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High field antiferro-, ferri-and paramagnetic resonance at millimeter wavelengths
S. Foner
To cite this version:
S. Foner. High field antiferro-, ferri-and paramagnetic resonance at millimeter wavelengths. J. Phys.
Radium, 1959, 20 (2-3), pp.336-340. �10.1051/jphysrad:01959002002-3033600�. �jpa-00236045�
336
HIGH FIELD ANTIFERRO-, FERRI-AND PARAMAGNETIC RESONANCE AT MILLIMETER WAVELENGTHS (1)
By S. FONER (2),
Lincoln Laboratory, Massachusetts Institute of Technology, Lexington, U. S. A.
Résumé. 2014 Les champs magnétiques pulsés ont été employés pour faire varier le couplage à
haute fréquence des systèmes antiferro-ferri- et paramagnétiques dans les ondes de longueur de 4
à 8 millimètres. On montre des exemples d’expériences de résonance pour chacun de
cessystèmes magnétiques et les résultats sont décrits et discutés. Pour compléter les
mesuresprécédentes,
on amesuré les susceptibilités magnétiques des monocristaux de MnF2 et Cr2O3. On indique ensuite
des applications
auxappareils à haute fréquence.
Abstract.
2014Pulsed magnetic fields have been employed to " tune " the high frequency magnetic
interactions of antiferro-ferri- and paramagnetic systems to 4
mmand 8 mm wavelengths.
Examples of
resonanceexperiments for each of these magnetic systems
aregiven, the nature of the information obtained is reviewed, and results of these experiments
aresummarized. Related magnetic measurements
arealso described ;
adetailed summary of susceptibility measurements for single crystal MnF2, CoF2 and Cr2O3 is given. Applications to high frequency devices
areindicated.
tE JOURNAL D E PHYSIQUE RADIUM: TOME 20, FEVRIER-MARS 1949,
Pulsed magnetic fields up to 750 kilogauss, pro- duced by capacitor discharge tbrough suitably designed coils [1], permit a variety of investiga-
tions [2], [3] which heretofore were not possible.
In particular, magnetic resonance phenomena
which involve large effective internal fields often
occur in the high-frequency ranges not yet attain- ed with present day technology. However, the high intensity pulsed fields may be used to
"tune "
the resonance to relatively low frequencies (35 to
70 kMcps) dictated by source power, pulse detec-
tion sensitivity and space limitations. In this paper, several examples of such resonances in anti- ferro- ferri- and paramagnetic materials are briefly
described in order to demonstrate the scope and limitations of the technique. Ih order to inter-
pret the resonance experiments additional detailed
magnetic data are often required. A summary of thèse magnetic measurements is also presented.
Because present information is most limited for
antiferromagnets, more details of both the reso-
nance and magnetic measurements are presented
for this class of materials. Finally, some brief
remarks concerning possible high-frequency appli-
cations of these materials and the pulsed field technique are also presented. The details of these various investigations are to be published elsewhere.
1. Antiferromagnetie Résonance.
-The reso- nance condition for
anuniaxial!antiferromagnetic
(1) The research reported in this document
wassup-
ported jointly by the U. S. Army, U. S. Navy and U. S. Air Force under contract with Massachusetts Institute of
Technology.
(2) Staff member.
single crystal, derived by Kittel [4], Keffer and
Kittel [5] and others [6] for Ho (2HEHA)1/2 is given by
where
6)is the angulâr frequency, y is ge/2mc, Hr,
is the exchange fieldi HA. is the anisotropy field,
ce =
XiliX.L (obtained from independent magnetic data), and Ho is the applied field parallel to the easy axis. Estimates show that for most antiferro- magnetics (Hx HA) is so large that low field obseri vation requires one4o one-tenth millimeter wave-
length radiation. The high field mode can be
observed at much lower wavelengths if Ho is sufli- ciently large [4], [5], The present capacitor dis- charge system [1], (2 000 uF, 3 000 V) and coils per- mit measurements at 70 kMcps with fields up to 600 kilogauss at room temperature and up to 350 kilogauss at 4.2 OK when a suitable Dewar
assembly is inserted into the pulsed field coil. This range of fields permits a survey of many antiferro- magnets. To date single-crystal MnF2, Cr20a, FeTi03, MnO, oc-Fe2O3, FeF2, CoF2, CoO, and NiO
have been examined ; the results for the first two
are summarized below, the next three appear to be more complex and are still being investigated,
and no resonance has yet ,been observed in the
last four. The important quantity, HA, is obtained
as a function of temperature from the résonance
data
-it is difficult to estimate
ormeasure by
other means. The normalized angular dependence
of this resonance for
ce =0, obtained by numerical methods, and shown in figure 1, indicates that for
low
(ù/y accurate alignment of the crystal is neces-
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphysrad:01959002002-3033600
337
sary for this resonance mode to be observed.
