Thermal effects in freeze-in neutrino dark mater production

被引:1
作者
Abada, A. [1 ]
Arcadi, G. [2 ,3 ]
Lucente, M. [4 ,5 ]
Piazza, G. [1 ]
Rosauro-Alcaraz, S. [1 ]
机构
[1] CNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, France
[2] Univ Messina, Dipartimento Sci Matemat & Informat Sci Fis & Sci, Via Ferdinando Stagno dAlcontres 31, I-98166 Messina, Italy
[3] INFN, Sez Catania, Via Santa Sofia 64, I-95123 Catania, Italy
[4] Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[5] INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
关键词
Early Universe Particle Physics; Models for Dark Matter; Particle Nature of Dark Matter; Sterile or Heavy Neutrinos; STERILE NEUTRINOS; MATTER; CONSTRAINTS; SYMMETRY; MASSES; LIMITS; VMSM;
D O I
10.1007/JHEP11(2023)180
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We present a detailed study of the production of dark matter in the form of a sterile neutrino via freeze-in from decays of heavy right-handed neutrinos. Our treatment accounts for thermal effects in the effective couplings, generated via neutrino mixing, of the new heavy neutrinos with the Standard Model gauge and Higgs bosons and can be applied to several low-energy fermion seesaw scenarios featuring heavy neutrinos in thermal equilibrium with the primordial plasma. We find that the production of dark matter is not as suppressed as to what is found when considering only Standard Model gauge interactions. Our study shows that the freeze-in dark matter production could be efficient.
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页数:39
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