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Direct Detection of Sub-GeV Dark Matter: Models and Constraints

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

I will make some general comments about the search for dark matter and other new particles, contrasting current research trends with those 10 years ago. I will then focus on recent ideas for direct detection experiments to search for dark matter with masses in the MeV-to-GeV range. I will then discuss briefly three topics: (i) the solar neutrino background (or “how low in cross section (interaction strength) can future direct-detection experiments probe before solar neutrinos become an irreducible background”), (ii) novel constraints on low-mass dark matter from Supernova 1987A, and (iii) strongly interacting dark matter (or “how large in cross section can direct-detection experiments probe before terrestrial effects stop sub-GeV dark matter from reaching the detector”).

Original languageEnglish
Title of host publicationIlluminating Dark Matter - Proceedings of a Simons Symposium, 2018
EditorsRouven Essig, Jonathan Feng, Kathryn Zurek
PublisherSpringer
Pages59-67
Number of pages9
ISBN (Print)9783030315924
DOIs
StatePublished - 2019
EventSimons Symposium on Illuminating Dark Matter, 2018 - Krün, Germany
Duration: May 13 2018 → May 19 2018

Publication series

NameAstrophysics and Space Science Proceedings
Volume56
ISSN (Print)1570-6591
ISSN (Electronic)1570-6605

Conference

ConferenceSimons Symposium on Illuminating Dark Matter, 2018
Country/TerritoryGermany
CityKrün
Period05/13/18 → 05/19/18

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