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HAL Id: jpa-00234402

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Submitted on 1 Jan 1951

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Magnetic saturation intensity and some other related

measurements

W. Sucksmith

To cite this version:

(2)

MAGNETIC SATURATION INTENSITY AND SOME OTHER RELATED MEASUREMENTS

By

W. SUCKSMITH. Sommaire. - Dans la

première Partie, l’auteur attire l’attention sur le fait que des mesures

exactes de l’aimantation spontanée n’ont été effectuées que dans un très petit nombre de cas. Les résultats pour le cobalt, qui possède un réseau hexagonal jusqu’au point de Curie et un réseau cubique centré au-dessus, sont donnés et discutés. Une augmentation de 1,5 pour 100 se produit à la tempé-rature de transition.

Dans la deuxième Partie, la variation de l’aimantation à saturation et le degré de l’ordre dans

quelques alliages binaires sont donnés. Dans la dernière Partie, on montre l’importance des mesures

de l’aimantation à saturation pour étudier la détermination de l’équilibre des phases. L’auteur cite

l’application heureuse de cette méthode au cas du système fer-carbone, caractérisé par quelques phases qui ne figurent pas à l’état d’équilibre.

LE JOURNAL DE PHYSIQUE ET LE RADIUM. 12,

1~~~?

I. Saturation

Intensity

Measurements and

the Iaaur of

Corresponding

States. - Of the three

ferromagnetic

elements,

the variation of the

spontaneous

magnetization

with

temperature,

has

been most

thoroughly

investigated

in the case of

nickel,

the most exhaustive and accurate

measu-rements

having

been carried out

by

Weiss and Forrer

[1].

For

iron,

the lower

temperatures

were

covered

by

the work of the same two authors

[21

whilst the

investigation by

Potter

[3]

deals with the range from room

temperature

to the Curie

point.

Cobalt,

which was

investigated by

Bloch

[4]

presents

additional

difficulties,

chiefly

on account

of the

large

crystalline

anisotropy.

Bloch’s

mea-surements in fields up to about i3ooo Oe have been hitherto

regarded

as

representing

the

tempe-rature variation of

spontaneous

magnetisation,

a conclusion which must be

regarded

as open to

considerable criticism on the

following

grounds.

In the first

place

the

abnormally high crystalline

anisotropy

makes the

approach

to saturation of the

polycrystalline

material very slow. This rate of

approach

decreases as the

temperature

is lowered

owing

to the increased

difficulty

of

attaining

satu-ration in the basal

plane,

i.e. at -

i goo C only

80 per 100 saturation is reached in an effective field of io ooo Oe. In addition there is the

diffi-culty

that at

ordinary temperatures polycrystalline

cobalt exists as a mixture of face-centred cubic and close

packed hexagonal

structures, the

pro-portions

of which vary

considerably according

to

the method of

preparation

and is

subsequent

thermal and mechanical treatment and is not

fully

control-lable.

Further,

there is a

phase

transition

beginning

at about

’700

C,

above which the metal is

wholly

face-centred cubic.

Lastly,

it is not

impossible

that the wide variations in the recorded

density

of cobalt exercise some

effect,

if

only

in

limi-ting

accuracy of measurement. The

only

method of

securing

more

precise

data on the variation of

spontaneous

magnetisation

with

temperature

appears to be to use

single crystals

of the

metal,

and to make measurements

along

the easy

direc-tion of

magnetisation

up to the transition

tempe-rature. Above the transition range, the

wholly

face-centred metal has

anisotropy

constants similar

to the other cubic

ferromagnetics.

Myers

and Sucksmith have

just

completed

this

investigation

with the

following

results.

By

slow

cooling

of the molten metal

(99.9

per Ioo

purity)

through

the

melting point

and the solid metal

thus

produced through

the transition range,

single

crystals

of

hexagonal

cobalt were

produced.

