Boosting the production of sterile neutrino dark matter with self-interactions

被引:2
作者
Astros, Maria Dias [1 ]
Vogl, Stefan [1 ]
机构
[1] Univ Freiburg, Inst Phys, Herrmann Herder Str 3, D-79104 Freiburg, Germany
关键词
Early Universe Particle Physics; Particle Nature of Dark Matter; Sterile or Heavy Neutrinos; CONSTRAINTS; BARYOGENESIS; DISPERSION; MASS;
D O I
10.1007/JHEP03(2024)032
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
Sterile neutrinos are well-motivated and simple dark matter (DM) candidates. However, sterile neutrino DM produced through oscillations by the Dodelson-Widrow mechanism is excluded by current X-ray observations and bounds from structure formation. One minimal extension, that preserves the attractive features of this scenario, is self-interactions among sterile neutrinos. In this work, we analyze how sterile neutrino self-interactions mediated by a scalar affect the production of keV sterile neutrinos for a wide range of mediator masses. We find four distinct regimes of production characterized by different phenomena, including partial thermalization for low and intermediate masses and resonant production for heavier mediators. We show that significant new regions of parameter space become available which provide a target for future observations.
引用
收藏
页数:26
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