A second resonance for Ho > (2HEHA)1/2, just
after " spin-flop ", shoiild be observed when
Ho
=[2HgHA + (Coly)2]1n, The angular depen-
dence of this mode, shown in figure 2, indicates
FIG. 1.
-Angular dependence of antiferromagnetic
reso-nance
for
anuniaxial crystal. Symbols :
k0 - Hol(2H2 HA,)’/2, v = (cùly)1(211]EHA)112,
6 is the angle between Ho and the c-axis.
FIG. 2. - Angular dependence of second mode. The
curves on
the left of 8
=00 may be observable. Those
on
the right correspond to non-equilibrium conditions (not observable).
that for our parameters some good fortune is essen-
tial in order to observe this résonance. (This beha-
vior is borne out by many experiments.)
The results for MnF2 [7], [8], summarized in
figure 3, demonstrated that the molecular field
approximations and the dipolar source of Hd pre-
FIG. 3.
-Temperature dependence of (2HEHA) 1/2
for MnF2. Solid
curve -predicted Brillouin function for S
=5/2, triangles
-4
mmdata, circles and squares
-
8
mmdata,
crosses -high frequency data of Johnson and Nethercot (ref. 24).
dicted by Keffer [9] were satisfied in magnitude
and in temperature dependence. Most recent
results indicate that (2HrH&)112 is closer to 92 kilo-
gauss, but well within the experimental error.
Since the various interactions in MnF2 now appear to be well understood, this particular antiferro- magnet warrants a detailed analysis. Line-widths
as
narrow as 250 to 500 gauss at 36 kMcps were
observed at 4.2 OK. These measurements, corres- ponding to small differences measured near 80 kilo- gauss, are limited by various problems inherent
with pulse techniques. ’
Examples of the resonance data obtained for Cr203, again with Ho parallel to the easy axis, are
shown in figure 4. A constant value of
FIG. 4.
-Resonance field
versustemperature
for CrZ03 at two frequencies.
(2HEHJJl/2
=60 kilogauss from 4.2 oKto 200 OK
is calculated from this data if g
=2. 00 is assumed.
In contrast with the observations in MnF2, the
temperature dependence of (2HEHg)lJ2 does not
fit
aBrillouin function for spin 3/2. For Cr2O3, HE is about 2.1 X 10" gauss, (about four times that of MnF2), TN = 308 oR (TN = 68 oK for MnF2), and HA at low températures is 900 gauss (HA
=8 500 gauss in MnF2). Although the reso-
nance
data near TN agrees with Dayhoff’s re-
sults [10], the extrapolated temperature depen-
dence and absolute magnitude of (2HEHA)1/2 are quite different. The low temperature value of HA is about 1/3 that estimated by Dayhoff and 1 100 to 1/1000 of earlier estimates [11]. Appa- rently the lattice distorsions [12] which extend
over twice the température range investigated by Dayhoff, are important [3]. This is one of several
reasons which argue that low-frequency data near TN are not sufficient and that either high frequéncy
or
high field experiments are necessary. These
results,
aswell
asrecent detailed magnetic data,
indicate that Cr2O3 is not as simple as MnF 2. This
is not surprising because crystalline field inter-
actions are expected to be important for the C18+
ion, whereas for the Mn2+ ion, theory and experi-
ments indicate this effect is small.
Angular data taken at 4.2 oR and 77 oR for
v
~ 0.2 qualitatively agree with the results in
figure 1 ; an additional high field resonance
appears for 0 > 5° and tends toward ko = 1, and
ail resonances disappear for 0 greater than about
120. A broad very low field resonance was also observed for large 0. This is not predicted by the simple theory, and is being investigated further.
2. Ferrimagnetie Résonance.
---For the sim-
plest case (gi
=g2), the high frequency or " ex- change " resonance for
atwo sublattice ferri-
magnetic is given by [4]
where M1 + M2
=nM1 and HE == "’AMI. Here again Ho can be used to " tune " the resonance to
low frequencies, so that HE may be determined.