The variation of the saturation

intensity along

its easy direction of

magnetisation

shows the usual trend until a

temperature

of

4ooo

C is reached when the

phase

change

takes

place. Up

to this

temperature

quantitative comparison

of the results with other

ferromagnetic

materials is not

possible,

other than

on the somewhat

specious assumption

of a Curie

temperature

for the

hexagonal

material. On the

other

hand,

because of the close

agreement

in

part

of this range between our results and those of Guillaud

(see below),

it is not without interest to

extrapolate

such values as we have. The reduced

magnetisation

decreases from

unity

to a value

of

o.942

at

6730

abs. If we

extrapolate

these

values

according to j

=

2 ,

the Curie

temperature

2

is about 1150

abs.,

considerably

lower than the

Curie

temperature

for the cubic cobalt of

1404°

abs.

Assuming

a behaviour identical with that of nickel

(3)

431

(see

below),

leads to a Curie

temperature

at

about

1420°

abs. Whilst this close

agreement

is

wholly

fortuitous,

it can be taken to

point

to

the conclusion that the curve for

hexagonal

cobalt lies below

the j

curve

and close to that for the face centred nickel.

At the transition

temperature

the

magnetisation

rises

discontinuously

at the transition

by

about

1,5

per ioo

(see

f g.

I ),

and

thereupon

Fig. I.

follows a trend up to the Curie

temperature

identical

with that of nickel when the reduced

magneti-sation

G

is

plotted

against

the reduced

tempe-0

rature ( n )’

This means that in this upper

tempe-0

rature

region

the values are

greater

than for the theoretical curve

for j

= §.

Subsequent

heating

and

cooling through

the transition zone for both the

single

crystal specimens

and the

polycrystalline

material showed similar behaviour of a rather remarkable nature. With this thermal treatment

the

intensity

both above and below the transition increased

by

small amounts which decreased

pro-gressively

until the cobalt was 11 stabilized " after about 10

repetitions

of

the

thermal

cycle.

The

total increase amounts to a

change

at 3000

(i.

e. below the transition

region)

of about u =

0.4.

The

only possible

explanation

of this minor

anomaly

appears to be to

postulate

11

lattice mistakes "

in the structure.

The value of 6 for the

hexagonal phase

is found

to be 162.5 with pn =

1.72, and a Curie

tempe-rature of i 13 1

± 3° C,

the

density

at room

tempe-rature

being

p =

8.84!t

± o.oo5 in all cases. These

results are in fair

agreement

with the recent

measu-rements on a

single crystal

of cobalt of Guillaud and Roux

[5],

who obtained from measurements at and below room

temperature

c -=

16o.9

with

1.70. Their value for the ratio of the

intensity

at room

temperature

to that at absolute zero is about 1.005 and compares well with ours of

The best value for 7 for the cubic cobalt we estimate

to be

16~1.5

(p~ _ ~

this

being

obtained

by

extrapolation

from above the transition range and

consequently higher

than values obtained

by

others.

Comparison

of all the

ferromagnetic

elements

with

simple theory gives

the best accord

for j

== ~

7

with minor deviations in

general

common to all

threee

elements,

in that the measured

spontaneous

magnetisation

lies

slightly

below the theoretical

T

curves for small values of

(j’

, but at

temperatures

approaching

the Curie

temperature,

experimental

results exceed those demanded

by theory.

If one considers the

application

to

alloys,

in

particular

intermetallic

compounds,

the work of Guillaud

[6]

has added

considerably

to the

expe-rimental data available. For the three

compounds

for which data are available up to the Curie

tem-perature,

two of

these,

MnP and

Cr02’ approximate

more

closely to j

= ~

with

departures

of the same

type

as those

experienced

in the pure metals. On the other hand. Cr - Te

approximates

closely

to the

curve j

= 3.

The inherent

difficulty

in the utilization of all these measurements of saturation

intensity

lies in the determination of the

spontaneous

magnetisation.

