29 March 2023 to 1 April 2023
UCLA
US/Pacific timezone

Sub-GeV Dark Matter Searches with EDELWEISS and CRYOSEL

31 Mar 2023, 13:15
15m
PAB- 1-425 (UCLA)

PAB- 1-425

UCLA

UCLA Department of Physics and Astronomy 475 Portola Plaza, Los Angeles, CA 90095

Speaker

Jules GASCON

Description

The EDELWEISS collaboration searches for light Dark Matter (DM) particles using germanium detectors equipped with a charge and phonon signal readout.
To circumvent the problem of the large background of events with no ionisation signal ("Heat-Only" events) that limit the sensitivity of our detectors equipped with Ge-NTD sensors, the collaboration has tested the use of NbSi Transition Edge Sensors (TES). The observed HO background reduction in a 200g detector equipped with a TES readout and operated underground in the Laboratoire Souterrain de Modane (LSM) has yielded a sensivity to DM masses down to 32 MeV/c² and cross sections down to 10-29 cm². Further improvements have been more recently obtained by exploting the phonon yield from the Neganov-Luke-Trofimov effect to better resolve electron recoils from HO events. These results pave the way for a new detector design, named CRYOSEL, that is being optimized for such a discrimination.

Primary author

Presentation materials