Probing Relativity using Space-Based Experiments Fundamental Physics Research in Space International Workshop Washington DC 22-24 May 2006 Neil Russell Northern Michigan University, USA •The Standard-Model Extension (SME): a tool.

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Transcript Probing Relativity using Space-Based Experiments Fundamental Physics Research in Space International Workshop Washington DC 22-24 May 2006 Neil Russell Northern Michigan University, USA •The Standard-Model Extension (SME): a tool.

Probing Relativity using Space-Based Experiments
Fundamental Physics Research in Space
International Workshop
Washington DC
22-24 May 2006
Neil Russell
Northern Michigan
University, USA
•The Standard-Model Extension (SME):
a tool to search for signals
of quantum gravity at accessible energies
•Clock-Comparison Tests
•Optical and Microwave cavities
Studying Quantum Gravity at sub-Planck Energies
Energy
Quantum Gravity
EP
Standard Model
General Relativity
 Minkowski limit
Curvature / torsion
SM + GR  highly successful description of observed phenomena
These two field theories are expected to merge at the Planck scale 1019 GeV
Suppressed effects of the fundamental quantum-gravity theory may be
observable in sensitive experiments
Relativity violation is a possible Planck-scale signal
Any observable signals of Lorentz violation can be
described using effective field theory
Kostelecký, Potting
PRD 51 3923 (1995)
What should go into an effective QFT for Lorentz violation?
Standard Model with Gravity
Coordinate-independent
Lorentz violation
Standard-Model Extension
“SME”
SME contains
• Minimally-coupled SM action
• Pure-gravity action
• Leading-order terms for Lorentz violation constructed
from gravitational and SM fields
Minimal SME: SME operators restricted to mass dimension 3 and 4
Kostelecký, PRD 69 105009 (2004)
Colladay, Kostelecký, PRD 55 6760 (1997)
PRD 58 116002 (1998)
Special case: the Minimal SME
•
Neutral meson oscillations (*)
•
Neutrino oscillations
•
Clock-comparison tests – ground (*)
•
Clock-comparison tests -- space
•
Spin-polarized torsion pendulum (*)
•
Penning-trap tests of QED (*)
•
H (*) and anti H spectroscopy
•
Muon properties (*)
•
Cosmological birefringence (*)
•
Optical and microwave cavities (*)
•
Baryon asymmetry
•
Post-newtonian gravity
New Scientist 16 August, 2003
The minimal SME has been used as the
basis for a variety of investigations:
(*) : bounds already existing
There are now more than 500
papers on the SME
http://physics.indiana.edu/
~kostelec/faq.html
Sidereal variations
Kostelecký, PRL 80 1818 (1998)
Clock-comparison tests
Kostelecký, Lane,
PRD 60, 116010 (1999)
Bluhm, Kostelecký, Lane, Russell
PRL 88, 090801 (2002)
PRD 68, 125008 (2003)
Clock-comparison tests
frequency
Line from
atomic
transition
Stable clock
9.1 GHz
time
Lorentz-violation signal could occur as
minuscule variation in clock frequency
To detect signal, compare two clocks:
one sensitive,
one inert or differently affected
sensitive
inert
Clock-comparison tests
Accessing coefficients without suppression:
Need change in z component of angular momentum
Eg, for Hydrogen maser,
1,0  0,0
is suppressed,
making a good reference clock;
1,1  1,0
is sensitive at leading order,
making a good signal clock.
To search for Lorentz and CPT violation in SME context, perturbation is…
(Details of multiparticle aspects etc omitted)
Kostelecký, Lane, PRD 60, 116010 (1999)
Summary of SME bounds from Clock-comparison experiments
minus log (bound/GeV)
species
neutron
Hughes et al
PRL 1960
Drever
Phil Mag 1961
Prestage et al
PRL 1985
Be / H maser
proton
Comment
electron
27, 25
Lamoreaux et al PRL 1986
Hg / Hg
29, 27, 26
Chupp et al
PRL 1989
Ne / He
27
Berglund et al
PRL 1995
Hg / Cs
30, 28
Bear et al
PRL 2000
He / Xe maser
D. Phillips et al
PRD 2001
H / H maser
Cane et al
PRL 2004
He / Xe maser
Wolf et al
PRL 2006
Cs fountain
Analyzed in SME context
by Kostelecky and Lane,
PRD 1999
27, 25
27, 22
31
27
27
first boost bound
25, 22, 21
Possible advantages of space include:
•
greater boosts
•
greater fountain free-fall time
•
choice of orbital plane
c tilde parameter
Boosted clocks
Clock-comparison analyses considering rotational effects:
Kostelecký,Lane PRD 60 116010 (1999)
Can consider also boosted trajectories of clocks in space.
Bluhm, Kostelecký, Lane, Russell, PRL 2002 & PRD 2003
Issues:
1. A changing velocity is useful for improved sensitivity
 satellite in orbit is a good candidate
2. A standard inertial reference frame must be selected
Good candidates are centered on the Sun, the galaxy, and the CMB.
Earth-centered frame is not suitable.
 Choose Sun-centered frame, T starting at vernal equinox in 2000
Laboratory choices
Wanted: fast-moving, rotating laboratory
Speed
v/c
period
ground
0.4 km/s
(wrt Earth)
10-6
24 h
ISS
8 km/s
(wrt Earth)
10-5
92 min
Earth
30 km/s
(wrt Sun)
10-4
365 d
Sun
200 km/s
(wrt galaxy)
10-3
Dedicated
experiment
300 km/s
(wrt Sun)
10-3
~10
sec
SpaceTime?