At low

temperatures,

the law of

approach

is of

secondary

importance

and

extrapolation

to infinite field

gives

an

adequate

method in which the error

cannot be

large.

For

higher

temperatures,

however,

where the

change

oaf " saturation "

magnetisation

with

temperature

is

greater,

and the

approach

to

saturation is more

gradual, extrapolation

becomes

increasingly

difficult and uncertain. The

best,

method for

determining

the

spontaneous

magne-tisation comes from the

magnetocaloric

effect,

the rise of

temperature

on

magnetisation

is

directly

related to the variation of the square of the spon-taneous

magnetisation

with

temperature,

so that

T

only

for values

of 6

above about

o.6,

where there is a

sufflciently

great change

of cr with

T,

is it pos-sible to obtain measurable results.

Weiss,

however,

has made use of curves

giving

the field as a function of

temperature

for constant values of the

magne-tisation. These curves are linear for the

higher

values of the

field,

and

extrapolation

to zero field

gives

the

temperature

which

corresponds

to the

particular

value of 6

employed.

The two methods have been found to a gree for metal over the limited range of

temperature

where both measurements

are

possible,

but the accuracy is far from

adequate

to enable

satisfactory comparison

with

theory.

There is therefore a need for considerable extension of

magnetocaloric

measurements on

ferromagnetics.

Accurate measurement of the small

temperature

(4)

which accurate

knowledge

of the values of the

spontaneous

magnetisation

to be

considerably,

increased. As

yet,

no

attempts

have been made to

extend the measurements to any of the

important

alloys

which are the

subject

of

investigation

to

day.

In the absence of these

data,

one is

compelled

to

assume that the saturation

intensity

is an

adequate

measure of the

spontaneous

magnetisation,

this

assumption becoming increasingly

hazardous with the slower

approach

to saturation characteristic of

nearly

all

ferromagnetic alloys.

For

example,

the reduced curves

G,

T)

change shape

markedly

in solid solutions of a

ferromagnetic

and a

non-ferromagnetic

element. It is not

yet

definitely

known whether the

spontaneous magnetisation

curve is of the same

shape,

and more extensive

measurements of the

magnetocaloric

effect as well as

comprehensive

determinations of

.I~

curves over the whole

temperature

range are

requi-red. The writer is

initiating

experimental

work in the

hope

of

extending

the range of information of this nature.

II. Saturation

Intensity

Measurements and Order-Disorder. - The

writer,

in

investigations

on the Fe-Ni-Al

alloy

system,

has

previously

noted differences in the variation of saturation

inten-sity

of ordered and disordered

alloys.

At least three diff erent

examples

are

present

in this

system,

two of which have been the

subject

of further

inves-tigations

and will be dealt with below. The

third,

which is the

prototype

of the

permanent magnet

precipitation alloys,

showed saturation

intensity

data which fit in well with the now

generally

accep-ted view of the processes involved. The

(g, T)

curve for the annealed

alloy (two phase),

shows

behaviour characteristic of the

single phase type

with a Curie

temperature

approaching

closely

to that of pure iron and a saturation

intensity

of about 105

units,

i. e.

slightly

less than half that

of

iron,

thus

justifying

the view that the two

phases

are Fe and the

nonmagnetic

Ni Al. The

quenched

material, however,

has a

higher

saturation

intensity

than the annealed

alloy,

and after

tending

to a lower Curie

temperature

than pure iron up to

4ooo C,

gradually

shows the break up of the

single phase by

an arrest in the fall of the

magnetisation,

and

finally

at about 6ooO C reaches the

equilibrium

intensity

of the two

phase alloy.

Of other work in this

field,

probably

the most

important

is that on the 5o per 10o

Fe,

5o per I oo Co

superlattice.

Ellis and Greiner

[7]

had shown evidence of the existence of the

superlattice by

X-rays, supported

by

the additional evidence of the thermal arrest method.

