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Electric dipole moment searches
E.A. Hinds
Birmingham 11th July 2011
Centre for Cold MatterImperial College London
YbF
atom/moleculelevel
EDM: from particles to atoms and molecules
nuclearlevel
NNNN Schiffmoment
mercury
HiggsSUSY
Left/Right
StrongCP
field theoryCP model
qGG
neutron
nucleonlevel
electron/quark level
de
dq
dcq
~
P. HarrisIoP 2011
Measurement principle
B E
mB
Measure Larmor spin precession freq in parallel & antiparallel B and E fields
d makes precessionfaster...
Reverse E relative to B, look for freq shift.... or slower.
Pulsed YbF beam
PumpA-X Q(0) F=1
ProbeA-X Q(0) F=0
PMT
3K beam
F=1
F=0
rf pulse
B HV+
HV-
eEDM in practice (Imperial)Ch 15 Cold Molecules, eds. Krems, Stwalley and Friedrich, (CRC Press 2009)
P. HarrisIoP 2011
nEDM in practice
N S
Magnetic shielding
Storage cell
Magnet & polarizing foil Ultracold
neutrons(UCN)
UCN detector
Approx scale 1 m
Magnetic field coil
B
High voltage lead
E
/analysingfoil
Status of eEDM and nEDM
de = (-2.4 5.7 1.5) ×10-28 e.cm
68% statisticalsystematic - limited by statistical noise
• New eEDM result – YbF – Hudson et al. (Nature 2011)
• Previous eEDM result - Tl atoms de < 2.0 × 10-27 e.cm with 90% confidence
Regan et al. (PRL 2002)Nataraj et al. (PRL 2011)
de < 1 × 10-27 e.cm with 90% confidence dn < 3 × 10-26 e.cm with 90% confidence
Current upper limits
Left -Right MSSM
f ~ a/p
Multi Higgs
MSSM f ~ 1
10-24
10-22
10-26
10-28
10-30
10-32
10-34
10-36
eEDM (e.cm)
Imperial eEDM starting to explore
this region
Standard Model
de < 1.0 x 10-27 e.cm
Imperial eEDM (2011)Excluded region
e.g. Pospelov and RitzarXiv:hep-ph/0504231(2005)
P. HarrisIoP 2011
Constraints on SUSY parameters
Pospelov & Ritz, hep-ph/0504231
MSUSY = 500 GeVtan b = 3
e
P. HarrisIoP 2011
SUSY again Lebedev et al., hep-ph/0402023
n
Tl YbF (2011)n (2006)
Where do we go from here?nEDM Better polarisation
Higher E field Longer spin coherence time More neutrons
10 x betterCryoEDM
eEDM Better field control Longer spin coherence time More YbF molecules
10 x betterCryoYbF
Cryogenic YbF experiment (Imperial)
YbF beam
YAGablationlaser3K He gas cell
Yb+AlF3target
New J. Phys. 11 123026 (2009) Physical Review A (2011)S. M. Skoff et al.
Uses new molecular beam source
eEDM prospects with new source15 more molecules
3 longer interaction time
=> access to few x 10-29 e.cm range
=> 10 better signal:noise ratiowill improve systematics as well as statistics
+-+-
+-
+-
+-
garnet
E+-
squid magnetometer
GGG (LANL), GIG (Amherst)Gadolinium Garnets
Huge number of electrons
Other electron EDM searches+-
+-
+-
+-
+- E+-
Cs atomsFountain (LBL), Trapped (Penn State), Trapped (Texas) Long coherence time
Molecules Large effective E field
PbF beam (Oklahoma) similar to YbFMetastable ThO beam (Yale/Harvard) similar to YbF
Trapped HfF+ ions (JILA) 1 molecule; very long coh.time
none competitive with YbF in the immediate future
P. HarrisIoP 2011
Cryogenic nEDM experiment
• Neutrons produced, transported, & stored. Need lower losses.
• 10 kV/cm applied; aiming for 20-30 kV/cm
• Polarisation observed, but must improve
• Detector efficiency set to improve significantly
• Magnetic field stability to be improved by factor 1000
Sussex, RAL, Oxford, ILL,Kure
P. HarrisIoP 2011
Other nEDM experiments PSI (50 people) aim 5 10-27 by 2015 ORNL (90 people) construction 2017;
aims eventually for 5 10-28
e.cm
ILL: Russian group. Reinstating system from 1990 measurement. Perhaps 1 10-26 e.cm eventually.
FRM, Munich: hoping to install UCN source. Nothing firm yet
Masuda, Japan: observed resonance, but very low stats. Move to TRIUMF?
P. HarrisIoP 2011
... and other particles Muon EDM: from g-2
(7E-19 e.cm; proposed upgrades could reach ~10-24 e.cm by ~2020)
Deuterium EDM: similarprinciple (claimed potential reach ~10-29 e.cm)
Tau weak dipole moment – look for CP-odd observables in diff. x-sec at Z res.(6E-18 e.cm from LEP data)Sensitivity to physics BSM depends on source of CPv
Conclusions
These place strong constraints onCP-violation beyond std model
de < 1 × 10-27
e.cm dn < 3 × 10-26
e.cm
Current upper limits
UK leads the world in both
Will continue to do so if projects funded.