Z
Satellite orbit
z
w sT s
Y
a
Equatorial plane
X
Spring
equinox
Bluhm, Kostelecký, Lane, Russell, PRL 88, 090801 (2002);
PRD 68, 125008 (2003)
Need the inertial-frame quantities in terms of the lab-frame quantities…
Bluhm, Kostelecký, Lane, Russell, PRL 88, 090801 (2002);
PRD 68, 125008 (2003)
General form of boost and rotation dependence for b3 tilde
bs = speed of satellite relative to the Earth = 8 km/s
b
= speed of Earth relative to the Sun = 10
4
c = 30 km/s
Without boosts, recover rotation dependence
equivalent to result in Lane, Kostelecky PRD 1999
Optical and Microwave cavities
Kostelecký and Mewes
PRL 87, 251304 (2001)
PRD 66, 056005 (2002)
Lorentz-violating photon sector (dimensionless)
Kostelecký and Mewes, PRL 87 251304 (2001);
PRD 66 056005 (2002)
1
Parity
even
3x3,
traceless,
symmetric
Parity
odd
5
5
5
3x3,
antisymmetric
3
Total coefficients: 19
These 19 coefficients describe
all dimensionless photon-sector
observer-independent Lorentz
violations
SME Birefringence Tests
The vacuum is found to be birefringent
10 relevant coefficients:
10 particular combinations:
Comparison of polarization for
different wavelengths
Analysis based on data for 16 sources
Kostelecký and Mewes,
PRL 87 251304 (2001);
PRD 66 056005 (2002)
Cavity Oscillators
Kostelecký and Mewes, PRL 87 251304 (2001);
PRD 66 056005 (2002)
Fractional frequency shifts for cavity
optical:
microwave, T010 cylindrical mode:
Nˆ
Tests with Optical and Microwave cavities
Each experiment bounds different SME coefficient combinations
Brillet,Hall (PRL 1979) Michelson-Morley type
1 combination of coeffs < 10-15
Hils,Hall (PRL 1990) Kennedy-Thorndike type
1 comb. of coeffs < 10-13
Lipa et al. (PRL 90 060403, 2003)
-9
4 combs. of coeffs <10-13 ; 5 comb. of coeffs <10
Müller, Herrmann, Braxmaier, Schiller, Peters, (PRL 91 020401, 2003)
-11
4 combs. of kappa coeffs <10-15 ; 5 comb. of kappa coeffs <10
Müller, Herrmann, Saenz, Peters, Lämmerzahl , (PRD 68 116006, 2003)
-12
2 combs. of electron coeffs <10-14 ;1 comb. of electron coeffs <10
Wolf, Tobar, et al, (GRG 36 2352, 2004); and (PRD 70 051902, 2004)
combs. of kappa coefficients <10-15
Müller, (PRD 71 045004, 2005)
kappa coeffs <10-15 ; electron coeffs <10
Stanwix, Tobar, Wolf et al (PRL 95 040404, 2005)
kappa e minus, ZZ component: 5.7 < 10-14 ; …
2.2 < 10-14 ; …
Antonini, Okhapin, Göklü , Schiller (PRA 72 66102, 2005)
5.2 < 10-15 ; …
Herrmann, Peters et al, (PRL 95 150401, 2005)
-16
Planned or proposed space tests include:
“SuperSUMO”
Lipa, Wang, Nissen, Kasevich, Mester : (see poster)
possible in principle to resolve c/c at 10–20
STEP orbiter platform (for example)
ACES
Cs Atomic clock (PHARAO) and space H maser (SHM)
see talk by C. Salomon
OPTIS
Optical cavities and atomic clocks
 photon and fermion sectors of SME
See talk by Laemmerzahl,
poster by H. Dittus
SpaceTime
 three ion clocks, trajectory close to Sun
 higher boost factor than Earth satellites
 see talk by Maleki
PARCS
 PARCS Primary atomic reference clock in space, on ISS
RACE
 Rubidium atomic clock experiment on ISS
SUMO
 Superconducting microwave oscillator on ISS
Gravitational tests : see talk by Kostelecky
Examples: ACES, PARCS, RACE:
Cesium and Rubidium
Transition changes the z component of angular momentum eg: 4,4  4,3
For sensitivity of 100 Hz, bounded terms include:
Proton and electron parameters:
~
GeV on bZ
~
-25
10
GeV on dZ
~ ~ ~ ~ ~
-23
10
GeV on bT, d±, dQ, dJK, HJT
10-27
Proton parameters:
10-25 GeV on c~Q from single and double frequencies
Hydrogen maser
Hyperfine transition: 1,1  1,0
Estimate, using 400 Hz variation limit:
Proton and electron parameters:
~
10-27 GeV on bZ
~ ~ ~ ~ ~
10-23 GeV on bT, d±, dQ, dJK, HJT
Summary
The Standard-Model Extension (SME)
• Allows study of all possible Lorentz violations
in context of Standard Model and General Relativity
• Limit of underlying Quantum-Gravity models
The SME predicts
• signals at the orbital and double-orbital frequencies
• signals at the frequency of the Earth’s orbital motion
Specific calculations for Cs 133, Rb 87, and H clocks are available and
include relativistic effects at first order in the boost
Estimates for attainable sensitivities for space have been obtained
10 of the 19 dimensionless photon coefficients are strongly constrained by
birefringence
The remaining ones have been vigorously pursued in cavity experiments;
space tests hold the potential for even higher resolutions