Self-interacting scalar dark matter with local symmetry
arXiv:1402.6449 · doi:10.1088/1475-7516/2014/05/047
Abstract
We construct a self-interacting scalar dark matter (DM) model with local discrete symmetry that stabilizes a weak scale scalar dark matter . The model assumes a hidden sector with a local dark gauge symmetry, which is broken spontaneously into subgroup by nonzero VEV of dark Higgs field (). Compared with global DM models, the local model has two new extra fields: a dark gauge field and a dark Higgs field (a remnant of the breaking). After imposing various constraints including the upper bounds on the spin-independent direct detection cross section and thermal relic density, we find that the scalar DM with mass less than GeV is allowed in the local model, in contrary to the global model. This is due to new channels in the DM pair annihilations open into and in the local model. Most parts of the newly open DM mass region can be probed by XENON1T and other similar future experiments. Also if is light enough (a few MeV O(100) MeV), it can generate a right size of DM self-interaction and explain the astrophysical small scale structure anomalies. This would lead to exotic decays of Higgs boson into a pair of dark Higgs bosons, which could be tested at LHC and ILC.
17 pages, 3 figures; references updated; version appears in JCAP
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