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Santa Fe Polarized Drell-Yan Physics Workshop October 31- November 1, 2010 Santa Fe, NM 87501, USA. AFP – a fast & easy nuclear polarization reversal ?. P. Hautle Paul Scherrer Institut CH-5232 Villigen PSI Switzerland. Outline. Introduction polarised targets = unique DNP systems. - PowerPoint PPT Presentation
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P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
AFP – a fast & easy AFP – a fast & easy nuclear polarization nuclear polarization
reversal ?reversal ?P. Hautle
Paul Scherrer InstitutCH-5232 Villigen PSI
Switzerland
Santa Fe Polarized Drell-Yan Physics WorkshopOctober 31- November 1, 2010
Santa Fe, NM 87501, USA
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
OutlineOutline
Introduction polarised targets = unique DNP systems
Overview of Experimental Data overview of experimental data
some details / comments
AFP Theory thermodynamic of a nuclear spin system
classical picture - rotating frame
quantum statistical description – spin temperature
which effects set limits on the optimum efficiency
Implementation technical and physics constraints
what can be expected
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
PSI East
PSI West
Aare
SLS
cw Proton accelerator (590 MeV, 2.2 mA)
(, , SR SINQ, UCN)
SwissFEL
Accelerator Facilities
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
100 cm100 cm33
„„Frozen Spin“ Frozen Spin“ Polarised Polarised
TargetTarget
Particle physics experimentson beams of pions, protons, neutrons…..
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
60 μm thick polystyrene foil cooled to 200 mK by a sub micron thick film of superfluid 4He
cell with two 500 nm thick Si3Ni4 windows
“Ultra-thin” polarised solid target
[J.P Urrego Blanco et al., NIM B 261 (2007) 1112]
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
suppress background suppress background scattering by TOFscattering by TOF
coincident coincident in situin situ detection of low detection of low energy recoil protons energy recoil protons in the target itselfin the target itself
polarisedpolarised nuclei in nuclei in the the scintillatingscintillating detector itselfdetector itself
O
N
HC
HC
n
CH3
O
CH3
CH3
CH3
N·B. van den Brandt B. van den Brandt et al.,et al., NIM A 446 (2000) 592 NIM A 446 (2000) 592
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
BeamBeamDetector
neutron beamneutron beam
Observe DNP build up with Observe DNP build up with
small angle neutron scatteringsmall angle neutron scatteringthrough spin contrast variation
Europhys. Lett. 59 (2002) 62 Eur. Phys. J. B 49 (2006) 157–165J. Appl. Cryst. 40 (2007) s106-s110
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
BB00=2.5T=2.5T
58
mm
58
mm
d-PS targetd-PS targetdoped with d-TEMPOdoped with d-TEMPO
Ø Ø 5 mm x 1.2 mm5 mm x 1.2 mm
66LiFLiF
targettargetholderholder
45 mm45 mm
Pseudomagnetic precession of cold Pseudomagnetic precession of cold neutronsneutrons
[F. M. Piegsa et al., NIM A 611 (2009) 231]
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Dissolution DNP for MRI / NMRDissolution DNP for MRI / NMR
Polarize organic samples labeled with 13C, 6Li, 15N nuclei in solid state (1 K / 5T)
Dissolve rapidly and inject into rat in imager (9.4 T) => image of brain metabolismimage of brain metabolism
Details and List of publications see: http//: sdnpi.epfl.ch
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Nuclear Spin Nuclear Spin ThermodynamicThermodynamic
ss
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Frequency [MHz]149.0 149.2 149.4 149.6 149.8 150.0
ii i
dH h
dt
equation of motion
H
ih
External field ( ~ T) including rf field (~ G)
“Local field” which spin i feels because of neighbours 3 5
3j iji j ij
j ij ij
rh r
r r
2 212L iH h (averaged over all orientations and spin states)
~ few GLH
Nuclear spin system (in a solid) in external Nuclear spin system (in a solid) in external fieldfield
ii
M
I H
FWHM (Gaussian)
2 523LH M
22 2ln 2 M
Magnetization
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Energy – Entropy – Isentropic coolingEnergy – Entropy – Isentropic cooling
0 / SM CH T
2 / 3C N kCurie Law
0ZE M H 1
2S i ii
E h
2 /S L SE CH T20 /Z SE CH T
Energy
Entropy 2 2/ 2 / 2S S S L SS E T CH T 2 20/ 2 / 2Z Z S SS E T CH T
Applied field Local field
2 2 212 0 /Z S L SS S C H H TS constantconstantIsentropic coolingIsentropic cooling
Adiabatic demagnetizationAdiabatic demagnetization
0 /M H kT
(spin energy / thermal energy)
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Isentropic cooling –Isentropic cooling –Adiabatic demagnetizationAdiabatic demagnetization
2 2 212 0 /Z S L SS S C H H TS constantconstant
HL
H0
precession about H0
