fe g = 0 · conclusions • the dilution of ls co3+ in ndfe 1-xco xo 3 is equivalent to the...
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![Page 1: Fe G = 0 · Conclusions • The dilution of LS Co3+ in NdFe 1-xCo xO 3 is equivalent to the inclusion of magnetic vacancies in the system • The vacancies uncompensate the AF Fe](https://reader033.vdocuments.us/reader033/viewer/2022042921/5f6896e56f72247d0c666733/html5/thumbnails/1.jpg)
x > 0 : distribution of internal fieldsx > 0 : distribution of internal fields
Relevant parameter: G = level of uncompensationRelevant parameter: G = level of uncompensation
Fe
Co
Nd
G = 0G = 0
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x > 0 : distribution of internal fieldsx > 0 : distribution of internal fields
Relevant parameter: G = level of uncompensationRelevant parameter: G = level of uncompensation
Fe
Co
Nd
G = 1G = 1
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x > 0 : distribution of internal fieldsx > 0 : distribution of internal fields
Relevant parameter: G = level of uncompensationRelevant parameter: G = level of uncompensation
Fe
Co
Nd
G = 2G = 2
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x > 0 : distribution of internal fieldsx > 0 : distribution of internal fields
Relevant parameter: G = level of uncompensationRelevant parameter: G = level of uncompensation
Fe
Co
Nd
G = 0G = 0
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x > 0 : distribution of internal fieldsx > 0 : distribution of internal fields
Relevant parameter: G = level of uncompensationRelevant parameter: G = level of uncompensation
Fe
Co
Nd
G = 4G = 4
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x > 0 : distribution of internal fieldsx > 0 : distribution of internal fields
0
20
40
60
80
100
0 1 2 3 4
x = 0.03, x = 0.97
x = 0.1, x = 0.9
x = 0, x = 1
x = 0.2, x = 0.8
0.5
% d
e io
nes
Nd
G (en iones Fe3 + descompensados)
Relevant parameter: level of uncompensationRelevant parameter: level of uncompensation
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x > 0 : sum of Schottky contributionsx > 0 : sum of Schottky contributions
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x > 0 : sum of Schottky contributionsx > 0 : sum of Schottky contributions
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x > 0 : sum of Schottky contributionsx > 0 : sum of Schottky contributions
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x > 0 : sum of Schottky contributionsx > 0 : sum of Schottky contributions
0 1 2 3 4 5 60.0
0.2
0.4
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ConclusionsConclusions
• The dilution of LS Co3+ in NdFe1-xCoxO3 is equivalent to theinclusion of magnetic vacancies in the system
• The vacancies uncompensate the AF Fe ordered sublattice,increasing the Fe-Nd interaction and
inhibiting Nd cooperative order for x ≥ 0.1
• A mean field model for the parent compound has beenmodified to take account for low doping NdFe1-xCoxO3 (x ≤
0.1)
• It is appealing to suggest that this is the mechanism fornegative magnetization in manganites (isntead of
ferrimagnetism)
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RMORMO33 : Model systems : Model systemsM-M, M-R, R-R interactions.M-M, M-R, R-R interactions.
• M-M
• M-R
•R-R
1000 K
100 K
10 K
1 K
M antiferro order (Cr, Fe, Ni, ...)
M SRT’s, ...
R induced order: M-RR cooperative order: R-R
(Nd, Sm, Gd, Er, ...)
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NdNiONdNiO33 : Peculiar : Peculiar systemsystem
TN = TM-I = 200 K
Ni AF order(a very unusual one!)M-I transition &Orbital order
1000 K
100 K
10 K
1 K
TNd = 20 K Nd induced order(very unusual one, too!)
