Journal
PHYSICAL REVIEW LETTERS
Volume 113, Issue 17, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.113.171301
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Funding
- U.S. National Science Foundation [PHY-1002399]
- Israel Science Foundation
- US-Israel Binational Science Foundation
- EU-FP7 Marie Curie
- CIG fellowship
- I-CORE Program of the Planning Budgeting Committee
- Israel Science Foundation [1937/12]
- DOE [DE-AC02-76-SF00515]
- Weizmann Institute of Science-National Postdoctoral Award Program for Advancing Women in Science
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We present a new paradigm for achieving thermal relic dark matter. The mechanism arises when a nearly secluded dark sector is thermalized with the standard model after reheating. The freeze-out process is a number-changing 3 -> 2 annihilation of strongly interacting massive particles (SIMPs) in the dark sector, and points to sub-GeV dark matter. The couplings to the visible sector, necessary for maintaining thermal equilibrium with the standard model, imply measurable signals that will allow coverage of a significant part of the parameter space with future indirect-and direct-detection experiments and via direct production of dark matter at colliders. Moreover, 3 -> 2 annihilations typically predict sizable 2 -> 2 self-interactions which naturally address the core versus cusp and too-big-to-fail small-scale structure formation problems.
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