Tests of Lorentz Invariance with alkali- metal– noble-gas co-magnetometer (+ other application)
Michael Romalis Princeton University
Tests of Lorentz Invariance with alkali- metal noble-gas - - PowerPoint PPT Presentation
Tests of Lorentz Invariance with alkali- metal noble-gas co-magnetometer (+ other application) Michael Romalis Princeton University Tests of Fundamental Symmetries Parity violation weak interactions CP violation Three
Michael Romalis Princeton University
Tests of Fundamental Symmetries
Lorentz and CPT symmetry
⇒For example, Plank mass introduces an energy scale, so a particle given a Lorentz boost to p ~ Mpl should experience different physics due to quantum gravity effects. Symmetry violations found before corresponding particles were produced directly
⇒ Motivations for possible violation ⇒ Experimental signatures
⇒ Elimination of alkali-metal spin-exchange broadening ⇒ Alkali-metal noble gas co-magnetometer ⇒ Limits on Lorentz-violating spin coupling
⇒ Sensitive magnetometer for detection of brain fields ⇒ Nuclear spin gyroscope
Parametrizing Lorentz and CPT Violation
⇒ spontaneous symmetry breaking: vector fields with VEV ⇒ Modified dispersion relationships: E2 = m2 + p2 + η p3/MPl ⇒ Non-commutative space time [xµ,xν] = θµν
a,b - CPT-odd, dimension of energy c,d - CPT-even, dimensionless
Kostelecky et al.
D = 3
L = – ψ (m + aµγ µ + bµγ5γ µ)ψ + i
2 ψ (γν + c
µν γ µ + dµν γ5 γ µ)∂νψ
D = 4 + higher dimension operators
Jacobson, Amelino-Camelia Myers, Pospelov, Sudarsky Witten, Schwartz, Pospelov
Experimental Signatures
directional dependence of the speed of light
L = – bµψγ5γ µψ = – b ·S
S B⋅ − = = m ge A e 2 ψ γ ψ
µ µ
L
c.f.
i L = 2 ψ c
µν γ µ ∂ ν
ψ
(cπ-c)/c ~ c00
In general, spin coupling seems to be the most robust effect in most models.
Spin coupling experiments
and avoid cancellation by magnetic shields
could be the direction of motion relative to CMB
bµ hν1= 2µ1 B + 2β1 (b·nB) hν2= 2µ2 B + 2β2 (b·nB) ) ( 2
2 2 1 1 2 2 1 1 B
h n b⋅ µ β − µ β = µ ν − µ ν
B µ ω
T2 1/(πT2)
FFT
Quantum noise limit for N atoms:
Choice of Active Species:
Alkali metal atoms: Na, K, Rb, Cs
Collisions between alkali atoms, with buffer gas and cell walls
⇒ Increasing density of atoms decreases spin relaxation time ⇒ Under ideal conditions:
T 2
–1 = σse v n
σ se = 2 × 10–14cm2
δB ¥ 1fT
cm3 Hz T2N = σsevV
Mechanisms of spin relaxation
Why do spin-exchange collisions cause relaxation?