0.1 KT = 0.2 K Enhancement of the
diffracted neutron intensities(unclear origin)
for a review, see M. Medarde, J. Phys.:Condens Martter 9, 1679 (1997)J.L. García Muñoz et al., Phys. Rev. B 50, 978 (1994)
S. Rosenkranz, Ph.D. Thesis ETH Zürich, 11853 (1996)
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NdNiONdNiO33 : : crystal structurecrystal structure
•• Pbnm Pbnm orthorhombicorthorhombic perovskite
Ni
O
Nd
Each Nd ion is placed at theEach Nd ion is placed at thecenter of a Ni cubecenter of a Ni cube
Ni occupies Ni occupies abab planes : planes :A planesA planes
b
c
a
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Ni Ni magnetic order inmagnetic order in NdNiONdNiO33 : : ““Model 1Model 1””
Stacking of alternating ab layers A+ A- A- A+A+ A- A- A+ A+...
AntiferroAntiferroNi spinsNi spins
ddxx22-y-y22
ddzz22
b
b’a’
aA+A+
A+A+
A-A-
A-A-J.L. García Muñoz et al., Phys. Rev. B 50, 978 (1994)
J.L. García Muñoz et al., Phys. Rev. B 51, 15197 (1995)
TTN N = 200 K= 200 K
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Model 1 hypothesisModel 1 hypothesis
““Model 1Model 1””: Two kind of magnetic Nd ions: Two kind of magnetic Nd ions
--Nd BNd B++
Ni ANi A++
Nd BNd B00
Uncompensatedenvironment:
Strong polarization
Ni ANi A++
Ni ANi A--
Compensatedenvironment:
Zero polarization
J.L. García Muñoz et al., Phys. Rev. B 50, 978 (1994)J.L. García Muñoz et al., Phys. Rev. B 51, 15197 (1995)
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““Model 1Model 1””: Diffracted intensity: Diffracted intensityfrom polarized Ndfrom polarized Nd
Macroscopic Experimental test of Macroscopic Experimental test of ““Model 1Model 1””::
Low-temperature specific heat Low-temperature specific heat
However...However... Nd compensated environments :
non-zero Zeeman splittings
NdCrO3 : Δ = 27 K ;NdFeO3 : Δ = 5.7 KNdMnO3: Δ ~ 25 K
J.L. García Muñoz et al., Phys. Rev. B 50, 978 (1994)
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Low-temperature contributionLow-temperature contribution
Model 1
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0 1 2 3 4
Specific heat (R)
T (K)
NdNiO3
Schottky-like maximumSchottky-like maximumTTN2 = 0.77 K = 0.77 K
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0
1
2
3
4
5
-0.2 0 0.2 0.4 0.6
INS intensity (arb. units)
Ei (meV)
Two channels evidenced by HR-INS:Two channels evidenced by HR-INS:
ΔΔ00 = 4.1 K ; = 4.1 K ; ΔΔ±± = 5.2 K = 5.2 K
T = 2K
A microscopic probe:A microscopic probe:high resolution Inelastic Neutron Scatteringhigh resolution Inelastic Neutron Scattering
ΔΔ±±
ΔΔ±±
ΔΔ00
ΔΔ0 0 = 0= 0
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The Ni Nx magnetic modePOLARIZES
the Nd subsystem in a mode (let’s call it nx)
belonging to the same irep of the magnetic group than Nx
Nd-Nd cooperative orderwill favour another mode
(let’s call it r) belonging to another irep
b a
c
Quadruple Magnetic unit cell, TQuadruple Magnetic unit cell, TN N = 200 K= 200 K
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Mean field model: Mean field model: specific heatspecific heat
2 2 ˆH ˆ 2 ˆ 2 2
p2
cexcB !"#"µ!"#" $$$$$= xxxpc g nnrH
Self interaction terms Self interaction terms Ni-Nd Zeeman term (eff. exchange field)Ni-Nd Zeeman term (eff. exchange field) Nd-Nd exchange of the polarized component N Nd-Nd exchange in cooperative mode
ˆ 2
1- r=!
where...
ˆ 2
1- xn=!
are mean field order parameters for the cooperative and induced order modesand
c! p!and are the Nd-Nd exchange constants
in cooperative and polarized modes
Spin Hamiltonian for the Nd system:Spin Hamiltonian for the Nd system:
< > < >
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Free energy :Free energy :
If we impose:If we impose: 0
excexc HH >± , the free energy splits into two terms:, the free energy splits into two terms:
!"#
$%&
''(
)**+
, -.+= /
±= TT
2cosh2ln
2
1
2
1
á2
p2
c0,á
á 0121F
with
( ) ( )2pá2
cá
!"µ#" ++=$ excBx Hg
being the exchange splittings of the Nd3+ (±, 0) ground doublets.
