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Cullity B.D. Introduction to Magnetic Materials. Second Edition (2008)

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114 DIAMAGNETISM AND PARAMAGNETISM

3.3The susceptibility of FeCl2 obeys the Curie–Weiss law over the temperature range 90 K to room temperature, with u ¼ 48K. Its molecular susceptibility at room temperature is 1.475 1022 emu/Oe/(g mol).

a.What is the effective magnetic moment in Bohr magnetons?

b.What are the spin-only values of J and mH (max)?

c.At an applied field of 8000 Oe, what is the value of the molecular field at 08C and at 1008C?

3.4Show that the Brillouin function B(J, a0) reduces to Equation 3.35 for J ¼ 1, to Equation 3.40 for J ¼ 12, and to Equation 3.45 when a0 is small.

3.5Plot the relation between M/M0 and H, according to quantum theory, for a material with g ¼ 2 and J ¼ 12 for fields up to 10 T and temperatures of 208C and 2K.

a.What is the effective moment?

b.What is the atomic susceptibility at 208C?

c.What percentage of the saturation magnetization is attained at a field of 10 T at 208C?

d.What field is needed to produce 85% of saturation at 2K?

3.6Repeat the plots of Problem , according to classical theory.

a.What is the atomic susceptibility at 208C?

b.What percentage of the saturation magnetization is attained at a field of 10 T at 208C?

c.How can the susceptibilities be the same (for classical and quantum theories) but the saturation percentages be different?

3.7The susceptibility of a-Mn is

766

 

10 6

A m2

766

 

10 6

m3

at 20 C:

A m 1 kg ¼

 

kg

 

 

 

 

8

The susceptibility of MnCl2 obeys the Curie–Weiss law, with u ¼ 3.0K and an effective moment of 5.7 mB per molecule. Calculate the susceptibility per atom of Mn in a-Mn as a percentage of the susceptibility per atom of Mn in MnCl2.

CHAPTER 4

FERROMAGNETISM

4.1INTRODUCTION

Magnetization curves of iron, cobalt, and nickel are shown in Fig. 4.1. These curves are partly schematic. The experimental values of the saturation magnetization Ms are given for each metal, but no field values are shown on the abscissa. This is done to emphasize the fact that the shape of the curve from M ¼ 0 to M ¼ Ms and the strength of the field at which saturation is attained, are structure-sensitive properties, whereas the magnitude of Ms is not. The problems presented by the magnetization curve of a ferromagnet are therefore rather sharply divisible into two categories: the magnitude of the saturation value, and the way in which this value is reached from the demagnetized state. We shall now consider the first problem and leave the details of the second to later chapters.

A single crystal of pure iron, properly oriented, can be brought to near saturation in a field of less than 50 Oe or 4 kA/m. Each cubic centimeter then has a magnetic moment of about 1700 emu, or each cubic meter a moment of about 1.7 MA m2 or MJ/T. At the same field a typical paramagnet will have a magnetization of about 1023 emu/cm3 or 1 A/m. Ferromagnetism therefore involves an effect which is at least a million times as strong as any we have yet considered.

No real progress in understanding ferromagnetism was made until Pierre Weiss in 1906 advanced his hypothesis of the molecular field [P. Weiss, Compt. Rend. 143 (1906) p. 1136–1139]. We have seen in the previous chapter how this hypothesis leads to the Curie–Weiss law, x ¼ C/(T 2 u), which many paramagnetic materials obey. We saw also that u is directly related to the molecular field Hm, because u ¼ rgC and Hm ¼ gM, where g is the molecular field coefficient. If u is positive, so is g, which means that Hm and M are in the same direction or that the molecular field aids the applied field in magnetizing the substance.

Introduction to Magnetic Materials, Second Edition. By B. D. Cullity and C. D. Graham Copyright # 2009 the Institute of Electrical and Electronics Engineers, Inc.

115

116 FERROMAGNETISM

Fig. 4.1 Magnetization curves of iron, cobalt, and nickel at room temperature (H-axis schematic). The SI values for saturation magnetization in A/m are 103 times the cgs values in emu/cm3.

Above its Curie temperature Tc a ferromagnet becomes paramagnetic, and its susceptibility then follows the Curie–Weiss law, with a value of u approximately equal to Tc. The value of u is therefore large and positive (over 1000K for iron), and so is the molecular field coefficient. This fact led Weiss to make the bold and brilliant assumption that a molecular field acts in a ferromagnetic substance below its Curie temperature as well as above, and that this field is so strong that it can magnetize the substance to saturation even in the absence of an applied field. The substance is then self-saturating, or “spontaneously magnetized.” Before we consider how this can come about, we must note at once that the theory is, at this stage, incomplete. For if iron, for example, is self-saturating, how can we explain the fact that it is quite easy to obtain a piece of iron in the unmagnetized condition?

