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Measurement of spontaneous magnetic fluctuations
Ph. Refregier, M. Ocio
To cite this version:
Ph. Refregier, M. Ocio. Measurement of spontaneous magnetic fluctuations. Revue de Physique Appliquée, Société française de physique / EDP, 1987, 22 (5), pp.367-374.
�10.1051/rphysap:01987002205036700�. �jpa-00245551�
Measurement of spontaneous magnetic fluctuations
Ph.
Refregier
and M. OcioService de
Physique
du Solide et de RésonanceMagnétique, CEN-Saclay,
91191 Gif-sur-YvetteCedex,
France(Reçu
le 7 octobre1986, accepté
le 26janvier 1987)
Résumé. 2014 Nous décrivons le
premier dispositif expérimental
utilisé pour mesurer les fluctuationsthermodynamiques
de l’aimantation d’unsystème
àl’équilibre.
Nousprésentons
le calcul ducouplage
de cesfluctuations avec le
système
de mesure, ensoulignant
les différencesqui
existent avec lesexpériences
demesure de
susceptibilité
alternative. Les spectres des deux verres despins
isolantsCdCr1,7In0,3S4
etCsNiFeF6
sontprésentés
dans l’intervalle defréquence 10-2 Hz, 102
Hz et nous montrons que leurdépendance
en
fréquence
est de type1/f .
Lacomparaison
de ces résultats avec des mesures desusceptibilité
alternative permet de penser que le théorème defluctuation-dissipation
estapplicable
pourCsNiFeF6.
Abstract. 2014 We describe the first
experimental
system used to observe the thermalmagnetic
fluctuations in amagnetic
system atequilibrium.
Wedevelop
the calculation of thecoupling
of spontaneousmagnetic
fluctuations to a
measuring
system,emphasizing
the difference with the classical case ofsusceptibility
measurements. We report the power spectrum of the two
spin glasses CdCr1.7In0.3S4
andCsNiFeF6
whichexhibit a
1/f dependence
in the range10-2
Hz to102
Hz.Comparison
between this observation and conventional a.c.susceptibility experiments
in the same range offrequency
supports theapplicability
of thefluctuation-dissipation
theorem forCsNiFeF6.
Classification
Physics
Abstracts07.55 - 75.90
1. Introduction.
Electrical noise due to the fluctuations of conduction electrons at thermal
equilibrium
was observed many years ago[1].
The observation gave rise to thetheory
of the linear irreversible processes whose first form - the famousNyquist
theorem[2]
- wasgeneralized
later to all lineardissipative systems [3].
This
general
form is the so called fluctuation dissi-pation
theorem(FDT) [4].
Neverthelessalthough
the FDT states that
magnetic
fluctuations must exist in realsystems,
it can be showneasily
thatthey
arevery difficult to detect
experimentally [5].
As amatter of
fact,
the detection ofmagnetic
fluctuations has been madepossible [5-8] by
the use ofSQUID magnetometers
whosesensitivity
is several orders ofmagnitude
better than that of classicalsystems.
On the other hand thereis,
at theday,
a renewal ofinterest for
thermodynamic
fluctuation studies onmagnetic materials,
sincethey
cangive
informationson the
dynamics
ofsystems
in the absence of any external disturbance. This is ofparamount import-
ance in disordered
systems,
likespin-glasses,
wherenon linearities with field and
ergodicity breaking
areexpected
below the transitiontemperature [9].
Fur-thermore,
fluctuation measurements are agood
toolto test the
validity
of the FDT in such non classicalsystems.
This paper is devoted to the
description
of anexperimental set-up
which has beenalready
used todetect
magnetic
fluctuations on severalinsulating spin glasses [5, 6]. Particularly
we derive the exper- imentalparameters allowing
toperform
aquantita-
tive
analysis
of the measured fluctuations.Finally,
it is worthnoting
that we areonly
interested here on
equilibrium fluctuations,
not oninduced
effects,
amongwhich,
forexample,
is the socalled « Barkhausen noise ».
