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1 Testing the Equivalence Principle in space with MICROSCOPE Joel Bergé (ONERA) On behalf of Pierre Touboul and the Microscope team Joel Bergé, LISA symposium, 05/22/2014 Tuesday, June 17, 14

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1

Testing the Equivalence Principle in space with

MICROSCOPEJoel Bergé (ONERA)

On behalf of Pierre Touboul and the Microscope team

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Weak Equivalence Principle

2

All test bodies follow the same universal trajectory in a gravitational field, independently of their mass, detailed internal structure and composition.

a.k.a the universality of free fall; Galileo

For all test bodies, the inertial mass and the gravitational mass are equal: mi = mg

Precision measured in terms of the Eötvös ratio

F = mi aFg = mg g

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Einstein Equivalence Principle

The structure of 20th century physics

3

Weak Equivalence Principle

Local Lorentz Invariance

Local Position Invariance

General RelativityGravity = metric

Einstein equations

Equations of motion for matterMaxwell equations

Dirac equation

Matter determines gravity

Gravity determines dynamics

Joel Bergé, LISA symposium, 05/22/2014

Two successful formalisms - Quantum Field Theory describes small scales (Standard Model) - General Relativity describes large scales

Diagram by Claus Lämmerzahl

Tuesday, June 17, 14

LCDM concordance model: towards new physics?

4

Massey+ 2007

?Dark sector... ...or new physics?

- Modified gravity- Quantum gravity- String theory- New interaction- ...

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

New physics?

5

- Modified gravity - Scalar-vector-tensor theories - Modified action theories (generalizes GR’s action), eg f(R) - ...- Extra scalar field associated to a long range fifth force, coupled to matter (CDM and matter) -- chameleon, dilaton...- Loop quantum gravity- String theory- ...

Predict Equivalence Principle violation e.g. due to coupling’s dependence on matter species => finding such a violation will be a smoking gun for new physics beyond GR.

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

WEP tests up to now

6

Torsion balance

Lunar Laser Range

Eötvös, Eöt-Wash

Probes fall of Earth and Moon towards the Sun

Wagner+ 2012

Joel Bergé, LISA symposium, 05/22/2014

Will 2006

Williams+ 1996

Tuesday, June 17, 14

The near future, what to expect?

7

Microscope10-15

2016

Reaching the limits on Earth => go to space

Both masses do not have the same orbit

Free fall of different materials

Joel Bergé, LISA symposium, 05/22/2014

Will 2006

Expected violations (string theory, new scalar fields...)

Tuesday, June 17, 14

MICROSCOPE measurement principleMicro-satellite à traînée compensée pour l’Observation du Principe d’Equivalence -- Drag-free microsatellite for the observation of the Equivalence Principle

8

Differential electrostatic accelerometer: 2 coaxial cylindrical inertial sensors

Sensors forced to follow the same orbit (permanent pico-meter control) => we measure the electrostatic forces needed to keep the sensors centered.Signal measured along an ultra-sensitive axis.

Signal: gravity field modulated by satellite’s motion around the Earth => sine of known frequency fEPfEP can be varied by either:- Keeping the satellite in inertial

motion- Or spinning it

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

9

What we measure: differential acceleration

EP violation signal

Earth gravity gradient tensor: model, S/C position and attitude

Instrument’s moments of inertia: minimized by AOCS from SST and instr. data

Separation between test masses’ centers: minimized by instrument design

Coriolis acceleration

Relative acceleration

Bias difference: limited thermal fluctuations

Differential mode sensitivity matrix: estimated by in-flight calibration

Non-gravitational accelerations => drag-free system

Quadratic factor

Total acceleration applied to proof-mass

Instrument noise

Angular-linear couplings

Scale factor

Coupling between instrument’s axes

Instrument’s axes / satellite reference frame alignment

Joel Bergé, LISA symposium, 05/22/2014

Common mode sensitivity matrix: estimated by in-flight calibration, limited by design

Tuesday, June 17, 14

Microscope in a nutshellMicro-satellite à traînée compensée pour l’Observation du Principe d’Equivalence -- Drag-free microsatellite for the observation of the Equivalence Principle

10

SU-REF

SU-EP

Payload: T-SAGE (Twin Space Accelerometer for Gravitation Experiment)Two differential electrostatic accelerometers (Sensor Units): - Each accelerometer made of 2 coaxial cylindrical accurate test masses (relative dissymmetry of moments of inertia < 7x10-4, inhomogeneity ~ 10-4)- One with test masses of same composition (Pt/Rh) for reference- The other one with test masses of different composition (Pt/Rh - Ti) for EP test

Satellite- drag compensation (residual< 10-12 ms-2 @ fEP) and fine attitude control (angular stability < 7µrad, velocity < 10-9 rad/s + acceleration < 10-11 rad/s2 @ fEP) => very sensitive 6-axis sensor and very fine actuators- fine passive thermal control (~mK @ fEP) and soft electromagnetic environment- satellite position on orbit known at < 7 m- no mechanism (minimize micro-disturbances eg changes in self-gravity)- magnetic shield for the payload

Dedicated space instrument for EP violation testsPI: Pierre Touboul (ONERA), in collaboration with OCA Nice and CNES

Instrument + Data processing and analysis: ONERA / OCA NiceSatellite: CNES

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Why Pt/Rh and Ti test masses?

