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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.)

Short Answer

Expert verified

(a). The required condition of this part is proved.

(b). The result is M0MTM0=22.3152πVN2mkTh23/2

(c). The heat capacity due to magnetic excitations in a ferromagnet at low temperature is CV=5π1.7833V2mh23/2k5/2T3/2.

(d). The required condition of this part is proven.

Step by step solution

01

Part (a) step 1: Given Information 

We need to find the number of magnons per unit volume in a three-dimensional ferromagnet is given.

02

Part (a) step 2: Simplify

The number of magnons equal the sum of Planck distribution all over the modes nx,nyand nzmultiplied by the factor of 1because we have two polarization modes, that is:

Nm=nxnynzn-P1ϵ=nx,ny,nzn-Plϵ

but,

n-Plϵ=1eϵ/kT1

where,

ϵ=p22m

consider we have a cubic box with volume of and side width of , the allowed momenta for magnons is given by:

p=hλ=hn2L

therefore,

ϵ=h2n28mL2

substitute into the above equation to get:

Nm=nz,ny,nz1eh2n2/8mL2kT1

now we need to change the sum to an integral in spherical coordinates, by multiplying this by the spherical integration factor n2sin(θ)so we get:

Nm=0π/2dΦ0π/2sinθdθ0n2eh2n2/8mL2kT1dn

the first two integrals are easy to evaluate, and they give a factor of π/2so:

localid="1650306816172" Nm=π20n2eh2n2/8mL2kT1dn

now let,

localid="1650306825074" x=h2n28mL2kTn=8mL2kTxh2dn=2mL2kTh21xdx

thus,

localid="1650306839587" Nm=π201ex12mL2kTh28mL2kTxh21xdx

localid="1650306845592" Nm=2π2mL2kTh23/20xex1dx

but the volume is given as localid="1650306851531" V=L3therefore:

localid="1650306857173" Nm=2πV2mkTh23/20xex1dx

using we can find the integral numerically, the code is shown in the following picture and the value of the integral is localid="1650306864643" 2.3152, therefore:

localid="1650306870482" Nm=22.3152πV2mkTh23/2

03

Part (b) step 1: Given Information 

We need to find an expression for the fractional reduction in magnetization.

04

Part (b) step 2: Simplify 

The total magnetization at the temperature of T=0is 2μBNeach magnon reduces the total magnetization by a value of 2μBthen the fractional reduction in the magnetization is:

M0MTM0=2μBNm2μBN=NmN

substitute from the result of part (a) to get:

M0MTM0=22.3152πVN2mkTh23/2=TT022.3152πVN2mkTh23/2=TT03/2

solve for T0, we get:

TT0=22.3152πVN2/32mkTh2T0=122.3152πNV2/3h22mk

now we need to find this value for iron, the volume of one mole of iron is

V=7.11×106m3and the number of atoms in one mole of iron is N=6.022×1023the mass of the iron atom is m=1.24×1029kgsubstituted with these values to get:

T0=122.3152π6.022×10237.11×106m32/36.626×1034Js221.24×1029kg1.38×1023J/K

T0=4152K

05

Part (c) step 1: Given Information 

We need to find the magnon and phonon contributions to the heat capacity.

06

Part (c) step 2: Simplify

To find the heat capacity we first need to find the total energy, in the same way of finding Nm,but we must multiply the distribution with, that is:

U=nxnynzϵn-Plϵ=nz,ny,nzϵn-Plϵ

but,

n-Plϵ=1eϵ/kT1

where,

ϵ=p22m

consider we have a cubic box with volume of and side width of , the allowed momenta for magnons is given by:

p=hλ=hn2L

therefore,

localid="1650306911538" ϵ=h2n28mL2

substitute into the above equation to get:

localid="1650306915837" U=h28mL2nx,ny,nzn2eh2n2/8mL2kT1

now we need to change the sum to an integral in spherical coordinates, by multiplying this by the spherical integration factor localid="1650306922250" n2sin(θ)so we get:

localid="1650306926387" U=h28mL20π/2dΦ0π/2sinθdθ0n4eh2n2/8mL2kT1dn

he first two integrals are easy to evaluate, and they give a factor of localid="1650306933758" π/2, so:

localid="1650306941435" U=h28mL2π20n4eh2n2/8mL2kT1dn

now let,

localid="1650306949525" x=h2n28mL2kTn=8mL2kTxh2dn=2mL2kTh21xdx

thus,

localid="1650306955308" U=h28mL2π28mL2kTxh220x2ex12mL2kTh21xdxU=2πV2mkTh23/2kT0x3/2ex1dx

using we can find the integral numerically, the code is shown in the following picture and the value of the integral is localid="1650306961001" 1.7833therefore:

localid="1650306967244" U=2π1.7833V2mh23/2k5/2T5/2

now to find the heat capacity we diffrentiate the total energy with respect to localid="1650306974153" T, that is:

localid="1650306980247" CV=UT=T2π1.7833V2mh23/2k5/2T5/2

localid="1650306985176" CV=5π1.7833V2mh23/2k5/2T3/2

we can write the heat capacity as follow:

CVNk=TT13/2

where

1T13/2=5π1.7833VN2mkh23/21T1=5π1.7833VN2mkh23/22/31T1=5π1.7833VN2/32mkh2T1=15π1.7833NV2/3h22mk

but,

T0(22.3152)2/3=1πNV2/3h22mk

therefore:

T1=22.315251.78332/3T0

substitute with T0to get:

T1=22.315251.78332/34152K=2682.5KT1=2682.5K

07

Part (d) step 1: Given Information 

We need to find the integral for the total number of magnons that diverge.

