution over the full range of speeds from 0 to infinity can be carried out (the so-called Gaussian integrals of Appendix K), over any restricted range, it is one of those integrals that. unfortunately. cannot be done in closed form. Using a computational aid of your choice. show that the fraction of molecules moving faster thanis; faster than6vrmsis-10-23; and faster than10vmsis~10-64. wherevrms" from Exercise 41, is3kBT/m. (Exercise 48 uses these values in an interesting application.)

This problem investigates what fraction of the available charge must be transferred from one conductor to another to produce a typical contact potential. (a) As a rough approximation treat the conductors as10cmx 10 cm square plates2cm apart-a parallel-plate capacitors so thatq=CV , where C=σ0(0.01m2/0.02m). How much charge must be transferred from one plate to the other to produce a potential difference of 2V?(b) Approximately what fraction would this be of the total number of conduction electrons in a 100gpiece of copper. which has one conduction electron per atom?

The Stirling approximation.J!≡2πJJ+1/2e-J, is very handy when dealing with numbers larger than about100 . Consider the following ratio: the number of ways Nparticles can be evenly divided between two halves of a room to the number of ways they can be divided with60%on the right and40%on the left.

(a) Show, using the Stirling approximation, that the ratio is approximately4046065Nfor largeN.

(b) Explain how this fits with the claim that average behaviours become more predictable in large systems.

By carrying out the integration suggested just before equation (9-28), show that the average energy of a one-dimensional oscillator in the limit kBT≫³óÓ¬0iskBT.

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.