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Improved Tests of the Equivalence Principle
...Using TorsionBalances
Frank Fleischer,University of Washington
11 May 2011
The Equivalence Principle (EP)
Fundamental assumption of general relativity
locally a homogenous gravitational field looks the same as a uniform acceleration of the frame
usually tested via the universality of free fall (UFF)
Motivation: Why Test It?
Test the foundation of general relativity
More interesting: assume that classical gravity obeys the EP, then
use EP tests as extremely sensitive probes for new scalar or vector interactions!
Many ideas for physics beyond the standard model introduce such interactions.
Torsion balance experiments provide stringent limits on such models!
New Forces?
Examples for possible couplings: to baryon number B, B – L (L being the lepton number) ...
parameterization:
with a hypothetical ”charge”
B - L is especially interesting – conserved in GUTs
Testing the EP with Torsion Balances
To test the equivalence principle with a torsion balance, a couple things are needed:
a torsion balance with a composition dipole an attractor producing a force with a horizontal
component modulation of the signal
Eötvös parameter
Possible Attractors
nearby attractor
earth
sun
center of galaxy
need to providerotation
use theearth'srotation
Also important: these attractors differ in composition!
Using the Earth as a Source Mass
If the EP is violated, ”down” is not a unique direction
➔ depends on the ratio of gravitational and inertial mass!
Using the Earth as Source Mass
fiber Simplified model of a
pendulum for EP tests
➔ Balance twists if the two force vectors are not parallel, i.e. if EP is violated or gravitational field is not uniform.
Choice of Test Body Materials
Obvious constraints: solid, non-magnetic
For complete coverage of the parameter space, more than one test-body pair / attractor combination is necessary.
Large differences in number of neutrons and nuclear binding energy give greater sensitivity.
x10-2 Be PE Al Ti Cu Pt
Be -12.65 -3.80 -1.58 -1.25 4.40
PE -12.63 8.85 11.07 11.40 17.05
Al -3.59 9.03 2.22 2.54 8.20
Ti -1.33 11.29 2.26 0.32 5.98
Cu -1.01 11.62 2.59 0.33 5.65
Pt 4.55 17.18 8.15 5.89 5.56
Early Torsion Balance Experiments
Loránd Eötvös (1922):
various test-body pairs in the field of the earth
e.g. Roll, Krotkov, Dicke (1964):
sun as attractor, feedback
Braginsky, Panov (1972):
sun as attractor, no feedback
Reminder:
State of the Art
Our group at UW started looking for EP violations after a reanalysis of the Eötvös data by Fischbach et al., claiming evidence of a ”fifth force” with finite range.
Most recent published experiment*:
rotating torsion balance employing different source masses
local topography earth sun galaxy
sensitive to forces with λ from ~1m upward * Schlamminger et al. 2009
State of the Art
5 cm
70g pendulum,suspended by a 20μm thick, 1.08 m long tungsten fiber
Screws to reduce residual coupling to gravitational gradients
Eight test bodies(4 Be & 4 Ti) or (4 Be & 4 Al)4.84g each
Design minimizes coupling to gravitational gradients:4-fold azimuthal symmetry and top-bottom reflection symmetry
State of the Art
High precision turn table for continuous smooth rotation.
State of the Art
Reminder:
EotWash group (2009):
Next Generation EP Tests
Two possibilities to push the limits of torsion balance experiments for EP tests:
Increase the signal by using more sensitive test body material pairs
Reduce the noise floor
Combine both? Would be ideal, of course - but difficult.
