6533b857fe1ef96bd12b5001

RESEARCH PRODUCT

Background discrimination capabilities of a heat and ionization germanium cryogenic detector

P. Di StefanoAngélique BenoitL. BergéA. BroniatowskiB. ChambonM. ChapellierG. ChardinP. CharvinJ. ChaumontM. De JésusD. DrainL. DumoulinPhilippe ForgetP. GarocheJ. GasconC. GoldbachM. GrosA. JuillardA. De LesquenD. L'hôteJ. MalletJ. ManginS. MarnierosN. MirabolfathiL. MiramontiL. MoscaX.f. NavickG. NollezP. PariS. PécourtE. SimonL. StabM. SternJ-p. TorreR. TourbotD. Yon

subject

Dark matterPopulationFOS: Physical sciencesAstrophysicsEDELWEISSAstrophysics01 natural scienceslaw.inventionNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]RecoillawIonization0103 physical sciencesNeutron010306 general physicseducationPhysicseducation.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsBolometerDetectorAstrophysics (astro-ph)Astronomy and AstrophysicsDark matter ; WIMP ; cryogenic detector

description

The discrimination capabilities of a 70 g heat and ionization Ge bolometer are studied. This first prototype has been used by the EDELWEISS Dark Matter experiment, installed in the Laboratoire Souterrain de Modane, for direct detection of WIMPs. Gamma and neutron calibrations demonstrate that this type of detector is able to reject more than 99.6% of the background while retaining 95% of the signal, provided that the background events distribution is not biased towards the surface of the Ge crystal. However, the 1.17 kg.day of data taken in a relatively important radioactive environment show an extra population slightly overlapping the signal. This background is likely due to interactions of low energy photons or electrons near the surface of the crystal, and is somewhat reduced by applying a higher charge-collecting inverse bias voltage (-6 V instead of -2 V) to the Ge diode. Despite this contamination, more than 98% of the background can be rejected while retaining 50% of the signal. This yields a conservative upper limit of 0.7 event.day^{-1}.kg^{-1}.keV^{-1}_{recoil} at 90% confidence level in the 15-45 keV recoil energy interval; the present sensitivity appears to be limited by the fast ambient neutrons. Upgrades in progress on the installation are summarized.

10.1016/s0927-6505(00)00127-4http://hdl.handle.net/2434/28208