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EFFECT OF IMPURITIES ON THE NÉEL
TEMPERATURE AND SPIN-FLOP FIELD IN THE
QUASI ID ANTIFERROMAGNET CsMnCl3
×2H2O
E. Velu, J. Renard, G. Corbel
To cite this version:
JOURNAL DE PHYSIQUE Colloque
C6,
supplPmen/ au no8,
Tome39,
aolit1978,
pageC6-7 17
EFFECT
OF
IMPURITIES
ON
T H EN ~ E L
T E M P E R A T U R EAND SPIN-FLOP
FIELD IN THE
QUASI
ID
A N T I F E R R O M A G N E TC S M ~ C ~ ~ ~ ~ H ~ O
E. Velu, J.P. Renard and G. Corbel
I n s t i t u t d'Electronique Fondamentale, Laboratoire Associd au CNRS, BEZtirnent
220,Universi
t dParis-Sud,
91405 Orsay Ceder, France
Rdsum6.- Nous avons mesurd en fonction du champ et au-dessus de 1,2
K
la susceptibilit6 magn6tique parallsle de lrantiferromagn6tique en chafne CsMnC13,2H20(CMC) dope ar desg
impuretds de Cobalt et Cuivre en concentrations atomiques respectives & 3,4x10- et 1,7x10-~ 3,4x10-~. Nous observons un net abaissement de la tempdrature ae NQel T di3 a m impure- tCs. De
T
et de la variation thermique de la susceptibilit6 au-dessus fle 30K,
nousN
dBduisons la valeur absolue de l'interaction d'dchange Cu-Mn dans CMC dopd au Cuivre. Nous avons dgalement determind la ligne de spin-flop de CMC avec impuret6s. On constate un abaissement du champ de spin-flop qui n'est pas compatible avec les theories de champ moyen.
Abstract.- The magnetic susceptibility of the quasi-ID antiferromagnet CsMnC13.2H20 (CMC) doped by cobalt and copper impurities in respective atomic concentrations 3.4x10-~ and 1.7~10 2, 3.4x10-~ has been measured versus field and temperature down to 1.2
K.
A net decrease of the NEells temperature TN due to impurities was observed. From T andN temperature dependence of susceptibility above 30 K in Cu doped CMC, the absolute value of the Cu-Mn superexchange interaction was determined. In addition the spin-flop field is strongly depressed by impurities. The observed reduction is not explained by mean- field theory.
Several studies on CsMnC13.2H20 (CMC) /I, 2/ have shown that this salt becomes antiferroma- gnetic below Neel's temperature
T
= 4.89 K. WithN
temperatures above TN, CsMnC13.2H20 is well repre- sented by I-D Heisenberg model. The exchange inte-
++
gral between neighbor Mn belonging to the same chain is about
-
3 K, the interchain exchange about-
0.03 K. Such a system is very sensitive to the presence of impurities. In effect, the latter cut the chains, shorten the correlation length and therefore modify Ndel's temperature.The effect of the impurities on the magnetic susceptibility has been theoretically studied by Richards /3/ for a system of classical spins with spin 1/2 impurities.++
The theory can be applied to CMC (Mn
,
S
= 5/2)++
which contain copper impurities (Cu
,
S' = 1/21. We prepared 3 monocrystals of CMC with impurities using the formula CsMnX
C13.2H20. The concen-l-X
Xtration X was measured by microanalysJs (table
I).
1) MAGNETIC SUSCEPTIBILITY VARIATION OF TN.- The magnetic susceptibility is measured using a mutual
inductance bridge functionning at 70
Hz,
at tempe- ratures varying between 1.2 and 77 K. The tempe- rature is measured with a carbon resistance, cali- brated using a CrK alum and recalibrated at each experiment at the fixed points 4.2 and 7.18K
temperature of the superconductive transition of lead.
We have thus studied the molar parallel s u s c e p t i b i l i t y ~ ~ along the easy axis b of pure CMC and of the sample 3 between 4.2 and 77
K
(figure 1). An increase o f x b due to the impuri- ties can be noticed.
Fig. 1 : Molar parallel susceptibility Xb versus T of pure CMC (black circ1es)and of the sample 3
(white circles). The crosses are the experimental data of the reference 2.The heavy line is calcula- ted with J/k=-3.17K/3/ and x=O. The dotted lines are calculated for X ~0.034,
J/k
=-
3.17 K ~ ' / k= -1.85 K(1ong dots)and J1/k(short dots)=+ 1.85
K.
The comparison o f
xb
o f p u r e CMC t o R i c h a r d ' s theo- r e t i c a l c u r v e a l l o w s u s t o d e t e r m i n e t h e i n t r a c h a i n++
exchange betweenMn
J / k =-
(3.172
0.03)K. T h i s v a l u e i s i n a c c o r d a n c e w i t h p r e v i o u s r e s u l t s . The d i f f e r e n c e between t h e t h e o r y and t h e e x p e r i m e n t below 25 K i s e x p l a i n e d by t h e f a c t t h a t , f o r T < 25 K t h e a n i s o t r o p y b e g i n s t o be f e l t w h i l e t h e t h e o r y d o e s n o t t a k e t h i s i n t o c o n s i d e r a t i o n .The measure o f
xb
between 4.2 and 7 K a l l o w e d u s t o d e t e r m i n e N l e l ' s t e m p e r a t u r e o f t h e 3 s a m p l e s and o f t h e p u r e CMC ( t a b l e I ) . I n e f f e c t , i f we p l o txb
v e r s u s T we o b s e r v e a r u p t u r e i n t h e s l o p e a t TN.