Increasing the Sensitivity
Significant gain in sensitivity possible with a ”hydrogen-rich” test body
Promising material: UHMWPE – Ultra-High Molecular Weight PolyEthylene
x10-2 Be PE Al Ti Cu Pt
Be -12.65 -3.80 -1.58 -1.25 4.40
PE -12.63 8.85 11.07 11.40 17.05
Al -3.59 9.03 2.22 2.54 8.20
Ti -1.33 11.29 2.26 0.32 5.98
Cu -1.01 11.62 2.59 0.33 5.65
Pt 4.55 17.18 8.15 5.89 5.56
Increasing the Sensitivity
Significant gain in sensitivity possible with a ”hydrogen-rich” test body
Promising material: UHMWPE – Ultra-High Molecular Weight PolyEthylene
Problems / challenges:
Precision in machining Low density (0.94 g/cm3) Large thermal expansion coefficient Dimensional stability when ”baking”? Gold coating?
Increasing the Sensitivity
Will Terrano designed and built a test pendulum to learn about the specific problems of this choice of material:
”test bodies” mounted near their center of mass to avoid big moment changes by thermal expansion
completely encapsulated in aluminum
First test planned: investigate the dimensional stability – determine moments, bake out and check for changes.
Reducing the Noise
An inherent limitation for torsion balance experiments is thermal noise
Cooling helps in two respects:
lower temperature T Higher values of Q possible at low temperatures:
values of order 105 reported with metal fibers at 4.2K
Reducing the Noise
An inherent limitation for torsion balance experiments is thermal noise
Cooling helps in two respects:
lower temperature T Higher values of Q possible at low temperatures:
values of order 105 reported with metal fibers at 4.2K
Build a cryogenic torsion balance toinvestigate operation at low temperature!
cooling to 4K: factor ~60
factor ~100
A Cryogenic Torsion Balance
Use a pulse tube cooler for cooling to cryogenic temperatures
Problem: vibrations!
Isolate the cold head vibrationally from the cryostat:
Separate wall mount Only flexible connections
(edge-welded bellows, flexible copper heat links)
Air springs for vibrational isolation
cold head
fiber
magneticdamper
aut
oco
llim
ato
rla
ser
bea
m
thermalshields
flexibleheatlinks
pump portsuperinsulation
Some Pictures...
cold headsupport
openedcryostat(without thermalshields)
Current Status – Cooling
By now, several thermal cycles.
Min. temperature: ~5.5K
Cool-down time: ~2 days
Warming up takes a similar amount of time.
Even slightly exceeds design values!
Current Status – Noise
Designed and built test pendulums to explore the noise spectrum.
small gravitational multipole moments mass similar to our latest EP test
pendulum explore cryo-compatible design – lots of
engineering challenges
Current Status – Noise
Current noise level slightly above thermal noise.
Excess noise due to magnetic effects?
At current level at least, no extra noise from cold head visible!
RT thermalnoise for Q=3000
6K thermalnoise for Q=200000
What About Q?
Even if without having reached thermal noise yet, it is possible to check the quality factor Q.
A lot of the improvement in thermal noise level is expected to come from a better Q!
➔ Measure Q at room temperature and when cold.
Much of the expectedimprovement comes from Q
Measuring Q
At room temperature:
Q as expected, ~3000
Still the same at 5K!
Possible limiting factor: eddy current damping?
Applying an additional magnetic field (a few times the earth's field):
Q ~ 1100
t [s]
angl
e [m
rad]
Need magnetic shielding!
Record free oscillation, fit exp. decaying sine wave:
Next Steps
Magnetic shield has just been completed and installed.
Should hopefully open the way to higher Q and bring down the noise.
With substantially improved noise, will need to develop more sensitive optical readout.
Physics with ColdWash
Current setup has potential for an order of magnitude improvement in limits on long-range EP violations.
Design a EP test pendulum for operation at low temperature.
Implement a tilt monitoring (and, if necessary stabilization) system – very important systematic!
More magnetic shielding?
Study other possible systematics.
Physics with the current setup:
Summary and outlook
Significant (order of magnitude) improvements over our current limits are possible.
We are following a two-fold approach to achieve higher sensitivity to EP violating forces:
increase signal (choice of test body materials) reduce noise (operation at low temperature)
Both paths are being pursued – hydrogen-rich test bodies and a cryogenic torsion balance under development.