PIRSA:12040104

The Direct Detection of sub-GeV Dark Matter: First Limits and Future Prospects

Essig, R. (2012). The Direct Detection of sub-GeV Dark Matter: First Limits and Future Prospects. Perimeter Institute. https://pirsa.org/12040104

Essig, Rouven. The Direct Detection of sub-GeV Dark Matter: First Limits and Future Prospects. Perimeter Institute, Apr. 17, 2012, https://pirsa.org/12040104 

          @misc{ pirsa_PIRSA:12040104,
            doi = {10.48660/12040104},
            url = {https://pirsa.org/12040104},
            author = {Essig, Rouven},
            keywords = {Particle Physics},
            language = {en},
            title = {The Direct Detection of sub-GeV Dark Matter: First Limits and Future Prospects},
            publisher = {Perimeter Institute},
            year = {2012},
            month = {apr},
            note = {PIRSA:12040104 see, \url{https://pirsa.org}}
          }

Rouven Essig Stony Brook University

DOI 10.48660/12040104
Collection
Talk Type Scientific Series
Subject

Abstract

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.