SF=1 B SF=2 ω ω SE
ω = ± gµB B h(2I + 1)
F=I±½
∆ω ≈ 1/ΤSE
S ω
F=2 F=1 mF = −2 −1 0 1 2
Ground state Zeeman and hyperfine levels
Zeeman transitions +ω Zeeman transitions −ω
SE
Eliminating spin-exchange relaxation
ω << 1/ΤSE
Atoms undergo spin-exchange collisions faster than the two hyperfine states can precess apart
B SF=2 SF=1 ω1
ω1 = 3(2 I + 1) 3 + 4 I (I + 1) ω = 2 3 ω
S ω
Complete elimination of spin-exchange broadening
destruction collisions
⇒ Convert spin angular momentum to rotational momentum of atoms
S
B
Chopped pump beam
10 20 30 40 50 Chopper Frequency (Hz)
0.0 0.1 0.2 Lock-in Signal (V rms ) − in phase − out of phase
Spin-exchange width: 3 kHz Observed width: 1 Hz
50 100 150 200 250 Chopper Frequency (Hz) 1 2 3 4 5 6 Resonance half-width (Hz)
Turning spin-exchange broadening back on
Magnetometer Schematic
Pump Laser Probe Laser
Alkali metal cell Polarizer Photodetector
Magnetometer Performance
Magnetic shield noise 7 fT/Hz1/2 Gradiometer Sensitivity 0.5 fT/Hz1/2 Volume : 0.3 cm3 Baseline: 3 mm Best SQUID
Previously best atomic magnetometer : ~1.8 fT/Hz1/2 with a volume 1800 cm3
3He Co-magnetometer
⇒T1 ~ 300 hours
5 10 15 20 25 30 35 Time (days) 20 40 60 80 100 NMR Signal (mV)
3He Co-magnetometer
collisions with alkali metal
K atoms
⇒K magnetometer operates near zero field
3He cancel
⇒3He spins experience a uniform field Bz ⇒Suppress relaxation due to field gradients
BK = 8π 3 κ 0MHe
m m m m B
T1
– 1 = D
∇Bx
2 + ∇B y 2
Bz
2
Magnetic field self-compensation
Magnetic field compensation
Slightly uncompensated Compensated
Frequency Response
T.W. Kornack and MVR, PRL 89, 253002 (2002)
Cancellation of magnetic field effects
Noise Compensation Gradient Compensation
Thermal Shields Magnetic shields with insulation Pump Laser Box Probe Laser Box Table Position Sensors
Development Run Data
S = Ax sin(Ωt)+Ay cos(Ωt) Ω - sidereal Earth rotation rate Ax = −0.76 ± 0.74 fT Ay = 0.59 ± 0.81 fT
Periodic zeroing of fields
Limits on Lorentz and CPT violating spin coupling
|bn| < 1.4 ×10−31 GeV |be| < 1.0 ×10−28 GeV
Limits from development run
|bn| < 1.1 ×10−31 GeV |be| < 0.3 ×10−28 GeV
Existing best limit
3He-129Xe co-magnetometer
Walsworth, Harvard-Smithonian Magnetic torsion pendulum Heckel, Adelberger, U of Washington
Natural size for Lorentz violation ?
pl
M m b
2
~ η
m - light mass scale: fermion mass SUSY breaking scale Pospelov, hep-ph/0505029
Existing limits: η ~ 10−9 − 10−12 1/Mpl effects are already highly excluded
What’s next?
⇒Further work on drift reduction and continuous data taking ⇒Constructing a miniature (30 cm size) system that can be placed on a rotating table to increase modulation frequency
1 day
Other applications of co-magnetometer
⇒ EDM violates CP symmetry, but very suppressed in the SM ⇒ Large EDMs generated in SUSY, other extensions
⇒Sensitivity 1 fT/Hz1/2 ⇒E = 10kV/cm, t = 107 sec
) sin( 24 ~
SUSY SUSY
2
φ π α M m e d
da ∝ deα2Z 3
δde= 10−29 e-cm, δdXe= 10−30 e-cm
Factor of 100 improvement in both limits
Cs-129Xe cell
Atomic Magnetoencephalography Setup
Atomic Gyroscope
Ω − =
Ω
1
n e z
R P S γ γ
For 3He 0.001 deg/hour1/2 ⇒ 1 fT/Hz1/2 For 21Ne 0.001 deg/hour1/2 ⇒ 10 fT/Hz1/2
Rotation signal
Conclusions
ways to experimentally probe Quantum Gravity
sensitive tests of Lorentz violation and other precision measurements.
Support: NIST, NASA, NSF, NIH, Packard
Foundation, Princeton University
Igor Savukov Igor Savukov Tom Kornack Tom Kornack Rajat Ghosh Rajat Ghosh Micah Ledbetter Micah Ledbetter Scott Seltzer Scott Seltzer Hui Xia Hui Xia Dan Hoffman Dan Hoffman Georgios Vasilakis Georgios Vasilakis Parker Meares Parker Meares
⇒Tom Kornack ⇒Iannis Kominis ⇒Scott Seltzer ⇒Igor Savukov ⇒Georgios Vasilakis ⇒Andrei Baranga ⇒Rajat Ghosh ⇒Hui Xia ⇒Dan Hoffman ⇒Joel Allred ⇒Robert Lyman