The Heidelberg Dark Matter Search Experiment

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The Heidelberg Dark Matter Search Experiment Laura Baudis Stanford University

description

The Heidelberg Dark Matter Search Experiment. Laura Baudis Stanford University. The HDMS collaboration. MPI fuer Kernphysik, Heidelberg Group of Prof. H.V. Klapdor-Kleingrothaus. The HDMS detectors. WIMP. 2 HPGe detectors in one cryostat system inner: WIMP target outer: active veto - PowerPoint PPT Presentation

Transcript of The Heidelberg Dark Matter Search Experiment

Page 1: The Heidelberg Dark Matter Search Experiment

The Heidelberg Dark Matter Search Experiment

Laura Baudis

Stanford University

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The HDMS collaboration

MPI fuer Kernphysik, Heidelberg

Group of Prof. H.V. Klapdor-Kleingrothaus

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The HDMS detectors

2 HPGe detectors in one

cryostat system

inner: WIMP target

outer: active veto

against multiple Comptons

passive Ge shield

WIMP

gamma

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Property Inner Detector Outer Detector

Crystal type p-type n-type

Mass [g] 202 2111

Active vol [cc] 37 383

Diameter [mm] 35.2 84.4

Length [mm] 40.3 86.2

Op. bias [V] + 2500 -1500

FWHM @ 300 keV

(1332 keV) [keV]

1.2 (1.87) 3.2 (4.45)

Threshold [keV] 2.0 7.5

Some detector properties

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Cross talk between detectors

linear correlation:correction offline

kio = 0.00375 +/- 0.43 x 10-4

koi = 0.12850 +/- 0.27 x 10-3

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Cross talk induced error

compare zero energy resolutions:

inner: no effectouter: from 0.3% to 0.4% at 1332 keV

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The HDMS detector

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HDMS in Gran Sasso

prototype: March 98-July 99

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Performance @ GS

stable running over ~ 15 months

individual runs ~ 0.9 dchecked daily: leakage current nitrogen flow overall trigger individual count rate, etc

weekly: calibration with 133Ba, 152Eu-232Th source

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Outer detector: 363 raw live-d

68Ge, 57Co, 58Co, 54Mn, 60Co, 65Zn, 137Cs, 238U, 232Th, 40K

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Inner detector: 363 raw live-d

68Ge, 54Mn, 57Co, 60Co, 210Pb, 212Pb, 214Pb, 40K

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Background model

MC simulation of dominant backgrd. MC simulation of dominant backgrd. sources with extended GEANT3.21sources with extended GEANT3.21

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Inner: low energy spectrum

68Ga X-ray

49Ti, 55Mncross talk?

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Structure at 32 keV: cross talk?

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Anticoincidence between inner and outer

Eth for anticoincidence: 3 sigma away from zero

threshold

[keV]

FWHM/2.35

[keV]

inner 2.0 0.40

outer 7.5 1.42

40-100 keV: factor 4.3

11-40 keV: 0.2 events/kg d keV40-100 keV: 0.07 events/kg d keV

3

1.2 keV

4.3 keV

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HDMS prototype limits

only last 49 d of data taking: 9.9 kg d2-30 keV: 0.5 events/kg y keV

L. Baudis et al., PRD63,2000

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73Ge-HDMS: full scale

inner crystal replaced by 73Ge crystalsensitive to spin-dependent interactions70Ge de-enriched by factor >50new copper holder systemno soldering of contacts

installed in GS: August 2000working wellfirst analysis: fall 2001?expectation: test DAMA withindependent technique and raw data

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HDMS goal

Based on: 0.07 events/kg d keV in 2 - 30 keV region

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Conclusions

HDMS prototype worked welllimits competitive to other Ge experiments

73Ge-HDMS installed in August 2000first 73Ge detector!first data to be analyzed soon...independent test of DAMA region sensitive to spin-dependent interaction

however, increase of target mass improbableno sensitivity to a WIMP signature