2. Measurement of
magnetic
fluctuations.The measurements are
performed by
an inductivemethod. A
piece
ofmagnetic
material is inserted into apick
up coil connected to adetecting system.
At
the day
the bestsensitivity
is obtainedby using
asuperconducting
flux transformer followedby
aSQUID system.
Thus theexperimental
set up isessentially
amagnetic
fluxmeasuring system
withhigh sensitivity. However,
the way to relate themean square
magnetization
in the material to themean square flux in the
pick
up coil is not classical.As will be seen
below,
the resultdepends strongly
onArticle published online by EDP Sciences and available at http://dx.doi.org/10.1051/rphysap:01987002205036700
368
the
spatial
correlations of themagnetic fluctuations, giving
rise to two very different behaviors in the two extreme cases of short range andlong
range correla- tions(the
characteristiclength
isobviously
thecharacteristic size of the
pick
upcoil).
In the
experiments
described in thefollowing sections,
the correlationlength
is small. The case oflong
range correlations isanalysed
in order to makea
comparison
with classicalsusceptibility
measure-ments.
2.1 RELATIONS BETWEEN MAGNETIC MOMENT FLUCTUATIONS AND FLUX FLUCTUATIONS. - The
relationship
between themagnetization m(r, t)
2013defined as the
spatial density
ofmagnetic
moments03BC 2013 and the induced
flux 0
in apick
up coil can be derived from a classicalreciprocity
theorem ofmagnetostatics.
A volume elementdr3
located at rwith
magnetization m (r, t )
will induce in the coil acontribution to the flux
where
h (r )
is themagnetic
field that the coil wouldproduce
if it carried a unit of current(see Fig. 1).
Then
by integrating
over the volume V of thesample,
one obtainsFig.
1. - Schematicrepresentation
of acylindrical sample
in a
simple
coil anddescription
of thesymbols
used insection 2.
Let
~m03BC(r, t)m03BD(r’, t’)~ and ~~(t) ~(t’)~
bethe autocorrelation functions of
respectively
themagnetization
and the flux in thepick
up coil.03BC, 03BD = x, y, z. Then :
For the sake of
simplicity,
someassumptions
areuseful :
- the fluctuations of the
magnetization
are statio-nary
(so
is the flux in thecoil)
- the fluctuations of the
magnetization
are homo-geneous,
isotropic
and itscomponents
are statistical-ly independent.
Consequently :
Use of
equation (3)
and of the Wiener-Khintchine theoremyields :
where
~-2(03C9) is
thespectral density
of the flux in thepick-up
coil andm2 (r - r’, w )
is thespectral density
of the
spatial
correlations ofmagnetization along
one
arbitrary
axis.Equation (6)
shows that thecoupling
between thesample
and thepick-up
coildepends strongly
on thespatial
correlations. Ac-tually,
there are two extreme cases of interest : the limit oflong à£d
short correlationlengths.
One can solve
equation (6)
for the two extremecases :
a)
Case 1: the fluctuations are considered asspatially
uncorrelated. Thus :where
Mz(w )
is thespectral density
of themagneti-
zation
M (t ) along
onearbitrary
axis in the volume VM (t )
is an intensivequantity
and ingeneral
isdifferent from the local
magnetization m(r, t).
Equation (6)
becomeswith
b)
Case 2 : the correlations are considered to ex-tend over
large
distances ascompared
to the size ofthe coil :
and
equation (6)
becomeswith
It is
important
to note that inequations (8)
and(11) M 2
is thespectral density
of the totalmagnetic
moment of thesample
dividedby
thesquare of the volume. Relations
(8)
and(11)
showthat in both cases the flux fluctuations are pro-
portional
to themagnetization fluctuations,
but thecoefficients of
proportionality
arequite
different.Obviously
for verylarge
correlationlengths,
onefinds the relation which
corresponds
to a classicalmagnetization
measurement. Theintegral of |h(r)|2
appearing
in(9),
if extended over the whole space, isproportional
to the inductance of themeasuring
coil.We can characterize the
integral (9)
as « incoherent »(incoherent relatively
to the direction of thefield),
and note that it
gives
the energy of themagnetic
fieldh in the volume V. On the
opposite
theintegral (12)
could be considered as « coherent » since
algebraic compensation (by symmetry)
may appear in the volumeintegral.