11

Overduin+ 2012

Test masses should: - have different nuclear properties to maximize signal - have special macroscopic properties (homogeneity, chemical stability, electrical and magnetic properties) - not be too difficult to machine industrially => Pt/Rh alloy (90%, 10%) Ti/Al/V alloy (90%, 6%, 4%)

Total baryon chargeNeutron/proton difference

Nuclear electrostatic energy

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

T-Sage Sensor Unit

12

SU-REF SU-EP Pumping device

ConnectorsProof masses

Electrode cylinders

Base plate assembly

Blocking device

Vacuum system

Core of the 2 inertial sensors

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Full instrument

13 Joel Bergé, LISA symposium, 05/22/2014

• Sensor Unit (SU) = differential accelerometer• 2 SU on a Mechanics Interface (SUMI)• Each SU = 2 concentric Test-Masses (Pt-Rh/Pt-Rh or Ti/Pt-Rh) • Each mass = inertial sensor (defines measurement frame)

• Front End Electronics Unit (FEEU)• Low noise analog electronic with high stability• One FEEU for each SU• Each FEEU = measure + electrostatic control of 6 degrees of

freedom

• Interface Control Unit (ICU)• 2 ICU stacked = ICUME• 1 ICU for each FEEU• Each ICU embarks 1 DSP + 1 FPGA for test-mass control and

data conditioning for the On Board Computer• Each ICU embarks 2 Power Control Unit (1 nominal + 1

redundant) which converts the sat 28V in very stable secondary voltages (+/-48V, +/-15V,+5V,3.3V)

30 cm x 25 cm x 11 cm – 5kg – 2 x 11W

360 x 348 x 180 mm3 - 25kg

MQV

2 x { 28 cm x 17 cm x 9 cm - 3.5kg - 7W }

MQV1 MV2

Tuesday, June 17, 14

Servo-loop control

14

Electronics control test mass’ position.

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Payload Assembly System

15

Payload Assembly System: - thermally insulates SU and FEEU from the satellite (autonomous passive thermal control) - magnetically shields SU

PAS = 2 stage system:- First stage supports

FEEU and its radiator- Second stage

supports SU and magnetic shielding

Requirements on payload - Thermal stability of SU < 1 mK at fEP - Thermal stability of FEEU < 5 mK at fEP

- Magnetically shielded

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Satellite

16

CNES Myriade satellite - almost “Off-the-shelf”modular micro-satellite - series of satellite (Demeter, Parasol, Picard) - mass: 325 kg - dimensions: 1380 mm x 1040 mm x 1580 mm - Cold Gas propulsion system -> developed by CNES with major ESA contribution

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Status

17

Instrument integrated, undergoing commissioning.

Delivery to CNES for satellite integration in September.

- Metrology: - SU-EP: off-centering 30.8 µm < 34.6 µm (spec) - SU-REF: off-centering 35.7 µm > 34.6 µm (spec) -> taken into account in the error budget: no impact on measurement accuracy

- Environmental tests (SU) - Thermal tests: OK - Vibration tests: OK - Free fall tests: ongoing, final oneJune 2014 (next slide)

- FEEU: tests in June-July 2014

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Catapult tests at ZARM drop tower (February - March 2014)

18

Z - µm/s²

Y - µm/s²apex

4.332 s

XZ

Y

Internal massExternal mass

Time (sec)

Acc

eler

atio

nA

ccel

erat

ion

Joel Bergé, LISA symposium, 05/22/2014

0100

0

100

Time (sec)

Tuesday, June 17, 14

Digital controller response verification

19

Measured position (drop test)

Measured accelerationSimulated PID response from actual measured position

Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Exploitation phase

20 Joel Bergé, LISA symposium, 05/22/2014

What must be done... - accurate measurements of the WEP test in various configurations - inertial pointing with 2 orientations at ascending node - spinning pointing at 2 different frequencies - modify test masses off-centering - validate the performance - accurate in-flight calibration of the major driving parameters - accurate characterization of the instrument thermal behavior and sensitivity to other parameters

... under some constraints - limited gas quantity for the thrusters => priorities established, no improvisation during the mission - operational security => need of planning in advance what to do and how

Tuesday, June 17, 14

Mission scenario

21

The reference mission scenario is established in advance, with well defined sequences and sessions.

- Commissioning phase: 2 months- Preliminary EP test: 1 month- Performance test + optimization of the experiment: 1 month- Calibration + EP test phases: 5 months- Consolidation EP tests: 2.5 months- + unavailability periods (eclipse, Moon): 3 months per year

Some flexibility is allowed to update the mission scenario in a weekly basis.

Nominal mission: 18-24 months

- Launched as auxiliary passenger (Sentinel 1b), Soyuz rocket- Expected as soon as February 2016.- Sun-synchronous orbit, 720 km, eccentricity < 5x10-3

Tuesday, June 17, 14

Ground segment / Science Mission Center

22

Science Mission Center’s status- Development of instrument’s monitoring software in progress- Development of data processing software in progress- Compatibility test with CNES (provides preprocessed data) in January 2015

Joel Bergé, LISA symposium, 05/22/2014

Science Mission Center (CMS) - Ensure all operational functions to maximize instrument’s operation - Day-to-day instrument management and monitoring - Weekly mission performance check - Propose modifications to the mission scenario - Data release and archiving

Tuesday, June 17, 14

Data distribution policy

23

• Proprietary period• Data publicly released after first results

are published• To get access to the data during the

proprietary period:– Call for ideas in 2014– Call for proposals in 2014/2015

Joel Bergé, LISA symposium, 05/22/2014

Talk to me ([email protected]) or Pierre Touboul ([email protected])

Tuesday, June 17, 14

Conclusions

- MICROSCOPE will test the Weak Equivalence Principle in space down to an accuracy of 10-15 (2 orders of magnitude better than current constraints)

- Test of fundamental physics, may rule out new theories that predict an EP violation around 10-14, or even GR

- Will show that the technology is ready for extremely fine satellite attitude control and precise drag-free system

- Launch expected in as soon as February 2016- Results in 2017

24 Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14

Partners

25 Joel Bergé, LISA symposium, 05/22/2014

Tuesday, June 17, 14