English

Background discrimination capabilities of a heat and ionization germanium cryogenic detector

Astrophysics 2009-10-31 v1

Abstract

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.

Keywords

Cite

@article{arxiv.astro-ph/0004308,
  title  = {Background discrimination capabilities of a heat and ionization germanium cryogenic detector},
  author = {P. Di Stefano and L. Berge and B. Chambon and M. Chapellier and J. Chaumont and G. Chardin and P. Charvin and M. De Jesus and D. Drain and L. Dumoulin and P. Forget and P. Garoche and J. Gascon and C. Goldbach and D. L'Hote and J. Mallet and J. Mangin and S. Marnieros and L. Miramonti and L. Mosca and X. -F. Navick and G. Nollez and P. Pari and S. Pecourt and E. Simon and L. Stab and J. -P. Torre and R. Tourbot and D. Yvon},
  journal= {arXiv preprint arXiv:astro-ph/0004308},
  year   = {2009}
}

Comments

Submitted to Astroparticle Physics, 14 pages