áF !!By minimizingBy minimizing andand , we get the , we get the
characteristic equations of the system, which gives thecharacteristic equations of the system, which gives theordered net Néel moments ordered net Néel moments as a function of as a function of T.T.!! andand
with respect to with respect to
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Ecuaciones características :Ecuaciones características :
!!"
#$$%
& '
'=
T2 tanh
2
á
á
c())
!!"
#$$%
& '
'
+=
T
Hg excBx
2 tanh
2
á
á
pá ()µ
(
0 =!
!!"
#$$%
& '=
'
T2tanh
2
á
c
á
(
Fase ordenadaFase ordenadacooperativamentecooperativamente
FaseFaseparamagnética conparamagnética conorden inducidoorden inducido
Transición de FaseTransición de Fase0
0.2
0.4
0.6
0.8
1
0 1 2 3 4
!
T (K)
"
Mom
ento
net
o no
rmal
izad
o
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Entropy...Entropy...
!!"
#$$%
& ''()
*
+,-
.!!"
#$$%
& '+= /
±= TTTS
2 tanh
2
2 cosh ln 2ln
ááá
0,á
C (R
) and specific heat : and specific heat :
0
0.1
0.2
0.3
0 1 2 3 4
B+-
B0
T (K)
Δ0t = 2.6 K ≅ Δ0
e = 4.1 K
Δ±t = 5.3 K Ζ Δ±
e = 5.2 K
TNt = TNe = 0.77 K
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0
0.1
0.2
0.3
0.4
0.5
0.6
0
Cp
/ R
2 4 6 8 10
ra = 3
rb = 0
a
b
t
0
0.25
0.5
0.75
0 2 4 6 8
Cp
/ R
10
a
b
ra = 1.5
rb = 0
t
0
0.2
0.4
0.6
0.8
1
0
Cp
/ R
2 4 6 8 10
t
ra = 1
rb = 0
a
b
0
0.5
1
1.5
0 2 4 6 8
Cp
/ R
10
ra = 0.5
rb = 0
a
b
t
Results for HResults for H00excexc = 0 : = 0 :
HH±± = 0.5 = 0.5
HH00 = 0 = 0
HH±± = 1 = 1
HH00 = 0 = 0
HH±± = 1.5 = 1.5
HH00 = 0 = 0
H± = 3
H0 = 0C
(R)
C (R
)C
(R)
C (R
)
C (R
)C
(R)
C (R
)C
(R)
0.4
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0
ra = 2
rb = 1
a
0.1b
0.2
Cp
/ R
0.3
0 2 4
t
6 8 10
0
0.1
0.2
0.3
0.4
0.5
0
Cp
/ R
2 4 6 8 10
ra = r
a = 2
a = b
t
0
0.1
0.2
0.3
Cp
/ R
0 2 4 6 8 10
t
ra = 3
rb
= 1
ab
Results for HResults for H00excexc > 0 : > 0 :
HH±± = H = H00 = 2 = 2
HH±± = 3 = 3
HH00 = 1 = 1
HH±± = 2 = 2
HH00 = 1 = 1 Only intermediate (though different)Only intermediate (though different)
values for both, Hvalues for both, H±±excexc and H and H00
excexc
reproduce the experimental resultsreproduce the experimental resultsC
(R)
C (R
)
C (R
)C
(R)
C (R
)C
(R)
0.2
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CCpp best fit best fit
C (R
)
0
0.2
0.4
0.6
0.8
1
0 5 10 15 20
T (K)
!
!1!2
Nor
mal
ized
net
mom
ent
0
0.1
0.2
0.3
0 1 2 3 4
B+-
B0
T (K)
ΔΔ00tt = 3.6 K = 3.6 K
ΔΔ±±tt = 5.6 K = 5.6 K
TTNtNt = 0.81 K = 0.81 K
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