Later,

Goldman and Smoluchowski

[8]

in

dealing

with

experimental

and theoretical data on saturation

magnetostriction

and

order,

show that the

magnetostriction

at

satu-ration increases

by

4o

per 10o upon

ordering.

In a

later

contribution,

the theoretical

prediction

that

the saturation moment should be about

4

per 100

higher

than in the random

alloy

has been confirmed. One

contributory

factor

leading

to the

high

permea-bility

of this

alloy (known

as

Permendur)

may be

due to the establishment of order

by appropriate

heat treatment. Some

support

of this view is

given by

work on the

Fe,Al

superlattice by

Ben-nett

[9].

The

(6, T)

curve for this

alloy,

both in the

quenched

and annealed states and for others

near this

composition,

show the usual

trend,

but the

intensities at low

temperatures

show notable features. Whilst the

intensity

of the ordered

alloys

falls off

smoothly

with increased aluminium content at a

gradually

increasing

rate,

the disordered

alloy

is more

magnetic

up to about 25 per i oo

Al,

but

drops

sharply

to a lower value than the ordered for

higher

aluminium content. This effect

persists

up to

about 3 o per 100. The reason for this is

presumably

due to the formation of

non-magnetic

Fe Al. In addition to this there is a

slight

discontinuity

in the

intensity-temperature

curve in the

neighbour-hood of the

ordering

temperature, though

the Curie

temperatures

of both

quenched

and annealed

specimens

do not differ

appreciably.

The effect

on the low field

properties

at room

temperature

was

investigated,

but the increase in

permeability

due to

ordering,

e. g. from about 2 ooo to 10 000,

was not marked. The

coercivity, irrespective

of the

degree

of order was less than i Oe in all cases. On the other

hand,

measurements of the

(~, H)

curve at

higher

temperatures

show

quite

different

results,

the

region

of

partial

order

showing

the

most marked effects. Here the

equilibrium

per-meability

fell from the

high

values of the order of some thousands to a value of about

4oo

just

below 5ooo C

rising again

with

increasing

tempe-rature. The

coercivity

reached a maximum of about 20 Oe in the same

region.

The difference in behaviour between

high

and low

temperature

measurements can be attributed to the time

required

for the establishement of order. A tentative

suggestion

for the

higher

coercivities in the transition

range

might

be made on the lines of the

existing

theories,

by postulating

small

regions

of order in a metrix of disordered

material,

with the

probable

accompaniment

of strains in the

boundary regions

between order and disorder.

An

investigation

into the

magnetic

properties

of the Fe-Cr

system

has been made

by

Ardron

[10].

Around the

composition Fe3Cr

there is

satisfactory

evidence of the existence of the

superlattice

both from

magnetic

saturation

intensity

and resistance

measurements.

Alloys

containing

20 and 27 per 100

chromium have low

temperature

intensities up

to

2,5

per 10o more for the ordered state than for

(5)

433

to a Curie

temperature

of about

8oo-gooo

C,

the Curie

temperature being

about

65~°

C for the 25 per 100

alloy.

The break down of order is

around

600° C,

so that the ordered

alloy

does not

reach its true Curie

temperature.

The

permea-bilities do not accord with the views

expressed

above,

the ordered

alloys showing

very low

permea-bilities,

but it has been

satisfactorily

shown that this is due to the

precipitation

of the

non-magnetic

sigma phase

which is

responsible

for the

high

coer-civity

with the

accompanying

low

permeability.

The writer has

previously

drawn attention to the

magnetic

evidence for the existence of the super-lattice

Ni3Fe [11].

The small

dependence

in the

ato-mic numbers of the two constituents makes

X-ray

evidence

difficult

but the

magnetic

saturation

intensity

measurements show a similar trend to those

already

referred to in the case of

Fe3Cr.

Fig. 2. - Variation of (c, T)

for ~5 atomic per 100 Ni, after cooling at 23~ : h.