Weiss answered this objection by making a second assumption: a ferromagnet in the demagnetized state is divided into a number of small regions called domains. Each domain is spontaneously magnetized to the saturation value Ms, but the directions of magnetization of the various domains are such that the specimen as a whole has no net magnetization. The process of magnetization is then one of converting the specimen from a multi-domain state into one in which it is a single domain magnetized in the same direction as the applied field. This process is illustrated schematically in Fig. 4.2. The dashed line in Fig. 4.2a encloses a portion of a crystal in which there are parts of two domains; the boundary separating them is called a domain wall. The two domains are spontaneously magnetized in opposite directions, so that the net magnetization of this part of the crystal is zero. In Fig. 4.2b a field H has been applied, causing the upper domain to grow at the expense of the lower one by downward motion of the domain wall, until in Fig. 4.2c the wall has moved right out of the region considered. Finally, at still higher applied fields, the magnetization rotates into parallelism with the applied field and the material is saturated, as in Fig. 4.2d. During this entire process there has been no change in the magnitude of the magnetization of any region, only in the direction of magnetization.

The Weiss theory therefore contains two essential postulates: (1) spontaneous magnetization; and (2) division into domains. Later developments have shown that both of these

4.2 MOLECULAR FIELD THEORY

117

Fig. 4.2 The magnetization process in a ferromagnet.

postulates are correct. It is a tribute to Weiss’s creative imagination that a century of subsequent research has served, in a sense, only to elaborate these two basic ideas.

4.2MOLECULAR FIELD THEORY

Consider a substance in which each atom has a net magnetic moment. Assume that the magnetization of this substance increases with field, at constant temperature, according to curve 1 of Fig. 4.3, as though the substance were paramagnetic. Assume also that the only field acting on the material is a molecular field Hm proportional to the magnetization:

Hm ¼ gM:

(4:1)

Line 2 in Fig. 4.3 is a plot of this equation, with the slope of the line equal to 1/g. The magnetization which the molecular field will produce in the material is given by the

Fig. 4.3 Spontaneous magnetization by the molecular field.

kTc
mgM0

118 FERROMAGNETISM

intersection of the two curves. There are actually two intersections, one at the origin and one at the point P. However, the one at the origin represents an unstable state. If M is zero and the slightest applied field, the Earth’s field for example, acts even momentarily on the material, it will be magnetized to the point A, say. But if M ¼ A, then line 2 states that Hm is B. But a field of this strength would produce a magnetization of C. Thus M would go through the values 0, A, C, E, . . . , and arrive at P. We know that P is a point of stability, because the same argument will show that a magnetization greater than P will spontaneously revert to P, in the absence of an applied field. The substance has therefore become spontaneously magnetized to the level of P, which is the value of Ms for the temperature in question. It is, in short, ferromagnetic. We may therefore regard a ferromagnet as a paramagnet subject to a very large molecular field. The size of this field will be calculated later.

We now inquire how this behavior is affected by changes in temperature. How will Ms vary with temperature, and at what temperature will the material become paramagnetic? To answer these questions, we replot Fig. 4.3 with a as a variable rather than Hm, where a ¼ mH=kT is the variable which appears in the theory of paramagnetism. Following Weiss, we will suppose that the relative magnetization is given by the Langevin function:

M

1

 

(4:2)

 

¼ L(a) ¼ coth(a)

 

:

M0

a

(Later we will replace this with the correct quantum-mechanical relation, namely, the Brillouin function.) When the applied field is zero, we have

a ¼ mHm ¼ mgM ¼ mgM M0 , kT kT kT M0

M

¼

kT

a:

M0

mgM0

(4:3)

(4:4)

M/M0 is therefore a linear function of a with a slope proportional to the absolute temperature. In Fig. 4.4, curve 1 is the Langevin function and line 2 is a plot of Equation 4.4 for a temperature T2. Their intersection at P gives the spontaneous magnetization achieved at this temperature, expressed as a fraction Ms/M0 of the saturation magnetization M0. An increase in temperature above T2 has the effect of rotating line 2 counterclockwise about the origin. This rotation causes P and the corresponding magnetization to move lower and lower on the Langevin curve. The spontaneous magnetization vanishes at temperature T3 when the line is in position 3, tangent to the Langevin curve at the origin. T3 is therefore equal to the Curie temperature Tc. At any higher temperature, such as T4, the substance is paramagnetic, because it is not spontaneously magnetized.

