Published December 1, 2017 | Version Published + Submitted
Journal Article Open

Light dark matter: Models and constraints

  • 1. ROR icon Lawrence Berkeley National Laboratory
  • 2. ROR icon University of California, Berkeley
  • 3. ROR icon University of California, San Diego

Abstract

We study the direct detection prospects for a representative set of simplified models of sub-GeV dark matter (DM), accounting for existing terrestrial, astrophysical and cosmological constraints. We focus on dark matter lighter than an MeV, where these constraints are most stringent, and find three scenarios with accessible direct detection cross sections: (i) DM interacting via an ultralight kinetically mixed dark photon, (ii) a DM subcomponent interacting with nucleons or electrons through a light scalar or vector mediator, and (iii) DM coupled with nucleons via a mediator heavier than ∼100 keV.

Additional Information

© 2017 American Physical Society. (Received 30 October 2017; published 26 December 2017) We thank Claudia Frugiuele, Dan Green, Ed Hardy, Rob Lasenby, Zoltan Ligeti, Sam McDermott, Michele Papucci, Surjeet Rajendran, Sean Tulin, Haibo Yu, and Yiming Zhong for useful discussions. We also thank Robert Lasenby for discussions leading to an updated SN1987a bound for the leptophilic model, and Surjeet Rajendran and Dan Green for discussions leading to a numerical correction in the BBN constraints for the B-L model. The authors are supported by the DOE under Contract No. DE-AC02-05CH11231. T. L. is further supported by NSF Grant No. PHY-1316783. We thank the Aspen Center for Physics, supported by the NSF Grant No. PHY-1066293, for hospitality while parts of this work were completed.

Attached Files

Published - PhysRevD.96.115021.pdf

Submitted - 1709.07882.pdf

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Additional details

Identifiers

Eprint ID
96435
Resolver ID
CaltechAUTHORS:20190613-164151727

Related works

Funding

Department of Energy (DOE)
DE-AC02-05CH11231
NSF
PHY-1316783
NSF
PHY-1066293

Dates

Created
2019-06-18
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

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Caltech groups
Physics Department