Wakelin

(in progress)

has

recently

extended these

observations,

of which the evidence for

the

Ni3Fe

superlattice

is shewn in

figure.

The spe-cimens were cooled from about 600~ C to

4000 C

at 0.23° per hour to

produce

order,

after which more

rapid cooling

to room

temperature

was pos-sible.

Magnetic

measurements were then taken from low

temperatures

upwards.

Above 5000 C the order is

destroyed

too

rapidly

for the

high

Curie

temperature

of the

superlattice

to be

reached,

and the curve falls

rapidly

to meet the lower curve for the disordered

alloy.

Similar measurements

have been carried out on a range of

alloys containing

between

45

and 85 atomic per 10oo iron. At both

these limits no difference in

magnetic

behaviour for

cooling

rates between

quenching

and the above slow rate were

detected,

but at 55 and 80 per I o0

quite

measurable differences of the

type

shown

in

figure

2 were

observed,

thus

indicating

some

ordering.

Resistance

temperature

measurements of the well-known

shape

confirmed the

magnetic

observations,

but

only

for the 25 per i oo Iron

alloy

was it

possible

to show the existence of the

super-lattice

by

direct

X-ray

measurements. The maxi-mum increase of v on

ordering

was about

4

units in I 15 for

Ni3Fe,

this

decreasing

on both sides of this

composition.

The

extrapolated

Curie

temperature

fort his ordered

alloy

is

evidently

about 2oo-3ooO

higher

than that for the disordered material. On the basis of such evidence as is available at

present,

one may conclude that the ordered

binary

alloys

have in

general,

intensities around per 100

greater,

with Curie

temperatures

up to 200-300° C

higher

than for the disordered

alloys.

III. Saturation

Intensity

Measurements and

Magnetic

Phase

Analysis.

- At a conference

at the Institute of

Physics

in the

University

of

Strasbourg

in

1939,

the writer

presented

a paper

dealing

with an

apparatus

for the convenient

measu-rement of saturation intensities at all

temperatures,

irrespective

of the

shape

of the

specimen, together

with results which had been obtained on a suitable

ternary

alloy

system,

Much

infor-mation can be derived from

analyses

of this

type.

Fig. 3.

A recent and useful summary of the measurements

and the information to be derived has been made

by Guillaud

[12].

In

particular,

he has made a

study

of the

alloys

of manganese with

arsenic,

bismuth,

antimony

and silicon. Two

parameters,

the variation of saturation

intensity,

and the

tem-perature

at which

ferromagnetism

disappears,

can be utilized to

provide

information. In a solid solution both saturation

intensity

and Curie

tempe-rature

usually

decrease with addition of a

non-ferromagnetic

diluent,

initially linearly,

but with

increasing proportions

at a more

rapid

rate. At a

(6)

temperature appearing

if the second

phase

is

ferro-magnetic.

The saturation intensities at any

tem-perature

are

proportional

to the

products

of the

intensity

per unit mass and the

intensity

at that

temperature,

thus

providing

quantitative

infor-mation.

A detailed

example

of this

procedure

has been

given

in the

magnetic analysis

of the Iron-Silicon

System by Guggenheimer,

Heitler and Hoselitz

[13].

In the

non-equilibrium

condition,

no less than four

phases,

three

magnetic

and one

non-magnetic,

have

been’satisfactorily

isolated

(see f g. 3).

In

addition,

however, it has been found

possible

to follow out rates of reaction of

physical changes

bv means of continuous observations of the

intensity

changes.

By

suitable heat treatment,

i. e.

quenching

from

appropriate

temperatures,

the

approach

to

equilibrium

can be followed

by

means of the

magnetic

observations.

Fig. 4.

One

example

is

given

in

figure 11,

which shows

the effect of

heating

at 65oo C an

alloy

which was

quenched

from

I 100° C,

after

being

maintained

at that

temperature

a sufficient time to

produce

equilibrium.

