2020
DOI: 10.48550/arxiv.2012.01875
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Light dark matter from dark sector decay

Yu Cheng,
Wei Liao

Abstract: We study the possibility that light dark matter can be produced with right relic density by the decay of other dark sector particles. We study this possibility in a model with right-handed neutrinos, a dark sector singlet scalar and a dark sector singlet fermion. The decay of the heavier dark sector singlet scalar gives rise to the lighter dark sector singlet fermion which serves as the dark matter candidate. We show that the right dark matter relic density can be produced by the decay of the dark sector singl… Show more

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Cited by 2 publications
(3 citation statements)
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“…In our FIMP DM scenarios, the next lightest stable particle (NLSP) decays into DM and sterile neutrinos N when N is light enough. For λ ds 10 −12 , NLSP decays fast to avoid constraints from BBN [37]. On the other hand, NLSP will decay to DM and light neutrinos through χ → φν or φ → χν when the N is heavier than the dark sector.…”
Section: Constraintsmentioning
confidence: 99%
See 1 more Smart Citation
“…In our FIMP DM scenarios, the next lightest stable particle (NLSP) decays into DM and sterile neutrinos N when N is light enough. For λ ds 10 −12 , NLSP decays fast to avoid constraints from BBN [37]. On the other hand, NLSP will decay to DM and light neutrinos through χ → φν or φ → χν when the N is heavier than the dark sector.…”
Section: Constraintsmentioning
confidence: 99%
“…Meanwhile, observable signature is still expected by indirect detection [28][29][30]32]. On the other hand, the coupling between DM and N can be tiny, thereby producing DM via the freeze-in mechanism [33][34][35][36][37][38][39]. Leptogenesis in the frame work of neutrino portal DM is also discussed in Ref.…”
Section: Introductionmentioning
confidence: 99%
“…The relation between these intriguing phenomena has been investigated in many works . One of the interesting possibilities is to connect the dark sector and the Standard Model through the RH neutrinos that realise the type I seesaw, which is usually named the neutrino portal scenario [102][103][104][105][106][107][108][109][110][111][112]. Some recent research [102][103][104] shows that dark matter particles can be dominantly produced through the neutrino Yukawa interactions in the seesaw sector non-thermally by the so-called "freeze-in" mechanism [113,114].…”
mentioning
confidence: 99%