In this case, HA and n are determined from magne- tic data. Eiren for our pulsed fields, the range of
experiments is limited to materials of relatively
small HE or small n. When g1 g2 the usual
resonance is given by
w =( M 1 + M2) H
e
eis given y
w = 0(MllYl + M2/Yt) H0
and the " exchange " resonance is correspond- ingly more complicated. In particular, for large Ho,
alarge term proportional to Ho HE (gi - g2)
must also be considered in [ ]1/2 . The rare-earth
iron garnets are ideal for such observations because HA is small, compensation points occur
near
orbelow 300 °K, and single-crystals are obtai-
nable. However, appreciable corrections for the
field dependent magnetization must be made for
these materials [13]. Both the high and low field
resonances have been observed for single-crystal gadolinium and erbium garnets over a wide tempe-
rature range and were reported elsewhere [13].
The usual resonance showed the qualitative fea-
tures obtained earlier in polycrystalline mate-
rials [14].
3. Paramagnetie Résonance.
-The large tuning
range supplied by pulsed fields may also be used to
study paramagnetic resonance. The pulsed field technique is particularly useful when
alarge zero-
field splitting is present because then the usual
laboratory fields limit observations to small
changes of the energy levels. From the resonance
data, the various terms in the spin-Hamiltonian
can be determined. ,
In collaboration with Dr. Horst Meyer of Har-
vard University, this technique
wasapplied to paramagnetic resonance experiments of 02 mole-
cules (isolated from each other by about 8 A)
contained in
asingle crystal of g-quinol clathrate.
Meyer, O’Brien, and Van Vleck [15] have conclud-
ed from magnetic data that the 02 molecules are
influenced by the crystalline field, and that
alarge zero-field splitting, corresponding to about
4.15 OK, should be present. In this interesting
case both higb fields and high frequencies would
be required in order to observe paramagnetic reso-
nance of the 02 spins. Preliminary experiments
at 4.2 OK with pulsed fields and both 37 kMcps
and 71 kMcps showed this resonance and confirmed
thé large zero-field splitting.
4. Magnetie Measurements.
-Examination ’of the literature
onantiferromagnetics indicates that the data are too limited to permit accurate tests of numerous existing theories. The difficulties arise from two causes. First, few known anti-
ferromagnetic systems have " simple " structures
-
MnO, the classic material chosen for comparison
with theory, is quite complex. Second,
nomeasu-
rements have been made
on asimple antiferro- magnetic in sufficient detail and over a sufficiently
wide range of temperatures. The best results so
far were obtained in uniaxial anhydrous fluorides by Stout and Matarresse [16] and by Bizette and
Tsaï [17]. Bizette and Tsaï also demonstrated that measurements in single-crystal antiferro- magnets are essential.
Evaluation of the antiferro- and ferrimagnetic
resonance data also requires accurate magnetic
data over
awide temperature range. Detailed
single-crystal susceptibility and magnetization
data are easily obtained in
auniform magnetic
field with the vibrating-sample magnetometer [18].
Since such data are of general interest, some of the
results are summarized below.
339
As
anexample, the perpendicular susceptibility
of
asmall single crystal of MnF2. plotted on an expanded scale, is shown in figure 5. The results
FIG. 5.
-Relative perpendicular susceptibility
of MnF2
versustemperature.
of such measurements on MnF2 are : 1) xx varies
by less than 1 % from 4.2 OK to 50 °K ; of the numerous spin-wave theories, Ziman’s [19] predicts
that xi should be independent of temperature ; 2) if the break in ya or the XII curve is used as
acriterion, TN
=68 OK, just at the specific heat anomaly ; 3) data from 300 OK to 350 °K lead
to 0
~80 OK (here e is the constant in the Curie-
Weiss law, x
=c/(T + e)), and 4) above 20 °K
x,,
oc71.5, where
asbelow 20 oK, XI,
ocT1.8. On the other hand, similar measurements on CoF2 indi-
cate U increases with increasing temperature,
XII
ocT1.6 above 15 °K, and X
ocT3-8 below 15 oK, but
does not follow
asimple power law at lowest tempe-
ratures. Furthermore, XII does not approach
azero
value at low temperatures. Finally, the suscep-
tibility measurements on Cr20S show that X, is constant to within 1 % from 4.2 oK to 100 OK,
and then increases with increasing temperature, and that xjj reaches a small constant value below 20 OK, and does not show
asimple power depen-
dence below 20 OK.