The

proportions

of the

phases

«" and E are each about o.5

(the

E

phase

is

non-magnetic

and the amount

present

determined

by

difference. Continuous measurements of the

intensity

show the break down of the all

phase

into « and n.

Pro-longed heating

over a

period

of weeks showed the

gradual disappearance

of the n

phase (which

is

only

stable between about 8500 C and io5oO

C),

with the

accompanying

increase of a and s. ’The whole

of the

ferromagnetics regions

of this

alloy

system

. has been examined in this

way. The

accompanying

table

gives typical

examples

of the

weight

propor-tions at different

stages

in the reaction. The

calculated amount of Si is shown in the last column

and agrees well with the chemical

analysis.

The most recent

development

in this field has

been carried out

by

Crangle

and Sucksmith

(in

progress)

in an

investigation

into pure Iron-Carbon

alloys.

Here an

interpretation

of

equilibrium

condi-tions

presents

little

difficulty .

For low carbon

contents, up to about 1.2 per 100

by weight,

the

components

are ferrite

(a

saturated solution of

carbon in

body

centred cubic iron which contains

~ o.oo5

per Ioo C at room

temperature

and is therefore

magnetically indistinguishable

from pure

iron),

and cementite

Fe,C,

for which a- = ~ 66 with a Curie

temperature

of about 215° C. The dotted curve in

figure

shows

equilibrium

conditions and the amounts of cementite and ferrite can be

deter-mined from the

intensity-temperature

magneti-sation curve, the results

agreeing

well with the known constitution of the

alloys.

The examination of

quenched

material shows

clearly

and

quanti-tatively

the three known

stages

in the

tempering

process.

Measurements of the first

change

up to about 1 50°C

gives (Ci,

T)

curves of the

type

marked ~. in

figure 5

Fig. 5.

a, decomposition of martensite; b, extrapolation of reversible

part of graph; c, curve obtained on cooling from This graph is steeper than the equivalent diluted iron

graph, showing that the precipitate is ferromagnetic; d, start of the austenite transformation; e, transformation at constant temperature of non-magnetic retained

aus-tenite ; f , that there is here no marked inflection of the

curve shows that the precipitate is mainly something other than cementite; g, decomposition of the first precipitate;

h, region where there appears to be a precipitated mixture of Fe.,C and Fe20 C9. The approach of the " quenched "

and " annealed "

graphs depends on temperature but not

sharply on time.

which is known to be due to the breakdown of the

martensite solid solution. The identification of the

breakdown as distinct from a Curie

temperature

is indicated

by

the

irreversibility,

whilst the

pro-duction of a

ferromagnetic component

with a lower

Curie

point

than iron is shown

by

the

cooling

curve c.

being

steeper

than for iron mixed with a

non-ferromagnetic

material.

Subsequent heating gives

reversible values

along

c. The Curie

temperature

of the new constituent is not less than about 3ooo C,

and it is

possible

that it may be identified with

the s-carbide

Fe,C,

which

though

not

yet

prepared

(7)

435

has a Curie

point

of 380~ C. It is also

noteworthy

that Jack has obtained

X-ray

reflections of this carbide from a

high

carbon steel

tempered

at I20~ C.

The second

stage

shows the transformation of the

non-magnetic

austenite

(face-centred

cubic

iron)

into a

magnetic

form thus

giving

the increase

indi-cated at e. After this transformation is

completed

the

(c, T)

curve is reversible

along f .

This is

steeper

than that measured before the commencement

of the austenite breakdown and contains an inflexion

in the

slope

at about 2 150

C,

i. e. at the Curie

tempe-rature of cementite. The

implication

is that some cementite is

produced, though

whether this is due to the austenite or the lower

temperature

martensite transformation is not

yet

clear.

The third

tempering

stage

is characterised

by

a

sharp

fall in

magnetisation,

and becomes

fairly

rapid

above 26oo C. The

change

is

again

irrever-sible and is

presumably

due to the breakdown of a carbide to a

phase,

the

magnetic

intensity

of which is low at this

temperature.