2.2 THE USE OF THE FLUCTUATION-DISSIPATION THEOREM. - In classical cases, a relation exists between the fluctuations of
physical quantities
atthermal
equilibrium
and the deterministic response of thesystem
to theirconjugate
field. This relation is the so calledfluctuation-dissipation
theorem. Theconditions for its
applicability
are :i)
the response of the medium must beergodic
andlinear ; ii)
themedium must be
stationary.
From now on the c.g.s.e.m.
system
of units will be used. If thesusceptibility
is definedby
where
M (w )
is the response of themagnetization
toa
periodic
uniformmagnetic field,
thenprovided
h03C9 «
kB T,
thefluctuation-dissipation
theorem canbe written :
where T is the
temperature, kB
the Boltzman con-stant and
X "
is theimaginary part
of ~.In the limit of short range
correlations, equation (8)
leads toThis result can be
directly
obtained. When apiece
ofmaterial with
susceptibility
is inserted into a coil with free inductance
Lo,
theinductance will
change
towhere q
is afilling
factor. From theimpedance
of thecoil
(its dissipative part
is 4TrqLo w X ")
andusing
the
Nyquist
theorem one finds :Remember that
(where
theintegration
isperformed
over the wholespace outside the coil
wire).
Thus(8), (9), (17) yield
The
meaning
ofequation (19)
is that thefilling
factorq is the ratio between the
« operational »
- i.e.pondered by |h(r)|2
- volumeoccupied by
thesample
and the total «operational
» volume.In the case of short range correlations
with
expression (19)
for qs.By generalization,
forthe case of
long
range correlationswith
2.3 THE COUPLING TO THE
SQUID
SYSTEM. - Theexperimental flux 0 (03C9)
is measuredby coupling
thepick
up coil to aSQUID system.
Thepick
up coilLo,
thecoupling
coil to theSQUID L,,
and the leadsconnecting
themle,
form a closedsuperconducting
circuit called the flux transformer
(see Fig. 2).
Theflux transfer ratio is
given by
the relation :Fig.
2. - Schematicrepresentation
of thecoupling
system between thesample
and the SQUID.370
Where
ls is
the self inductance of theSQUID
and k is thecoupling
coefficient between the coilLS
and theSQUID (i.e.
their mutual inductance is kls Ls). Neglecting le
which is minimizedby twisting
theconnecting leads, e
is maximum whenLo
=LS
andthen
using equation (20)
or(22) depending
on thecase of interest one finds :
For a
given sample
thecoupling
between theSQUID
and the
magnetization depends
onLo only
via thefilling
factor q.2.4 COMPUTED VALUES OF THE FILLING FACTOR.
- Relation
(25)
can be written~2
SQUID
( 03C9)
= M2( w)k
2ls 4L0
V
aFi
i = s or 1(26)
where a is the radius of the
pick
up coil andFi
isgiven by
thefollowing
relations :a)
caseof short
range correlationsb)
caseof long
range correlationsWe
present
the numerical results in the case where thepick
up coil is a thinring
of radius a.(The
detailsof the calculations are
given
inAppendix A).
Thesample
is acylinder,
centred in thepick
upcoil,
with radius a - e andheight
2 A(see Fig. 1).
Infigures
3and
4, F,
andFI
areplotted
as a function of039B/a.
WhenAla
is small(039B/a « e/a )
themagnetic
field is
approximately
constantwithin
thesample,
and the
filling
factors areequal
in both cases.Moreover in this range q increases
linearly
with thevolume,
thus with039B/a.