The Curie temperature can be evaluated from the fact that the slope of line 3 is the same as the slope of the Langevin curve at the origin, which is 13. Replacing T with Tc, we have

¼ 1 3

(4:5)

Tc ¼ mgM0 :

3k

4.2 MOLECULAR FIELD THEORY

119

Fig. 4.4 Effect of temperature on the value of spontaneous magnetization. Curve 1 is the Langevin function.

Therefore the slope of the straight line representing the molecular field is, at any temperature,

kT

¼

T

:

(4:6)

mgM0

3Tc

But the slope of the line determines the point of intersection P with the Langevin curve and hence the value of Ms/M0. Therefore Ms/M0 is determined solely by the ratio T/Tc. This means that all ferromagnetic materials, which naturally have different values of M0 and Tc, have the same value of Ms/M0 for any particular value of T/Tc. This is sometimes called the law of corresponding states.

This statement of the law is very nearly, but not exactly, correct. In arriving at the Langevin law in Equation 3.13, we considered the number n of atoms per unit volume and set nm ¼ M0. But n changes with temperature because of thermal expansion. Therefore, values of M=M0 at different temperatures are not strictly comparable, because they refer to different numbers of atoms. When dealing with magnetization as a function of temperature, a more natural quantity to use is the specific magnetization s, which is the magnetic moment per unit mass, because then thermal expansion does not affect the result.

If ng is the number of atoms per gram and m¯ the average component of magnetic moment in the direction of the field, then we can write Equation 3.13 as

ngm

 

s

1

 

(4:7)

 

¼

 

¼ coth a

 

:

ngm

s0

a

If we then define, for a ferromagnetic material, ss and s0 as the saturation magnetizations at TK and 0K, respectively, an exact statement of the law of corresponding states is that all

120 FERROMAGNETISM

materials have the same value of ss/s0 for the same value of T/Tc. The relation between the s and M values is

ss

 

Ms=rs

Msr0

,

(4:8)

 

¼

 

¼ M0rs

s0

M0=r0

where rs and r0 are the densities at TK and 0K, respectively. A change from M to s also involves a change in the molecular field constant g:

Hm ¼ gM ¼ gr(M=r) ¼ (gr)s:

(4:9)

Thus (gr) becomes the molecular field constant, and Equations 4.5 and 4.6 become

 

 

 

 

Tc ¼

mgrs0

,

 

 

(4:10)

 

 

 

 

 

 

 

 

 

 

 

 

 

3k

 

and

 

 

 

 

 

 

 

 

 

 

 

 

 

 

kT

 

 

T

 

 

 

(4:11)

 

 

 

 

 

 

¼ 3Tc :

 

 

 

 

mgrs0

 

Equation 4.4 therefore becomes

 

 

 

 

 

 

 

 

 

 

 

s

¼

 

kT

 

a ¼

T

a,

(4:12)

 

 

 

 

 

s0

mgrs0

3Tc

when the magnetization is expressed in terms of s.

Experimental data on the variation of the saturation magnetization ss of Fe, Co, and Ni with temperature are shown in Fig. 4.5. The temperature scales shown in Fig. 4.6 give the Curie points and the temperatures of phase changes and recrystallization for the three metals. The recrystallization temperatures are the approximate minimum temperatures at

Fig. 4.5 Saturation magnetization of iron, cobalt, and nickel as a function of temperature.

4.2 MOLECULAR FIELD THEORY

121

Fig. 4.6 Curie points (Tc), recrystallization temperatures [R], and phase changes in Fe, Co, and Ni. BCC ¼ body-centered cubic; FCC ¼ face-centered cubic; HCP ¼ hexagonal close packed. Ni is FCC at all temperatures.

which heavily cold-worked specimens will recrystallize; thus iron and cobalt can be recrystallized while still ferromagnetic, but nickel cannot. The three curves of Fig. 4.5 have similar shapes and, when the data are replotted in the form of ss/s0 vs T/Tc as in Fig. 4.7, the points conform rather closely to a single curve. Thus Weiss prediction of a law of corresponding states is verified. However, the shape of the curve of ss/s0 vs T/Tc predicted by the Weiss–Langevin theory does not agree with experiment. We can see this by finding graphically the points of intersection of the curve of Equation 4.7 and the lines of Equation 4.12 for various values of T/Tc. The result is shown by the curve labeled “classical, J ¼ 1” in Fig. 4.7. This disagreement is not surprising, inasmuch as we have already seen in Chapter 3 that the classical Langevin theory, which was the only theory available for Weiss to test in this manner, does not conform to experiment.

