2-9 julio 2014
Valencia, Spain
Europe/Madrid timezone

Low-Mass Dark Matter Searches with Sub-keV Germanium Detectors

4 jul. 2014 12:06
18m
Auditorium 3A ()

Auditorium 3A

Oral presentation Astroparticle Physics and Cosmology Astroparticle Physics and Cosmology

Ponente

Dr. ARUN KUMAR SOMA (ACADEMIA SINICA)

Descripción

Germanium detectors with sub-keV sensitivities can probe low-mass WIMP Dark Matter. This experimental approach is pursued at the Kuo-Sheng Neutrino Laboratory (KSNL) in Taiwan and at the China Jinping Underground Laboratory (CJPL) in China via the TEXONO and CDEX programs, respectively. The highlights of R&D efforts on point-contact germanium detectors and in particular the differentiation of surface and bulk events by pulse shape analysis [1] will be described. The latest results on WIMP-nucleon scattering cross-sections [2] will be presented. Some of the allowed parameter space implied by other experiments are probed and excluded. Future prospects will be discussed. 1. H.B. Li et al., Astropart. Phys. 56, 1 (2014) 2. H.B. Li et al., Phys. Rev. Lett. 110, 261301 (2013) ; W. Zhao et al. Phys. Rev. D 88, 052004 (2013).

Autor primario

Dr. ARUN KUMAR SOMA (ACADEMIA SINICA)

Materiales de la presentación

Ponencia

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