Recently, 19F nuclear resonance data [20] of
various antiferromagnetic fluorides have been used
to examine the temperature dependence of the
sublattice magnetization, M. It should be rea-
lized that susceptibility measurements permit eva-
luation of HE, do not depend
onthe presence of
appropriate nuclear spins species, and may com- pare in accuracy to the resonance results. The low temperature 19F resonance data indicate that aMoc T3.5 for MnF2, and OlVI oc T5.0 for CoF2, where
AM
=M(0) - M(T). If M varies
as anappro-
priate Brillouin function, xjj should show
atempe-
rature dependence one power lower than given by
the M data. This is almost the case
-the devia- tions and the particular temperature dependence
must be explained by spin-wave theory. Magne-
tic measurements from 1.5 to 4.2 °K are being
made to study this problem in greater detail.
Magnetization measurements of various single- crystal rare-earth iron garnets generally agreed
with earlier polycrystalline data [21] in both magnitude and temperature dependence.
5. Applications to high; lfrequency Devices.
--The three magnetic classes discussed above all
have the géneral feature of very high frequency
response because of large effective internal fields.
Conversely, when millimeter and sub-millimeter
wavelength sources become available, one would expect that these materials will be useful in practi-
cal devices. Since it is not economically feasible
to produce continuous fields of the required magni- tude, magnetic systems with the appropriate " built
in " internal field will be required. Tuning could
be accomplished by varying the crystal orientation,
field Ho, and /or temperature. For example, one
could make
anantiferromagnetic millimeter wave modulator. One advantage of antiferromagnetic
devices would be that demagnetizing field effects would be negligible.
It was pointed our earlier that suitable high fre-
quency sources are not yet available. Recently
we have been investigating the possibilities of generation and amplification of millimeter waves with a pulsed-field Maser [22]. One proposed
scheme involves
athree-energy-level paramagnetic system to which a pulsed field is applied in order
to generate
anoutput frequency much higher than
the pumping frequency. Tests of this device are being made.
The author wishes to thank Dr. H. J. Zeiger for
valuable discussions, Dr. H. H. Kolm for his valuable contributions to the developement of the pulsed field system, Mr. B. Feldman for assistance with the experiments, and the numerous interested
scientists [23] from various institutions, who so kindly furnished the single crystals essential for
this work.
REFERENCES
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[2] FONER (S.) and KOLM (H. H.), Conf.
onMagnetism
and Magnetic Materials, Oct. 1956, Boston, Mass.
(AIEE Proc., Feb. 1957).
[3] FONER (S.), Fifth Inter. Conf.
onLow Temp., Phys.
Chem., 39-4 (Madison, Wis., Aug. 1957).
[4] KITTEL (C.), Phys. Rev., 1951, 82, 565.
[5] KEFFER (F.) and KITTEL (C.), Phys. Rev., 1952, 85,
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[6] NAGAMIYA, YOSIDA and KUBO, Advances in Physics, 1955, 4, 1.
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[10] DAYHOFF (E. S.), Phys. Rev., 1957, 107, 84.
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[14] PAULEVÉ (J.), C. R. Acad. Sc., 1957, 244, 1908 ; 1957, 245, 408.
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[16] STOUT (J. W.) and MATARESSE (L. M.), Rev. Mod.
Physics, 1953, 25, 338.
[17] BIZETTE (H.) and TSAI (B.), C. R. Acad. Sc., 1954, 238, 1575.
[18] FONER (S.), Rev. Sc. Instr., 1956, 27, 548 ; Bull.
Amer. Phys. Soc., 1957, Ser. II, 2, 237. A detailed account is to be published.
[19] ZIMAN (J. M.), Proc. Phys. Soc., London, 1952, A 65, 540, 548.
[20] JACCARINO, SHULMAN and DAVIS, Bull. Amer. Phys.
Soc., 1958, Ser. II, 3, 41.
[21] BERTAUT (F.) and PAUTHENET (R.), Part B. Suppl.
n° 5 IEE Convention
onFerrites, 1956, p. 261.
[22] FONER (S.), M. I. T. Lincoln Laboratory, Quarterly Progress Report, 1 Feb. 1958.
[23] CZERLINSKI (E.), JONES (R. V.), MEYER (H.), NAGA-
MIYA