Thefilling
factor deviatesfrom the linear behaviour since the modulus of the
magnetic
field decreasesmarkedly
as the distancefrom the
plane
of thering
increases. For short range correlations thefilling
factor reaches aale depen-
dent constant value in the
039B/a »
1region.
Incontrast q1
decreases as(039B/a)-1/2
in the sameregion.
The difference between the behaviour of thefilling
factors(or F)
is enhanced infigure
4 whereale
= 10 ascompared
tofigure
3 whereale
= 2.One sees that there is a factor 2 between
FS
andFI
whenAla
is of order 1.5. This can be understoodFig.
3. - Calculated values of thecoupling
factorsF in both cases of short
(Fs)
andlong (F1)
range correlations. Case of a badcoupling (a/e
=2).
F has nodimension in cgs unit.
Fig.
4. - The same as infigure
3, but for agood coupling (ale = 10).
as follows.
Indeed,
as we have mentioned in the end of2.1,
in the case oflong
rangecorrelations,
the fluxin the coil is due to a
spatially
constantmagnetization
and
only
the contribution of thelongitudinal
mag- netization mz does not cancelby symmetry.
On theother hand for short range
correlations,
the fluctua- tions areindependent
and there is nocompensation by symmetry.
The variations ofFs
andFI
as afunction of the relative
radius a e
forAla
= 2 arepresented
infigure
5. It is notsurprising
thatFS
increases toinfinity
witha/e (or a e ) like
log (a/e).
It has been seen that theintegral
of|h(r)|2
defines also the self inductance when takenFig.
5. - Calculated values of thecoupling
factorsF as a function of the free space between the
sample
andthe coil.
over the whole space, and it is well known that the self inductance for a
ring
rises toinfinity (like log (a/e))
when the wire radius decreases towardszero. In this limit of
large a/e,
theasymptotic filling
factor which can be obtained
(i.e.
for a closewinding
with a wire of radius
e) is q
= 0.55.2.5 DISCUSSION. - In our
experiments, powdered samples
were used. The characteristiclength
of thegrain
is smallcompared
to the size of themeasuring
coil.
Thus,
in the case ofspontaneous magnetic fluctuations,
the correlationlength
can not belonger
than the size of the
grain
and we areobviously
in thecase of short range
correlations,
thecoupling
factorbeing
qs.However,
if asusceptibility experiment
isperformed
with such asample
with a uniformapplied magnetic field,
the field induced correlation of themagnetization
will extend over the wholesample,
and thus thecoupling
factor will be ql. This would be also the case for fluctuations inducedby
aspurious
externalmagnetic field ;
it is worthnoting
that such a contribution is cancelled inour
experiment by
thegradiometric geometry
of thepick
up coil(see
Sect.3).
Since the
spontaneous
fluctuations of the totalmagnetization
are verysmall,
thecoupling
with thecoil must be
drastically optimized.
Thepreceding
results show that
only
thepart
of thesample
near thecoil is efficient in the
coupling. Contrary
to the caseof classical
susceptibility
measurements - i.e.long
range correlation - the
filling factor qs
increasessignificantly
when thesample
isbrought
near thecoil. Thus in
spontaneous magnetic
fluctuation ex-periments
the coil must be wound as close aspossible
to thesample.
3.
Experimental
3.1 EXPERIMENTAL SET-UP. - The measurements
are
performed
at 4.2 K in a4He
dewar. Twomumetal shields
(one
external at 300 K and one inthe
4He
vessel at 4.2K)
and a lead shield screen theexperimental
spaceagainst
the ambientmagnetic
field
(see Fig. 6).
In order to reduce thesensitivity
ofthe
measuring system
to the residual ambient mag- netic noise - which will induce uniformmagnetic
fluctuations in the
sample
- thepick
up coil is athird order
cylindrical gradiometer,
made of +3,
-
6, + 6, -
3 tums of niobiumwire,
with thefollowing
size : coil diameter = 7.2 mm, wire diame-ter = 0.1 mm, basic
spacing
betweenwindings
= 5 mm. The rod
shaped sample
is contained in asample
holder of size L = 30 mm, d = 6.5 mm. Thesample
holder can be movedmanually
from theoutside in order to allow noise
recordings
with thesample
in or out of thepick
up coils.Fig.
