Simple theory for scotogenic dark matter with residual matter-parity

被引：17

作者：

Hernandez, A. E. Carcamo ^{[1
]}

Valle, Jose W. F. ^{[2
]}

Vaquera-Araujo, Carlos A. ^{[3
,4
]}

机构：

[1] Univ Tecn Federico Santa Maria, Dept Fis, Casilla 110 5, Valparaiso, Chile

[2] Univ Valencia, CSIC, Inst Fis Corpuscular, AHEP Grp, Parc Cient Paterna,C Catedrat Jose Beltran 2, E-46980 Paterna, Valencia, Spain

[3] Univ Guanajuato, DCI, Dept Fis, Campus Leon,Loma Bosque 103, Guanajuato 37150, Mexico

[4] Consejo Nacl Ciencia & Technol, Ave Insurgentes Sur 1582, Ciudad De Mexico 03940, Mexico

来源：

PHYSICS LETTERS B | 2020年 / 809卷

关键词：

MODEL; VIOLATION;

D O I：

10.1016/j.physletb.2020.135757

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Dark matter stability can result from a residual matter-parity symmetry surviving spontaneous breaking of an extended gauge symmetry. We propose the simplest scotogenic dark matter completion of the original SVS theory [1], in which the "dark sector" particles as well as matter-parity find a natural theoretical origin within the model. We briefly comment on its main features. (C) 2020 The Authors. Published by Elsevier B.V.

引用

页数：10

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