HH00 is decreased is decreased
precession about HL
Important change when H0
HL :
Entropy transferred from polarizationpolarization to spin-spin orderingspin-spin ordering
Reversibility:Reversibility: change of H0 slow compared to equilibration time (HL)1
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Adiabatic fast Adiabatic fast passage (AFP)passage (AFP)
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
rf field - Rotating frame of referencerf field - Rotating frame of reference[F. Bloch, Phys Rev 70 (1946) 460]
[A. Abragam, Principles of Nuclear Magnetism, 1961]
rotating framerotating frame
0 1 1ˆ ˆcos( ) sin( )ˆH H z H t x H t y
External field H
contains rf fieldrf field
0 1 ˆ( ) ˆ re rH z HH x
1 1
0 0
tan( )
H
H
0 0H Larmor frequency:
0zH H 12 cos( )xH H tstatic field: rf field:
H1
He
H0 ω/γ
H0rz z
rx
M
M
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
rf field - Rotating frame of referencerf field - Rotating frame of reference[F. Bloch, Phys Rev 70 (1946) 460]
[A. Abragam, Principles of Nuclear Magnetism, 1961]
rotating framerotating frame
0 1 1ˆ ˆcos( ) sin( )ˆH H z H t x H t y
External field H
contains rf fieldrf field
0 1 ˆ( ) ˆ re rH z HH x
1 1
0 0
tan( )
H
H
0 0H Larmor frequency:
0zH H 12 cos( )xH H tstatic field: rf field:
H1
He
H0 ω/γ
H0rz z
rx
M
M
HHee can be rotated by 180° can be rotated by 180°
sweeping sweeping HH00 or or ω ω through through resonance resonance
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Adiabatic TheoremAdiabatic Theoremd
Hdt
equation of motion
For any vector satisfying a similar equation of motion the angle For any vector satisfying a similar equation of motion the angle between and remains constant provided the change of between and remains constant provided the change of direction of in time is sufficiently slowdirection of in time is sufficiently slow
H H
Possible to reverse the magnetization
What happens to the magnetization ? M
21
dHH
dtAdiabaticAdiabaticity: FastFaster than relaxation: 1
1H
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Adiabatic TheoremAdiabatic Theoremd
Hdt
equation of motion
For any vector satisfying a similar equation of motion the angle For any vector satisfying a similar equation of motion the angle between and remains constant provided the change of between and remains constant provided the change of direction of in time is sufficiently slowdirection of in time is sufficiently slow
H H
Possible to reverse the magnetization
2 2 212 /e LR SS C H H T constantconstant
What happens to the magnetization ? M
Thermodynmics in Thermodynmics in solidsolid sample sample
Adiabtic demagnetization in the rotating frame (ADRF) Isentropic passageIsentropic passage
Important change when He
HLR :
Entropy transferred from polarizationpolarization to spin-spin orderingspin-spin ordering
((Zeeman Zeeman toto dipolar ordering dipolar ordering))
21
dHH
dtAdiabaticAdiabaticity: FastFaster than relaxation: 1
1H
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Frequency [MHz]149.0 149.2 149.4 149.6 149.8 150.0
( )g
Estimate the losses -Estimate the losses -AFP in the spin temperature modelAFP in the spin temperature model
[M. Goldman et al., Phys Rev 168 (1968) 301]
1 LH H
( ) 1g d
Provotorov equations describe mixing between Zeeman and spin-spin subsystem:
0H
Conditions:
High temperatures
Low nuclear polarizations
2 21( ) ( )W H g Mixing rate:Mixing rate:
AFPAFP:: variation of very small during time T2 D
12
W T
2 2
/ ( )
/ ( / )( )
d dt W
d dt W D
Evolution of inverse spin temperatures and to common value
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Frequency [MHz]149.0 149.2 149.4 149.6 149.8 150.0
( )g
Sweep of field / frequency through the Sweep of field / frequency through the resonanceresonance
121expfinal
initial
PP H dH dt
P
Fast sweepFast sweep – in time much shortershorter than mixing time W1
21
3exp
4 LR
P H dH dtH
1
exp L
D
R
T
HP
dH dt
Slightly saturating passageSlightly saturating passage H1
Quasiadiabatic fast passageQuasiadiabatic fast passage – in time much longerlonger than mixing time W1
Quasiadiabatic partQuasiadiabatic part
RelaxationRelaxation
Sudden to adiabatic transitionSudden to adiabatic transition~ 5 – 8 % loss, almost independant of 21H dH dt
1DT Spin-lattice relaxation of the spin-spin (dipolar) interactions
2 21( ) ( )W H g
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
A = H12/(dH/dt)
1 10 100
Effi
cien
cy
P [P
F/P
I]
-1.0
-0.8
-0.6
-0.4
-0.2
0.0
H1 = 0.25 G
quasiadiabtic relaxation
= 10 kHz, T1D = 1 s = 25 kHz, T1D = 1 s
= 50 kHz, T1D = 1 s
= 50 kHz, T1D = 10 s
21 1
1 1 2 2LR
DLR
HT T
H
Spin-lattice relaxation in the rotating frame
Theoretical predictionTheoretical prediction
Sample temperature & dopant concentration !!
