Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Consider a degenerate electron gas in which essentially all of the electrons are highly relativistic ϵmc2so that their energies are ϵ=pc(where p is the magnitude of the momentum vector).

(a) Modify the derivation given above to show that for a relativistic electron gas at zero temperature, the chemical potential (or Fermi energy) is given by =

μ=hc(3N/8πV)1/3

(b) Find a formula for the total energy of this system in terms of N and μ.

Short Answer

Expert verified

The chemical potential is given by:

μ=hc23NπV1/3

Total energy of the system is:

U=3N4ϵF

Step by step solution

01

Given information

Consider a degenerate electron gas in which essentially all of the electrons are highly relativistic ϵmc2 so that their energies are ϵ=pc (where p is the magnitude of the momentum vector).

02

Explanation

The allowable wavelengths and momenta for a relativistic particle in a one-dimensional box are the same as for a non-relativistic particle, and they are provided by:

λn=2Lnpn=hn2L

Where,

n is positive integer

In the three dimensional box, the momenta are:

px=hnx2Lpy=hny2Lpz=hnz2L

Energy for relativistic is:

ϵ=pc

But,

p=px2+py2+pz2

Thus,

ϵ=cpx2+py2+pz2

Substitute with momenta

localid="1650014884234" ϵ=hc2Lnx2+ny2+nz2ϵ=hcn2L

Where,

n=nx2+ny2+nz2each n can be a positive integer, so we can visualise this as a lattice of a points in the first octant.

Because we have two spin stats, the total number of electrons is equal to the volume of an octant of a sphere with radius of nmax multiplied by factor 2.

N=2×18×43πnmax3N=π3nmax3nmax=3Nπ1/3

the chemical potential is just the energy of the last level, which indicated by nmax, that is:

μ=ϵF=ϵnmax

Substitute with ϵ and nmax:

localid="1647741783682" μ=hcnmax2L=hc2L3Nπ1/3μ=hc23NL3π1/3μ=hc23NπV1/3

Here,

V=L3

03

Explanation

(b)Due to the spin, the total energy equals the sum of the energies of occupied states multiplied by factor 2, i.e.

U=2nxnynzϵ(n)

To convert this to spherical coordinates, multiply by the factor of the integration in spherical coordinates, which is n2sin(θ), as follows:

U=20π/2dΦ0π/2sin(θ)dθ0nmaxn2ϵdn

Substitute with ε

localid="1650015025150" U=hcL0π/2dΦ0π/2sin(θ)dθ0nmaxn3dnU=hcLπ2[1]nmax44U=hcπnmax48L

Substitute with nmax

localid="1650015120881" U=hcπ8L3Nπ4/3U=hcπ8L3Nπ3Nπ1/3U=3hcN8L3Nπ1/3U=3hcN83NπV1/3U=3N4hc23NπV1/3ϵFU=3N4ϵF

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 Vaia!

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

For a system of bosons at room temperature, compute the average occupancy of a single-particle state and the probability of the state containing 0,1,2,3bosons, if the energy of the state is

(a) 0.001eVgreater than μ

(b) 0.01eVgreater than μ

(c) 0.1eVgreater than μ

(d) 1eVgreater than μ

In Problem 7.28you found the density of states and the chemical potential for a two-dimensional Fermi gas. Calculate the heat capacity of this gas in the limit role="math" localid="1650099524353" kTεF· Also show that the heat capacity has the expected behavior when kTεF. Sketch the heat capacity as a function of temperature.

Repeat the previous problem, taking into account the two independent spin states of the electron. Now the system has two "occupied" states, one with the electron in each spin configuration. However, the chemical potential of the electron gas is also slightly different. Show that the ratio of probabilities is the same as before: The spin degeneracy cancels out of the Saha equation.

Use the formula P=-(U/V)S,N to show that the pressure of a photon gas is 1/3 times the energy density (U/V). Compute the pressure exerted by the radiation inside a kiln at 1500 K, and compare to the ordinary gas pressure exerted by the air. Then compute the pressure of the radiation at the centre of the sun, where the temperature is 15 million K. Compare to the gas pressure of the ionised hydrogen, whose density is approximately 105 kg/m3.

A ferromagnet is a material (like iron) that magnetizes spontaneously, even in the absence of an externally applied magnetic field. This happens because each elementary dipole has a strong tendency to align parallel to its neighbors. At t=0the magnetization of a ferromagnet has the maximum possible value, with all dipoles perfectly lined up; if there are Natoms, the total magnetization is typically~2μeN, where µa is the Bohr magneton. At somewhat higher temperatures, the excitations take the form of spin waves, which can be visualized classically as shown in Figure 7.30. Like sound waves, spin waves are quantized: Each wave mode can have only integer multiples of a basic energy unit. In analogy with phonons, we think of the energy units as particles, called magnons. Each magnon reduces the total spin of the system by one unit of h21rand therefore reduces the magnetization by ~2μe. However, whereas the frequency of a sound wave is inversely proportional to its wavelength, the frequency of a spin-wave is proportional to the square of 1λ.. (in the limit of long wavelengths). Therefore, since=hfand p=hλ.. for any "particle," the energy of a magnon is proportional

In the ground state of a ferromagnet, all the elementary dipoles point in the same direction. The lowest-energy excitations above the ground state are spin waves, in which the dipoles precess in a conical motion. A long-wavelength spin wave carries very little energy because the difference in direction between neighboring dipoles is very small.

to the square of its momentum. In analogy with the energy-momentum relation for an ordinary nonrelativistic particle, we can write =p22pm*, wherem* is a constant related to the spin-spin interaction energy and the atomic spacing. For iron, m* turns out to equal 1.24×1029kg, about14times the mass of an electron. Another difference between magnons and phonons is that each magnon ( or spin-wave mode) has only one possible polarization.

(a) Show that at low temperatures, the number of magnons per unit volume in a three-dimensional ferromagnet is given by

NmV=2π2m×kTh2320xex-1dx.

Evaluate the integral numerically.

(b) Use the result of part (a) to find an expression for the fractional reduction in magnetization, (M(O)-M(T))/M(O).Write your answer in the form (T/To)32, and estimate the constantT0for iron.

(c) Calculate the heat capacity due to magnetic excitations in a ferromagnet at low temperature. You should find Cv/Nk=(T/Ti)32, where Tidiffers from To only by a numerical constant. EstimateTifor iron, and compare the magnon and phonon contributions to the heat capacity. (The Debye temperature of iron is 470k.)

(d) Consider a two-dimensional array of magnetic dipoles at low temperature. Assume that each elementary dipole can still point in any (threedimensional) direction, so spin waves are still possible. Show that the integral for the total number of magnons diverge in this case. (This result is an indication that there can be no spontaneous magnetization in such a two-dimensional system. However, in Section 8.2we will consider a different two-dimensional model in which magnetization does occur.)

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.

Sign-up for free