Freeze-in dark matter within the seesaw mechanism

被引:1
作者
Lucente, Michele [1 ,2 ,3 ]
机构
[1] Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[2] INFN Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[3] Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany
关键词
Type-I seesaw; Dark matter; Freeze-in; Neutrinos; Lepton number symmetry; LYMAN-ALPHA FOREST; STERILE NEUTRINOS; MASSES; CONSTRAINTS; VIOLATION; SYMMETRY; DECAYS; VMSM; MSM;
D O I
10.1016/j.physletb.2023.138206
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that the minimal Type-I Seesaw mechanism can successfully account for the observed dark matter abundance in the form of a keV sterile neutrino. This population can be produced by the decay of the heavier neutral leptons, with masses above the electroweak mass scale, while they are in thermal equilibrium in the early Universe (freeze-in). Moreover, the implementation of the relevant phenomenological constraints (relic abundance, indirect detection and structure formation) on this model automatically selects a region of the parameter space featuring an approximate lepton number symmetry.(c) 2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons .org /licenses /by /4 .0/). Funded by SCOAP3.
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页数:7
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