6. -Cryogenic
system used in theexperiments,
schematic
representation.
The R.F.
SQUID
is atype
MS03 from the LETI(C.E.N.G. Grenoble, France).
It exhibits white noise withoptimal
r.m.s. value10-4 03A60/ Hz
(where Vo
is the fluxquantum : 03A60
= 2.07X
10- 7gauss/cm 2)
atfrequencies
down to 0.5Hz,
with a cross-over to
1/ f
noise below 0.1 Hz[10].
The
SQUID coupling
coil is made out of 0.1 mmniobium wire.
Finally,
theoutput voltage
is transferred to a512 channels
digital spectrum analyser covering
therange
10- 2
Hz to 25 kHz. Theanalysed amplitudes
are converted into r.m.s. flux
threading
theSQUID
~s(03C9), by
means of thevoltage/flux
transfer ratio ofthe
SQUID
which is 8V/03A60.
Themeasuring
pro-372
cedure is the
following :
a record of the noisespectrum
of theempty system
is firstperformed,
then the
sample
is raised into thegradiometer
andthe noise
spectrum
isagain
recorded. The noisespectrum
of thesample
is the difference between thespectra
with thesample
in and out of the coil.As mentioned
above,
thepick
up coil is a third ordercylindrical gradiometer,
but whatever the consideredloop
of thiscoil,
thelength
of thesample
allows to consider the
asymptotic
value ofFs(039B)
as agood approximation.
The ratioa/e
is estimated to be 8 ± 1. Thus for asingle loop
the factorFs(039B)
is180 emu ± 20. The
spectral density
of the flux is(Eq. (20))
Then for a coil of N turns the flux is
proportional
tothe effective surface :
The total self inductance
Lo
of thegradiometer
has been
calculated, taking
into account the mutualself inductance between
adjacent windings (M3 _ 6
= 17 nH between three turns and six turnswindings,
andM6-6
= 26 nH between both six turnswindings) : Lo
= 1 150 nH ± 17 %. The low values of the mutual inductances betweenwindings
show thatthe
respective
fluxes areindependent.
Thus the totalflux in the coil is
where the sum is over the four
windings.
For ourgradiometer,
Finally,
the characteristics of the flux transformerare the
following : coupling
coilLs
= 930 ± 20nH, input
mutual inductance of the twistedpair le
= 30 ± 5 nH. Thus the flux transfer ratio is derived from(23), e = (5 ± 1) · 10-3.
3.2 RESULTS. - In this section we
report
the direct observation ofthermodynamic magnetic
fluctuations in the twospin glasses CsNiFeF6
andCdCri yino 384.
The choice of these materials has been determined from the
following
criteria :-
High
value ofX "
in thefrequency
range between10-2
and102
Hz at 4.2 K.- No contributions from
eddy
current noise asfor metallic
spin glasses
CsNiFeF6
is acrystalline
insulatorbelonging
to themodified
pyrochlore family.
Thecrystal
structure isfcc and the
magnetic
ionsNi2 +
andFe3 +
aredistributed at random on a network of corner-shar-
ing
tetrahedra with nearneighbour antiferromagne-
tic interactions
[11]. CdCr1.7InO.3S4,
also aninsulating compound,
is a dilutespinel system.
Themagnetic
ions
Cr3 +
occupy the B site of thespinel
structureand there are
competing
interactions between first- nearest(ferromagnetic)
andhigher
order(antifer- romagnetic) neighbours [12].
Thesamples
weremade of
powder
embedded with silicon grease, andpacked
into thesample
holder. Thedensity
factorfor the
CsNiFeF6 sample
was 0.60 and 0.46 for theCdCr1.7In0.3S4 sample.
