2015
DOI: 10.1016/j.physletb.2015.01.001
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AMS02 positron excess from decaying fermion DM with local dark gauge symmetry

Abstract: Positron excess observed by PAMELA, Fermi and AMS02 may be due to dark matter (DM) pair annihilation or decay dominantly into muons. In this paper, we consider a scenario with thermal fermionic DM (χ ) with mass ∼O (1-2) TeV decaying into a dark Higgs (φ) and an active neutrino (ν a ) instead of the SM Higgs boson and ν a . We first present a renormalizable model for this scenario with local dark U (1) X gauge symmetry, in which the DM χ can be thermalized by Higgs portal and the gauge kinetic mixing.Assuming … Show more

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Cited by 11 publications
(8 citation statements)
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“…First of all, let us consider DM models where weak scale DM is stabilized by some spontaneously broken local dark gauge symmetries [14][15][16][17][18][19][20][21][22][23][24][25]. This possibility is not that often JHEP10 (2015)057 considered seriously.…”
Section: Dark Matter Models With Dark Gauge Symmetries And/or Higgs Pmentioning
confidence: 99%
“…First of all, let us consider DM models where weak scale DM is stabilized by some spontaneously broken local dark gauge symmetries [14][15][16][17][18][19][20][21][22][23][24][25]. This possibility is not that often JHEP10 (2015)057 considered seriously.…”
Section: Dark Matter Models With Dark Gauge Symmetries And/or Higgs Pmentioning
confidence: 99%
“…In contrast, decaying DM does not require a large boost factor as long as the decay lifetime is around 10 26 to 10 27 seconds [41][42][43][44][45][46][47][48][49][50], depending on the DM mass and decay channels. The γ-ray bound, nevertheless, still applies in this case and has ruled out many decaying DM models based on two-body decays [51][52][53][54][55].…”
Section: Introductionmentioning
confidence: 99%
“…It is natural to assume that DM may have some kind of (its own) gauge symmetries [26][27][28][29][30][31][32][33][34][35][36][37][38]. And then there could be other extra dark fields (such as dark Higgs or dark gauge fields) which might be not that heavy and so we may have to include them in our simplified models.…”
Section: Jhep01(2017)086mentioning
confidence: 99%