2016
DOI: 10.1016/j.astropartphys.2015.10.010
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Secluded WIMPs, dark QED with massive photons, and the galactic center gamma-ray excess

Abstract: We discuss a particular secluded WIMP dark matter model consisting of neutral fermions as the dark matter candidate and a Proca-Wentzel (PW) field as a mediator. In the model that we consider here, dark matter WIMPs interact with standard model (SM) particles only through the PW field of ∼ MeV -multi-GeV mass particles. The interactions occur via a U(1) ′ mediator, V ′ µ , which couples to the SM by kinetic mixing with U(1) hypercharge bosons, B ′ µ . One important difference between our model and other such m… Show more

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Cited by 20 publications
(24 citation statements)
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References 65 publications
(47 reference statements)
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“…Almost every day a paper with a new DM model can be found in arXiv. An obviously incomplete list of recent eprint papers includes [319,320,321,322,323,324,325,326,327,328,205,329,206].…”
Section: Exotic Dm Searchesmentioning
confidence: 99%
“…Almost every day a paper with a new DM model can be found in arXiv. An obviously incomplete list of recent eprint papers includes [319,320,321,322,323,324,325,326,327,328,205,329,206].…”
Section: Exotic Dm Searchesmentioning
confidence: 99%
“…So, in the context of indirect searches, instead of a 2 → 2 annihilation, we have a 2 → 4 one, as can be seen in the right panel of 1. We emphasize that there are many secluded DM models in the literature, which includes dark photons [8,20,21], heavy vector bosons [22,23], and also scalar fields [24,25]. After this brief description of the models, we will follow to the computation of the gamma-ray flux.…”
Section: Pos(icrc2021)577mentioning
confidence: 99%
“…1. We emphasize that there are many secluded DM models in the literature, which includes dark photons [8,20,21], heavy vector bosons [22,23], and also scalar fields [24,25]. After this brief description of the models, we will follow to the computation of the gamma-ray flux.…”
Section: Secluded Modelsmentioning
confidence: 99%