The Weiss theory may be modernized by supposing that the molecular field acts on a substance having a relative magnetization determined by a quantum-mechanical Brillouin function B(J, a0), as discussed in Chapter 3. In terms of specific magnetization, we have

s

¼

 

2J þ 1

coth

 

2J þ 1

a0

 

1

coth

a0

,

(4:13)

s0

 

2J

2J

 

 

2J

 

2J

 

 

where a0 ¼ mHH/kt from Equation 3.40. The straight line representing the molecular field is given by

s

 

kT

 

 

¼

 

a0:

(4:14)

s0

 

mHgrs0

 

122 FERROMAGNETISM

Fig. 4.7 Relative saturation magnetization of iron, cobalt, and nickel as a function of relative temperature. Calculated curves are shown for three values of J.

The slope of the Brillouin function at the origin is (J þ 1)/3J, from Equation 3.45. Therefore, the Curie temperature is

Tc ¼ mHgrs0 J þ 1

k 3J

¼ g(J þ 1)mBgrs0 :

3k

The equation of the molecular-field line can then be written

s0

¼

3J

Tc

 

s

 

J þ 1

 

T

a0:

 

 

 

 

 

(4:15)

(4:16)

(4:17)

Values of the relative spontaneous magnetization ss/s0 as a function of T/Tc can be found graphically from the intersections of the curve of Equation 4.13 and the lines of Equation 4.17. A different relation will be found for each value of J. The particular value J ¼ 12 is of special interest. Equations 4.13 and 4.17 then become

s

¼

 

s0

 

 

tanh a0

(4:18)

 

 

 

 

 

 

 

4.2 MOLECULAR FIELD THEORY

123

and

 

 

 

 

 

 

 

 

 

s

 

T

 

 

 

 

 

 

¼

 

a0:

 

(4:19)

 

 

 

s0

Tc

 

These can be combined to give

 

 

 

 

 

 

 

ss

 

¼ tanh

(ss=s0)

,

(4:20)

s0

(T=Tc)

which can be solved for ss/s0 as a function of T/Tc. The theoretical curves for J ¼ 12 and J ¼ 1 are plotted in Fig. 4.7. Either one is in fairly good agreement with experiment, with the curve for J ¼ 12 perhaps slightly better.

If J equals 12, the magnetic moment is due entirely to spin, the g factor is 2, and there is no orbital contribution. That this condition is closely approximated by ferromagnetic substances is also suggested by experimental values of g. Table 4.1 lists observed g factors for Fe, Co, Ni, and several ferromagnetic alloys, and they are all seen to be close to 2. We may therefore conclude that ferromagnetism in transition metals is due essentially to electron spin, with little or no contribution from the orbital motion of the electrons. At 0K the spins on all the atoms in any one domain are parallel and, let us say, “up.” At some higher temperature, a certain fraction of the total, determined by the value of the Brillouin function at that temperature, flips over into the “down” position; the value of that fraction determines the value of ss.

Up to this point we have put the applied field equal to zero and considered only the effect of the molecular field. If a field H is applied, the total field acting on the substance is (H þ Hm), where by H we mean the applied field corrected for any demagnetizing effects.

Therefore,

 

 

 

 

 

 

 

 

a0

¼

mH(H þ Hm)

¼

mH(H þ grs) ,

(4:21)

 

 

kT

 

kT

 

 

 

TABLE 4.1 Values of the g Factor

 

 

 

 

 

 

 

 

 

 

 

 

Material

 

 

 

 

 

g

 

 

 

 

 

 

 

 

 

 

Fe

 

 

 

 

 

2.10

 

 

Co

 

 

 

 

 

2.21

 

 

Ni

 

 

 

 

 

2.21

 

 

FeNi

 

 

 

 

 

2.12

 

 

CoNi

 

 

 

 

 

2.18

 

 

Supermalloy (79 Ni, 5 Mo, 16 Fe)

2.10

 

 

Cu2MnAl

 

 

 

 

 

2.01

 

 

MnSb

 

 

 

 

 

2.10

 

 

NiFe2O4

 

 

 

 

 

2.19

 

 

 

 

 

 

 

 

S. Chikazumi,

Physics of

Ferromagnetism, 2nd ed.

Oxford

University Press (1997), p. 69.