The AMS Transition Radiation Detector and the Search for Dark Matter Gianpaolo Carosi Lab for...

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Transcript of The AMS Transition Radiation Detector and the Search for Dark Matter Gianpaolo Carosi Lab for...

The AMS Transition Radiation Detector and the Search for Dark Matter

Gianpaolo Carosi Lab for Nuclear Science, MIT The AMS Collaboration Lake Louise Winter Institute 2/23/05

Outline• Signatures of dark matter in cosmic rays

• Overview of the AMS-02 detector

• Principles of Transition Radiation

• Construction of the AMS TRD system

• Physics reach of AMS-02 detector with the TRD

The Problem of Dark Matter• What is it?

-Matter which appears to not interact electromagnetically.

-Observed from gravitational interactions only!

v2

v1

Galactic Rotation Curves

R1

R2

R2R1

v1 v2

00 SUSY Dark Matter

• Neutralino – majorana particles

Direct searches: Scattering off nuclei

Indirect searches: Look for annihilation products.

Positrons: low intrinsic background

Energy correlated to WIMP mass

X 0

X 0

e+

e-

HEATBalloon Experiment

ve

ve

_

AMS-02 experimentConstraints:•9 g at takeoff/landing.•Weight < 14809 lbs•Power = 3 kW•Temperature: -40˚ - +65˚ C•Date rate = 2 Mb/sec•3 year remote operation without servicing

Operational ExperienceAMS-01 engineering test flight10 days: ~ 100 Million events

ISS

The Experiment

TRD: p+ rejection 102-103

ECAL: p+ rejection 103-104

Principle of Transition RadiationHigh energy charged particles crossing boundary between materials of different dielectric constants gives off X-rays.

Detection possible with Lorentz boosts > 300.

Discriminate e+ (TR) / p+ (no TR)

AMS TRD: Proportion tubes and fleece radiator

Construction of AMS TRDTRD Octagon/straw tubesRWTH Aachen

TRD Gas Supply/Circulation SystemMIT – Design CERN & MIT - Construction

TRD Slow Control SystemMIT & INFN Rome

TRD DAQTH Karlsruhe

DAQ Electronics Slow Control and Monitoring

50 liter/hr

DetectorVolume

DistributionSystem

CirculationSystem

Supply/MixingSystem

Vibration TestsThermal Vacuum Tests

Leak Tests

Extensive Testing

328 Modules (5248 straw tubes) Lengths: 0.8 – 2.0 m and 100 μm tolerance

Straw tube walls

Carbon Fiber Structure

Aachen

328 straw modules have been produced:

Gas System: Box S

• Mix Gas:

Xe:CO2 80:20

(to 1% accuracy)

• Refresh Supply Daily:

max 7 liter/day

Engineering model: CERN Flight system: ARDE Corp.

Xe49.5 kg

CO2

4.5 kg

Gas System:Box C• Circulate Gas:

50 liter/hr through Octagon• Monitor gas gain:

Calibration tubes coated with Fe55

Spirometer: Measures CO2 fraction

TRD Gas Slow Control/Monitoring

TRD DAQTRD FE-electronics: 20 Watt for 5248 channels => multiplexed pulse height only

• 20 layer TRD detector in the test beam at CERN in 2000• we have recorded 3 million events providing signals for protons, electrons,

muons and pions at energies from 5-250 GeV

HEAT experiment(experimental data + DM model)

AMS-02 experiment(simulated data + DM model)

Physics Reach

TRD + ECAL

Paolo Maestro: SIENA

AMS on the ISS: 2008

AMS TRD currently under constructionBeam tests: achieve 102-103 p+ rejection to 300 GeVCombined with ECAL will obtain precise e+ spectrum

Summary