Self-Interacting Dark Matter with Naturally Light Mediator
arXiv:1608.08277 · doi:10.1142/S0217732317500389
Abstract
A promising proposal for resolving the cusp-core anomaly in the density profile of dwarf galaxies is to allow dark matter to interact with itself through a light mediator of mass much less than a GeV. The theoretical challenge is to have a complete renormalizable theory where this happens naturally even though dark matter itself may be of the electroweak scale, i.e. 100 GeV to 1 TeV. I propose here such a model, with just two neutral complex scalar singlets under a softly broken dark global U(1) symmetry.
arXiv comment11 pages, 5 figures (discussion added)
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Cited by in corpus (7)
- Dark Matter Self-interactions and Small Scale Structure
- Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons
- Dark matter self-interactions from a general spin-0 mediator
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