16–19 Oct 2012
INFN-LNF
Europe/Rome timezone

First Direct Detection Limits on sub-GeV Dark Matter and Future Prospects

18 Oct 2012, 12:10
35m
Aula B. Touschek, Bldg 36 (INFN-LNF)

Aula B. Touschek, Bldg 36

INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy

Speaker

Prof. Rouven Essig (Stony Brook University)

Description

Direct dark matter (DM) detection experiments almost always focus on Weakly Interacting Massive Particles (WIMPs), which have a mass in the 1--1000 GeV range. However, what if DM is not a WIMP? In this talk, new direct detection strategies for DM particles with MeV to GeV mass will be presented. In this largely unexplored mass range, DM can scatter with electrons, causing ionization of atoms in a detector target material and leading to single- or few-electron events. I will present the first direct detection limits on DM as light as a few MeV, using XENON10 data. Theoretically interesting models can already be probed. Significant improvements in sensitivity should be possible with dedicated experiments, opening up a window to new regions in DM parameter space.

Primary author

Prof. Rouven Essig (Stony Brook University)

Presentation materials

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