Scattering Neutron spin meets electron spin Magnetic neutron diffraction Inelastic magnetic neutron scattering Polarized neutron scattering Collin Broholm* Hopkins University and NIST Center for Neutron Rese *Supported by the NSF through DMR-9453362 and DMR-0074571
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Magnetic Neutron Scattering Neutron spin meets electron spin Magnetic neutron diffraction Inelastic magnetic neutron scattering Polarized neutron scattering.
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Magnetic Neutron Scattering
Neutron spin meets electron spin Magnetic neutron diffraction Inelastic magnetic neutron scattering Polarized neutron scattering Summary+Impurities in spin-1 chains
Collin Broholm*Johns Hopkins University and NIST Center for Neutron Research
*Supported by the NSF through DMR-9453362 and DMR-0074571
CRNL 6/20/00
Magnetic properties of the neutron
m
meBn
The neutron has a dipole moment
n is 960 times smaller than the electron moment
960913.1
1836
en
e
m
m
A dipole in a magnetic field has potential energy rBr V
Correspondingly the field exerts a torque and a force
B BF
driving the neutron parallel to high field regions
CRNL 6/20/00
The transition matrix element
The dipole moment of unfilled shells yield inhomog. B-field
2
ˆ
4 R
g B RSB 0
The magnetic neutron senses the field
220
ˆ
4 Rm
mgV B
em
RSrBr
The transition matrix element in Fermi’s golden rule llm iF
grV
mrSkk
exp
22 02
Magnetic scattering is as strong as nuclear scatteringcm 1054.0
412
20
0
em
er
It is sensitive to atomic dipole moment perp. to
lll SSS
CRNL 6/20/00
The magnetic scattering cross section
rrr dexp isF
Spin density spread out scattering decreases at high
The magnetic neutron scattering cross section
t
eedteFg
rk
k
EEVpm
k
k
ll
ll
itiW
m
ll
SS
kkEdd
d
RR
2
0
2
2
22
20
22
2
For unspecified incident & final neutron spin states
Edd
d
Edd
d 2
21
2
CRNL 6/20/00
Un-polarized magnetic scattering
llll
iti
W
teedt
eFg
rk
k
ll
SSrr 0
ˆˆ2Edd
d 22
20
2
llll
iti
W
teedt
eFg
rk
k
ll
SSrr 0
ˆˆ2Edd
d 22
20
2
Spin correlation functionSpin correlation function
Squared form factorSquared form factor Polarization factorPolarization factor
Fourier transformFourier transform
DW factorDW factor
CRNL 6/20/00
Magnetic neutron diffraction
Time independent spin correlations elastic scattering
llll
iW lleeFg
r
SSrrˆˆ
2d
d 22
20
Periodic magnetic structures Magnetic Bragg peaks
mm
mmv
Nr
22
32
0 ˆ2
d
dFF
The magnetic vector structure factor is
d
dd
2d
d S2
d
iW eeFg
F
Magnetic primitive unit cell greater than chemical P.U.C.
Magnetic Brillouin zone smaller than chemical B.Z.
CRNL 6/20/00
zS ˆB
smg
Simple cubic antiferromagnet
ab
*a*b
Real sp
ace
Reci
pro
cal S
pace
ma
mb
*ma
*mb
lkheFm W
B
s
sinsinsin82
ˆ 2
z
F
m
mzW
B
s
vFe
mrN
3222
2
0
21
2d
d ‘
No magnetic diffraction for S
SS
Not so simple Heli-magnet : MnO2
llll iS RQyRQxRwS sinˆcosˆexp
Insert into diffraction cross section to obtain
QwQ-w
d
d
vF
geSrN z
W3
22
220
21
2
111w and 7200Q characterize structure
*a
*c
a bc
CRNL 6/20/00
Understanding Inelastic Magnetic Scattering:
Isolate the “interesting part” of the cross section
,ˆˆ2
22
20
2 s
WeF
grN
k
k
Edd
d
The “scattering law” is defined as
tSSeedt llll
-iN
ti
0, ll rr1
S
for a wide class of systems It satisfies useful sum-rules
,exp,
SS
1,ddd
1
SS
Sq
q
''2 cos1
1
3
1),( llll
llllJN
d rrSS
S
Detailed balanceDetailed balance
Total moment
Total moment
First moment sum-ruleFirst moment sum-rule
CRNL 6/20/00
Scattering from a quantum spin liquid
Dimerized spin-1/2 system: copper nitrate
JTkB
CRNL 6/20/00
A spin-1/2 pair has a singlet - triplet gap:
Weak inter-dimer coupling cannot close gap
Bond alternation is relevant operator for quantum critical uniform spin chaininfinitesimal bond alternation yields gap
Inelastic scattering is not confined to disp. relations when• There is thermal ensemble of excitations present• and do not uniquely specify excited state
- electron hole pair excitations in metals - spinon excitations in quantum magnets
spinon continuum in spin-1/2 AFM chain
CRNL 6/20/00
and the magnetic susceptibility
Compare to the generalized susceptibility
0,2
llll
-itiB StSeedtN
g
ll rrq
They are related by the fluctuation dissipation theorem
eg B 1
1Im,q 2
qS
tSSeedt llll
-iN
ti
0, 1 ll rr
S
,S
We convert inelastic scattering data to• Compare with bulk susceptibility data• Isolate non-trivial temperature dependence• Compare with theories
q to
CRNL 6/20/00
Polarized magnetic neutron scattering
tll SS
0
Specify the incident and final neutron spin state
tSS zl
zl 0
tSS zl
zl 0
tSS ll
0
tSS ll
0
Non spin flip:SHS
Spin flip: SHS
CRNL 6/20/00
Polarized neutron scatteringH// H perp
Type of scattering SF NSF SF NSFNuclear coherent 0 1 0 1Nuclear isotope incoherent 0 1 0 1Nuclear spin incoherent 2/3 1/3 2/3 1/3Magnetic Sxx+Syy 0 Sxx Syy