At 3ooO C the

change

becomes very

slow,

but the

magnetic

intensity

remains

higher

than the annealed state

until a

temperature

of about 5oo-55oo C is attained. The

interpretation

of this

stage presents

considerable

difficulty.

The trend of the

(o-, T)

curve up to about 3ooo C can be

reproduced by assuming

that

the three constituents are

ferrite,

cementite and

iron

percarbide (Fe2oC9).

This latter has been

isola-ted and measured

magnetically.

The Curie

tempe-rature is

2 ~o°

C which agrees well with the values obtained

by

Pichler and Merkel

[14], though

sligh-tly higher

than the value of

2470

C

given by

Hofer,

Cohn and Peebles

[15].

Iron

percarbide

however,

decomposes

into cementite above

45oo

C,

and thus the

only ferromagnetic

constituent available in the

temperature

range 300°-500°C is the

ferrite,

the

quantity being

in excess of the

equilibrium

percen-tage.

Further work is in progress to

try

and elucidate these

points.

TABLE.

Results

of

Quantitative Magnetic

Analysis of

Some I’hree-Phase

cr-1Y Curçes,

and

Cornparison

with 1-rotal Silicon Content.

w = Relative amounts of each phase; £w - i.

It is

hoped

that the

examples

considered above

indicate the

importance

of

magnetic

saturation

intensity

measurements both in the field of

magnetic

phase analysis

and that of the

physical

interpre-’

tation of

magnetic phenomena.

Remarque

de M. Goldman. - 11 existe un

pr6-cedent pour

l’hypothèse

de Sucksmith relative à la coexistence des

phases

ordonn6e et

desordonnee

dans

Fe3Al.

Smoluchowski et Newkirk ont trouv6 que dans CoPt les

phases

ordonn6e et

desordonnee

pouvaient

exister en même

temps.

Dans un tel

syst6me,

le durcissement

magn6tique peut provenir

de la

precipitation

d’une

phase

ordonn6e

t6tragonale

dans une matrice de

phase

cubique

desordonnee.

Remarque

de 11,1. Hoselitz. -

During

the

magnetic

studies of iron nickel

alloys

of

composition

approxi-matively Fe3Ni,

I found that in the

non-magnetic

y state there existed a

superlattice

which can be detected

by

magnetic

measurement

owing

to the

fact that a 25 per 100 nickel

alloy undergoes

irre

versible

phase change

to the

magnetic

oc form when cooled to the

temperature

of

liquid

air. Thus

an

alloy

with 23 per 100 at.

nickel,

when annealed

at a

temperature

of 5250 C and

subsequently

cooled

to the

temperature

of

liquid

air,

showed three

magnetic

constituents. The two

equilibrium

concen-trations at 5250

C,

i. e.

containing

about g

and 27 per 100 nickel

respectively,

and a 25 per 100

nickel constituent which must have been formed

during

the

annealing

treatment

prior

to

cooling

in

liquid

air

(HOSELITZ,

J.

o f

Iron a Steel

Inst.,

I9!l4,

Part

I,

p.

193).

Remarque

de M.

Shockley.

- In connection with the iron aluminium

alloy

discussed

by

Prof. Sucks-mith it may be

appropriate

to remark that the in

immediate

neigborhood

of the critical

temperature

for order, there may be ordered and disordered

phases

present

of different

compositions.

The

observation

by

Prof. Smoluchowski of ordered and

(8)

by

Prof. Goodman and the

theory

of

phase

diagrams

requires

in

general

that the

compositions

be diff

e-rent. The difference in

composition

may lead to stresses and other discontinuities

’which

contribute

to the coercive force.

-Remarque

de iV. Sfoner. - 11 faut

souligner

l’im-portance

de ces mesures

pr6cises

de la variation

de 1’aimantation

spontan6e

avec la

temperature.