08

Part (d) step 2: Simplify

For two dimensional array, we can write the number as:

Nm=nz,ny1eϵ/kT1

now we need to change the sum to an integral in polar coordinates, by multiplying this by the polar integration factor (ndθ),(dn)so we get:

Nm=π20neϵ/kT1dn

change the integral to be in x, that is

Nm0nex1dx

near x=0we can expand the exponential using ex=1+xso we get:

Nm011+x1dxNm01xdx

but the integration of1/xislnxso the number diverge at the lower limit(0).

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Most popular questions from this chapter

Figure 7.37 shows the heat capacity of a Bose gas as a function of temperature. In this problem you will calculate the shape of this unusual graph.

(a) Write down an expression for the total energy of a gas of Nbosons confined to a volume V, in terms of an integral (analogous to equation 7.122).

(b) For T<Tcyou can set μ=0. Evaluate the integral numerically in this case, then differentiate the result with respect to Tto obtain the heat capacity. Compare to Figure 7.37.

(c) Explain why the heat capacity must approach 32Nkin the high- Tlimit.

(d) For T>Tcyou can evaluate the integral using the values of μcalculated in Problem 7.69. Do this to obtain the energy as a function of temperature, then numerically differentiate the result to obtain the heat capacity. Plot the heat capacity, and check that your graph agrees with Figure 7.37.

Figure 7.37. Heat capacity of an ideal Bose gas in a three-dimensional box.

Consider any two internal states, s1 and s2, of an atom. Let s2 be the higher-energy state, so that Es2-Es1=ϵ for some positive constant. If the atom is currently in state s2, then there is a certain probability per unit time for it to spontaneously decay down to state s1, emitting a photon with energy e. This probability per unit time is called the Einstein A coefficient:

A = probability of spontaneous decay per unit time.

On the other hand, if the atom is currently in state s1 and we shine light on it with frequency f=ϵ/h, then there is a chance that it will absorb photon, jumping into state s2. The probability for this to occur is proportional not only to the amount of time elapsed but also to the intensity of the light, or more precisely, the energy density of the light per unit frequency, u(f). (This is the function which, when integrated over any frequency interval, gives the energy per unit volume within that frequency interval. For our atomic transition, all that matters is the value of u(f)atf=ϵ/h) The probability of absorbing a photon, per unit time per unit intensity, is called the Einstein B coefficient:

B=probability of absorption per unit timeu(f)

Finally, it is also possible for the atom to make a stimulated transition from s2down to s1, again with a probability that is proportional to the intensity of light at frequency f. (Stimulated emission is the fundamental mechanism of the laser: Light Amplification by Stimulated Emission of Radiation.) Thus we define a third coefficient, B, that is analogous to B:

B'=probability of stimulated emission per unit timeu(f)

As Einstein showed in 1917, knowing any one of these three coefficients is as good as knowing them all.

(a) Imagine a collection of many of these atoms, such that N1 of them are in state s1 and N2 are in state s2. Write down a formula for dN1/dt in terms of A, B, B', N1, N2, and u(f).

(b) Einstein's trick is to imagine that these atoms are bathed in thermal radiation, so that u(f) is the Planck spectral function. At equilibrium, N1and N2 should be constant in time, with their ratio given by a simple Boltzmann factor. Show, then, that the coefficients must be related by

B'=BandAB=8πhf3c3

The heat capacity of liquid H4ebelow 0.6Kis proportional to T3, with the measured valueCV/Nk=(T/4.67K)3. This behavior suggests that the dominant excitations at low temperature are long-wavelength photons. The only important difference between photons in a liquid and photons in a solid is that a liquid cannot transmit transversely polarized waves-sound waves must be longitudinal. The speed of sound in liquid He4is 238m/s, and the density is 0.145g/cm3. From these numbers, calculate the photon contribution to the heat capacity ofHe4in the low-temperature limit, and compare to the measured value.

Sometimes it is useful to know the free energy of a photon gas.

(a) Calculate the (Helmholtz) free energy directly from the definition

(Express the answer in terms of T' and V.)

(b) Check the formula S=-(F/T)Vfor this system.

(c) Differentiate F with respect to V to obtain the pressure of a photon gas. Check that your result agrees with that of the previous problem.

(d) A more interesting way to calculate F is to apply the formula F=-kTlnZ separately to each mode (that is, each effective oscillator), then sum over all modes. Carry out this calculation, to obtain

F=8πV(kT)4(hc)30x2ln1-e-xdx

Integrate by parts, and check that your answer agrees with part (a).

Each atom in a chunk of copper contributes one conduction electron. Look up the density and atomic mass of copper, and calculate the Fermi energy, the Fermi temperature, the degeneracy pressure, and the contribution of the degeneracy pressure to the bulk modulus. Is room temperature sufficiently low to treat this system as a degenerate electron gas?

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