narrow line widthnarrow line width long relaxation time in RF long relaxation time in RF
= Spin-lattice relaxation of the spin-spin system
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
A = H12/(dH/dt)
0.01 0.1 1 10 100 1000
Effi
cien
cy
P [P
F/P
I]
-1.0
-0.5
0.0
0.5
1.0
n-butanol + 4 x 1019 e /cm3
porphyrexideT = 0.5 K / B = 2.5 T
EHBA(CrV)T ~ 80 mK / B = 2.5 T
Experimental results I - ProtonsExperimental results I - Protons
effect of sample temperatureeffect of sample temperature
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
A = H12/(dH/dt)
0.01 0.1 1 10 100 1000
Effi
cien
cy
P [P
F/P
I]
-1.0
-0.5
0.0
0.5
1.0
7LiH irradiated
T ~ 80 mK / B = 2.5 T
Experimental results II – Experimental results II – 77LiHLiH
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Experimental results IIIExperimental results III
substance nucleu
sdopant
e- conc.[spins/g]
T[K]
P max
1-butanol 1H porphyrexide 4.0 x 1019 0.5 0.36
1-butanol 1H CrV EHBA 4.0 x 1019 0.08 0.76
7LiH7Li
irrad low ? 0.08 0.88
1H 0.92
8-fluoro-pentanol
19FTEMPO 2.0 x 1020 0.08
0.37
1H 0.40
d-butanol
2H
CrV EDBA 6.35 x 1019
1 0.75
2H 0.5 0.85
2H 0.08 0.90
d-butanol 2H CrV EDBA 2.36 x 1019 0.08 0.92
Deuterated alcohols are a different storyDeuterated alcohols are a different story::
large quadrupolar coupling
small dipolar coupling
1 and ½ sweep to reverse the polarization of the spin 1 system
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Experiment & TheoryExperiment & Theory
Data fitted with spin temperature model
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
e concentration [x 10 19]
2 3 4 5 6 7
Effi
cien
cy
P [P
F/P
I]
-0.96
-0.92
-0.88
-0.84
-0.80
-0.76
-0.72
Col 1 vs Col 2 Col 1 vs Col 3 Col 1 vs Col 4 Col 1 vs Col 5 Col 1 vs Col 6
T = 0.08 K
T = 0.5 K
T = 1 K
Sample temparature / dopant concentrationSample temparature / dopant concentration
d-butanol + EHBA(CrV)-d22
increase sweep rate for higher temperaturesincrease sweep rate for higher temperatures
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
1
6ln 2LRH
22 2( ) (0) 1M P M P
Line width / PolarizationLine width / Polarization
Frequency [MHz]149.0 149.2 149.4 149.6 149.8 150.0
FWHM (Gaussian)
22 2ln 2 M
50 kHz HLR = 2.9 G
Proton AFP efficiency vs line widthT ~ 80 mK and B = 2.5 T
FWHM NMR line width [kHz]
44 46 48 50 52 54 56 58
AF
P e
ffici
en
cy
P
-0.94
-0.92
-0.90
-0.88
-0.86
-0.84
-0.82
positive polarizationnegative polarization
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
7Li AFP efficiency vs polarizationT ~ 80 mK and B = 2.5 T
7Li nuclear polarization [%]
10 20 30 40 50
AF
P e
ffici
ency
P
-0.90
-0.88
-0.86
-0.84
-0.82
-0.80
-0.78
1
6ln 2LRH
22 2( ) (0) 1M P M P
Line width / PolarizationLine width / Polarization
Frequency [MHz]149.0 149.2 149.4 149.6 149.8 150.0
FWHM (Gaussian)
22 2ln 2 M
50 kHz HLR = 2.9 G
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Two nuclear spin speciesTwo nuclear spin species
Time [sec]0 200 400 600 800 1000
Deu
tero
n po
lariz
atio
n [a
.u.]