Infigures 7
and 8 we havereported
the rms value of the noisespectrum
(in 03A60/ Hz
at theSQUID input)
as a function offrequency,
forCsNiFeF6
andCdCr1.7In0.3S4 respect- ively.
The noisespectrum
of theempty system
is alsodisplayed
in thefigures.
Eachspectrum corresponds
FREQUENCY (Hz)
Fig.
7. - R.M.S. noise ofCsNiFeF6 (upper curve)
aftersubtracting
the noise of the empty system(lower curve).
The noise is
given
as the R.M.S. flux at theinput
of the SQUID. Thewaiting
time aftercooling
the system is greater than 60 h.FREQUENCY
(Hz)
Fig.
8. - The same asfigure
7 forCdCr1.7InO.3S.
to an average of 256 successive
recordings.
To avoidageing effects,
which have beenreported
inprevious
works
[5, 6], recordings
have been taken afterhaving
spent
70 hours at 4.2 K. A clear1 / f
likedependence
of the noise power is seen in both materials.
It should be noted that in the
present results,
dueto the
improvement
on theSQUID characteristics,
and on the number of
averaged recordings,
theresolution of the
spectra
isstrongly improved
ascompared
to the resultsreported
in references[5]
and
[6].
This allows us toanalyse
in more details the behaviour of the out ofphase susceptibility X "
whichcan be calculated from
equations (15)
and(25) according
to the fluctuationdissipation
theorem.The result is
given
infigures
9 and10, showing
aslight departure
of the noise power from the1/ f slope.
The noise power is well accounted for in both materialsby
a1/f1 + x law,
with x ~ 0.02 forFREQUENCY(Hz)
Fig.
9. - Calculated values of~"(03C9)
fromfigure
8 forCsNiFeF6, using
the fluctuationdissipation
theorem. Forcomparison,
measured values ofX"(w ) (0)
arereported.
The calibration of
the X "
valuescorresponds
to the results of reference[11].
The dashedparallel
lines show ourestimate of the absolute calibration error.
FREQUENCY (Hz)
Fig.
10. - Calculated values of~"(03C9)
fromfigure 7
forCd Cr 1.7IIlo.3S4.
CsNiFeF6
and x = 0.02 forCdCr1.7In0.3S4.
Infigure
9the values of
x ",
measured in a conventional suscep-tibility experiment,
have also beenreported.
Withinthe
experimental
errors on the noise calibration(mainly
due to the uncertainties on the self induct-ance
values),
asatisfactory agreement
is obtained between both determinations of theimaginary
sus-ceptibility.
It thus appears that the fluctuation
dissipation
theorem is
obeyed
inspin glasses
below the transitiontemperature
asyet emphasized by
several authors[5, 6, 8] ; although
it isstrongly suspected
thatspin glasses
could benon-ergodic.
For anon-ergodic medium,
the «equilibrium
»stationary
noise revealsonly
the existence ofquasi equilibrium dynamics
inthe range of
experimental
times(here,
somemultiple
of the inverse of the lowest measured
frequency), given
the material hasspent enough
time at themeasuring temperature (the
so called « age »[13]).
The
good agreement
betweensusceptibility
andnoise measurements, obtained on the basis of the FDT
only
shows that similar conditions ofquasi equilibrium
hold in both cases ofexperiments.
Moreprecisely,
for the FDT to bevalid,
thesystem
must beergodic,
i.e. time averages must beequivalent
tothermodynamic
averages. Thus a «quasi equilibrium
state » could be understood as the average over that
part
of thephase
space thesystem
can visitduring
the
experimental
time t. Aslong
as the samerestrictive conditions
apply
to both kinds of measure-ments, a FDT relation could hold between
M2t(03C9)
and
Xt’(w ). Moreover,
it isworthy
to remember thatin the
present work, powdered samples
of about1
cm3
are used. This results in an effective averageover the
disorder,
which can occult at least to someextend a
non-ergodic
behaviour. These openprob-
lems will be examined in more detail with the aid of
a new
experimental
deviceallowing
variable tem-perature
measurements, as well ascoupling
tosamples
of reduced size.Acknowledgments.