2 ) SPIN-FLOP LINE.- At T < TN, t h e s p i n - f l o p f i e l d HSF i s o b t a i n e d b y m e a s u r i n gxb
v e r s u s a s t a t i c magnetic f i e l d , p a r a l l e l t o t h e e a s y a x i s b.xb p r e s e n t s , a t t h e s p i n - f l o p f i e l d a n e t peak. The peak i s narrow f o r t h e p u r e sample e l l i p s o i d and much l a r g e r f o r t h e impure samples ( p a r a l l e l e p i - p e d s ) . F o r t h e p u r e s a l t HSFi s
measured a t_+
10 Gw h i l e t h e u n c e r t a i n t y of HSF r e a c h e s
2
100 G f o r t h e sample 3 a t a b o u t 3 K ( F i g u r e 2 ) . The sample 2 p r e s e n t s two s u s c e p t i b i l i t y p e a k s which a r e a b o u t 250 G a p a r t . The s p l i t t i n g between t h e s e two peaksi s r e p r e s e n t e d i n t h e F i g u r e 2 b y t h e u n c e r t a i n t y b a r s .
T a b l e I
We u s e T h o r p e ' s c a l c u l a t i o n s / 4 / t o de- duce, from t h e measured TN, t h e v a l u e o f t h e in- t r a c h a i n exchange Cu-Mn. J ' / k . The g e n e r a l formula o f t h e c o r r e l a t i o n l e n g t h f o r c l a s s i c a l s p i n s i s :
T)
E ( l-
X) / U ( + 2x(1-
X) u t 2 I-
( 1-
X)[ " l
-
x ( l-
x ) u ' 2 25 S ( S + I )-
w i t h u = c o t h kT kT 25 S ( S + l )'
2 J ' S S ' kT U ' = c o t h-
-
kTW'SS'
S(x, T N ( x ) ) TN(x) The r e l a t i o n = - E(0, T N ( 0 ) ) TN(0) ( 5 ) p e r m i t s u s t o c a l c u l a t e [ ~ ' / k ( i f we know J / k ( t a b l e I ) . T h e r e f o r e we c o n c l u d e I J f / k l = ( 1 . 8 52
+
0.10) K.The TN of t h e samples 2 and 3 , c a l c u l a t e d on t h e b a s e of t h i s v a l u e o f ( J ' / k l a r e r e s p e c t i - v e l y 4.60 and 4.34 K , which a r e c o n s i s t e n t w i t h t h e measured v a l u e s . The comparison of
xb
v e r s u s T t o t h e t h e o r e t i c a l c u r v e s /3/ c a l c u l a t e d f o r J ' / k = 1.85K and-
1.85 K s h o u l d a l l o w u s t o d e c i d e i f t h e ex- change Cu-Mn i s f e r r o - o r a n t i f e r t o m a g n e t i c (£ i g u r e I ) . I n p r a c t i c e t h i s comparison h o l d s t r u e o n l y when T > 3 0 K and t h e n t h e d i f f e r e n c e between t h e two2 3
TrKl
F i g . 2 : S p i n - f l o p l i n e s o f t h e f o u r s t u d i e d samples. Black c i r c l e s : p u r e CMC, b a r s : Sample 1 , w h i t e c i r c l e s : sample 2, t r i a n g l e s : sample 3. The heavy l i n e s r e p r e s e n t t h e l a w s H (T) o f t a b l e I . The d o t t e d l i n e r e p r e s e n t s t h e sp%-flop l i n e of p u r e CMC i n r e f e r e n c e / l / . G e n e r a l l y , t h e t e m p e r a t u r e dependence o f HSF i s w e l l f i t t e d by a l i n e a r f u n c t i o n , e x c e p t p e r h a p s i n t h e v i c i n i t y o f t h e b i c r i t i c a l p o i n t (sample 3 ) . Our s p i n - f l o p l i n e o f p u r e CMC i s s l i g h t l y d i f f e r e n t from t h e one i n r e f e r e n c e / I / . We o b s e r v e a c o n s i d e r a b l e d e c r e a s e o f HSF due t o t h e i m p u r i t i e s . Recent t h e o r e t i c a l work / 6 / sug- g e s t t h a t t h e e f f e c t of d i a m a g n e t i c i m p u r i t i e s i n c o n c e n t r a t i o n X on t h e p h a s e d i a g r a m i s a l i n e a r s c a l i n g of r a t i o I-X. T h i s r e s u l t i s n o t v e r i f i e d i n t h e p r e s e n t c a s e which we c a n a t t r i b u t e t o two r e a s o n s : t h e q u a s i I-D c h a r a c t e r of t h e s y s t e m and t h e paramagnetism o f t h e i m p u r i t i e s which c o u l d modify t h e m a g n e t i c a n i s o t r o p y .
References
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a
(1969) 259./2/
Kobayashi,H.
and Tsujikawa, J., J. of Low.Temp. Phys.10
(1973) 6 2 1 .
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14 (1976) 1239. / 4 / Thorpe,M.F.,
J. Physique36
(1975) 1177./ S / Dupas, C. and Renard, J.P., Phys. Rev.
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