0.75
0.80
0.85
0.90
0.95
1.00
1.05
1.10
without proton AFP
with proton AFP (P ~ 0.5)
99.4 % deuterated without proton AFP(6.35 x 1019spins/g)
98 % deuterated (4 x 1019spins/g)
Coupling of the nuclear spin systems through electron non-Zeeman system
start microwaves
[Cox, Bouffard, Goldman, J Phys C 6 (1973) L100]
polarization of both nuclear spin systems should be reversedpolarization of both nuclear spin systems should be reversed
heat capacity !heat capacity !
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
In practice: polarization reversal AFP vs DNPIn practice: polarization reversal AFP vs DNP
T =80 mK / B = 2.5 T
gain can be dramatic in certain cases gain can be dramatic in certain cases (especially at low temperatures)(especially at low temperatures)
DNP reversalDNP reversal
AFP reversalAFP reversal
AFP efficiency <-> DNP build up timeAFP efficiency <-> DNP build up time
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
radiation damping
asymmetry of efficiency
superradiance
e.g. typical AFP parameters for protons:
Technical aspects ITechnical aspects I
requirementsrequirements
challangeschallanges
solutionssolutions tune and match the rf coil ?
B1 = 0.3 G perpendicular to static field B0
homogeneity B1/B1 ~ 0.5
dB/dt = 10 – 20 G/s or 40 – 80 kHz/s
frequency sweep width = 400 kHz – 1 MHz
produce the required B1 amplitude
do not excessively heat the sample
potential pitfalls
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Technical aspects IITechnical aspects II
radiation damping -> superradianceradiation damping -> superradiance
2R T
12 / ZQM H
threshold
210
0.1
electromagnetic energy provided by the spins compensates losses in the circuit
auto-oscillationauto-oscillation
12 ZM NP
Two coupled systems: resonance circuit < - > rotating magnetization
102
R Q M damping time constant [S. Bloom, J Appl Phys 28 (1957) 800]
[M. Odehnal, V. Petricek, Physica 67 (1973) 377]
[Yu. F. Kiselev et al., JETP 67 (1988) 413]
AFP gets asymmetric
superradiance
superradiant polarization reversalsuperradiant polarization reversal
[L.A. Reichertz et al., NIM A 340 (1994) 278] (NH3, V = 6.5 cm3 ; Q = 33)
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
Technical aspects IIITechnical aspects III
Example Example design of a rf irradiation system
5 T / 1 K system (S. Pentilla) magnetic to be rotated to have vertical field
sample sizesample size
polarized target systempolarized target system
samplesample
cylinder of 8 cm length/ 1.5 cm diameter
ammonia / 6LiD
reversalreversal every 2 h
rf rf structurestructure (coil) B1 ~ 0.3 – 0.5 G @ 212 MHz
01 2 2
1
2
nB
a g
1 ~ 0.12B n G/A
212 cP I R
large sample tuning not possible (superradiance)
solenoid
match to 50 Ohm
rf power ~ 10 W or more -> heat load !!
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
AFP used by the Standford group
1 180 B
AFP <-> 180° pulse (pulsed NMR)AFP <-> 180° pulse (pulsed NMR)
Frequency [MHz]149.0 149.2 149.4 149.6 149.8 150.0
50 kHz need to excite ~ 100 kHz
apply strong pulse: H1 > HL
1 1 2 100 B kHz
5 s
B1 11.7 G
[F. Bloch, W.W. Hansen, M Packard, Phys Rev 70 (1946) 474]
superradiance !!
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010
ConclusionConclusion
low temperature, T 1 K
low concentration of paramagnetic centers
experimental conditions
sample properties
one „free“ parameter : relaxation time in the rotating frame
local field HL
line width
(dipolar relaxation time T1D )
dipolar relaxation time T1D
““Strategy“ to get a high AFP efficiency ??Strategy“ to get a high AFP efficiency ??
What can be expected (conservative guess)What can be expected (conservative guess)
6LiD 5 T / 1K P > 0.5 2.5 T / 80 mKP ~ 0.9
Ammonia 5 T / 1K P < 0.5 2.5 T / 80 mKP ~ 0.7
Trade off between AFP efficiency and DNP build up time
P. Hautle, Santa Fe Polarized Drell-Yan Physics Workshop, Nov 2010