The authors are indebted to H. Bouchiat and P. Monod for their fruitful discussions and remarks.
We also thank J.
Hammann,
M.Alba,
E. Vincent and R. Gerard Deneuville.Appendix
A.The purpose of this
appendix
is to derive tractable relationsgiving
thefilling factor q
in real exper- imentalgeometries.
The
filling
factor for arod-shaped sample coupled
to a thin
ring surrounding it,
has beennumerically computed.
The notations are thefollowing : a
is theradius of the
ring, e
is the distance between thering
and the
edge
of thecylinder,
and A is the halfheight
of the
cylinder (see Fig. 1).
374
The function
h (r )
isgiven by
classicalmagnetostat-
ics[14] ;
incylindrical
coordinates :where
and
K(k)
andE(k)
are thecomplete elliptic integrals
of first and second kind
[15].
The
filling
factors aregiven by
relations(9)
and(22) respectively
for short andlong
range cor- relations. Theproblem
is tocompute
theintegrals
For this purpose, reduced
quantities
are usedand
Then
In the case of
long
rangecorrelations hz
is theonly
.
non-vanishing
term in theintegral
Fs(03BB) and F1(03BB)
have the dimension of apermeability (no
dimension in e.m.u.units).
Finally,
thefilling
factor reads :where
Lo
is the self inductance of thering.
The
computed
values ofFs(03BB)
andF1(03BB)
arereported
infigures
3 and 4 for different values ofa/e,
andfigure
5represents
the variation ofFs
andFI
as a function ofale
for À = 2. See text fordiscussion of the results.
Actually,
theproblem
is the calculation of thefilling
factor for a realwinding
and not for an idealthin
ring. However,
aperturbative
calculation has shown that the correction of theprevious
results donot exceed 10 %. This is masked
by
theimprecision
in the determination of the
experimental
self in-ductance.
References
[1] JOHNSON,
J. B.,Phys.
Rev. 32(1928)
97.[2]
NYQUIST, H.,Phys.
Rev. 32(1928)
110.[3]
CALLEN, H. B. andWELTON,
T.A., Phys.
Rev. 83(1951)
34.[4]
KUBO, R., J.Phys.
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12(1957)
570.[5]
OCIO, M. BOUCHIAT, H. and MONOD, P., J.Phys.
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647.[6] OCIO,
M., BOUCHIAT, H. andMONOD,
P., J.Mag.
Mag.
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11.[7]
SLEATOR, T., HAHN, E. L.,HILBERT,
C. and CLARKE,J., Phys.
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1742.[8] REIM,
W., KOCH,R. H., MALOZEMOFF,
A. P.,KETCHEN,
M. B. andMALETTA,
H.,preprint.
[9]
For areview,
see forexample FISCHER,
K.H., Phys.
Stat. Sol.
(b)
116(1983)
357 and 130(1985) 13 ;
and PALMER, R.
G.,
Adv.Phys.
31(1982)
669.[10] Comparison
with the results of references[5]
and[6]
shows that the
sensitivity
of the SQUID has beenstrongly improved. Particularly,
the effect of4He
bath instabilities at lowfrequencies
has beenreduced
by
an order ofmagnitude.
[11]
PAPPA,C.,
HAMMANN,J.,
JEHANNO, G. and JACOBONI,C.,
J.Phys.
C 18(1985)
2817.[12]
ALBA, M., HAMMANN, J. andNOGUÈS, M.,
J.Phys.
C 15
(1982)
5441.[13] OCIO,
M.,ALBA,
M. and HAMMANN, J., J.Phys.
Lett. 46
(1985)
1101.[14] LANDAU,
L. D. and LIFSHITZ, E. M., Electronicsof
Continuous Media
(Pergamon Press) Vol. 8, p. 193.
[15] GRADSHTEIN,
I. S. andRYZHIK,
I.M.,
Tablesof Integrals,
Series and Products(Academic Press,
N.Y. and