Comme

je

1’ai

deja

dit,

les resultats ne sont pas

en accord avec la theorie

classique

pour j

2

ni avec la th6orie des electrons collectifs.

Mais,

en

prin-cipe

on

peut

d6duire des d6saccords comment les interactions

d’6change

varient avec

1’aimantation,

ce

qui

est tr6s

important

du

point

de vue

th6orique.

Les mesures

magn6to-caloriques

que M. Sucksmith a commene6es a faire sur les

alliages

pourront

aussi donner des

renseignements pr6cieux.

L’analyse

des r6sultats

exp6rimentaux pr6sente beaucoup

de difficultes mais nous pensons

pouvoir d6velopper

a Leeds des m6thodes

convenables;

des mesures

pr6cises

comme celles de M. Sucksmith sont

indis-pensables

pour cela.

Remarque

de M. Néel. - Les désaccords

signal6s

par M. Stoner

peuvent

provenir

non seulement

de la variation des interactions

d’6change

avec 1’aimantation mais aussi de la variation avec la

temperature.

Remarque

de ll4I. Van Vleck. - 11 faut

souligner

le fait

qu’a

basse

temperature

le calcul de 1’aiman-tation a saturation est très difficile. On

peut

com-prendre

pourquoi,

a basse

temperature,

la dimi-nution de 1’aimantation par

rapport

a sa valeur pour T = o est

plus grande

exp6rimentalement

que la diminution calcul6c avec le mod6le du

champ

mol6culaire;

on doit

plut6t

utiliser la m6thode des

ondes de

spin qui

donne une loi

d’approche

de la

forme a

= o~o ~

Aux basses

temp6ratures,

il

s’agit

de fluctuations li6es aux ondes de

spin

et non

comprises

dans la th6orie du

champ

mole-culaire. Les difficultés relatives aux basses

temp6-ratures se

pr6sentent

d’une

façon f rappante

dans la

m6thode de Bethe-Peierls

d6velopp6e

pour le

magn6-tisme par Peter Weiss. Anderson a observe

qu’avec

cette m6thode il existe une

temperature

au-dessous

de

laquelle

il ne devrait pas exister de

f

erromagne-tisme. On doit attribuer ce r6sultat absurde au fait

qu’a

basse

temperature

il existe des corr6lations

et des

longues

ondes

qu’on

ne

peut

pas traiter

facilement par la m6thode de Bethe-Peierls.

REFERENCES.

[1] WEISS and FORRER. 2014 Ann.

Physique, 1926, 5, 153.

[2] WEISS and FORRER. 2014 Ann.

Physique, 1929, 12, 279.

[3] POTTER. - Proc.

Roy. Soc., 1934, 146, 362.

[4] BLOCH. 2014 Z.

Physik, 1930, 64, 817, and 1933, 81, 790.

[5] GUIELLAUD and Roux. - C. R. Acad. Sc., 1949, 229,

1062,

[6] GUILLAUD. - C. R. Acad. Sc., 1946, 222, 1110.

[7] ELLIS and GREINER. - Bell

Telephone Tech. Publ., B 1257.

[8] GOLDMAN and SMOLUCHOWSKI. 2014 Phys. Rev., 1949, 75,

140, 310.

[9] BENNETT. 2014 Thesis. Sheffield, 1949

(unpublished).

[10] ARDRON. 2014 Thesis. Sheffield, 1949 (unpublished).

[11] SUCKSMITH. - Proc.

Roy. Soc., 1939, 171, 525.

[12] GUILLAUD. - Rev. Métall., 1949,

46, 453.

[13] GUGGENHEIMER, HEITLER and HOSELITZ. - J. Iron and

Steel Inst., 1948, p. 192.

[14] PICHLER and MERKEL. 2014 U. S. Bureau

of Mines Techn,

Paper 718, 1949.

[15] HOFER, COHN and PEEBLES. 2014 J. Amer. Chem. Soc.,

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