Connecting neutrino physics with dark matter

被引：35
|
作者：
Lattanzi, Massimiliano [1 ]
Lineros, Roberto A. [2 ]
Taoso, Marco [3 ]
机构：
[1] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy
[2] Ist Nazl Fis Nucl, Sez Ferrara, Polo Sci & Tecnol, I-44122 Ferrara, Italy
[3] Univ Valencia, CSIC, Inst Fis Corpuscular, E-46980 Paterna, Spain
来源：
NEW JOURNAL OF PHYSICS | 2014年 / 16卷
基金：
欧洲研究理事会;
关键词：
neutrinos; dark matter; flavour; majoron; sterile neutrinos; HUBBLE-SPACE-TELESCOPE; STERILE NEUTRINOS; INFLATIONARY UNIVERSE; CONSTRAINTS; MASSES; MAJORON; MODELS; SYMMETRY; VIOLATION; FLATNESS;
D O I：
10.1088/1367-2630/16/12/125012
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The origin of neutrino masses and the nature of dark matter are two in most pressing open questions in modern astro-particle physics. We consider here the possibility that these two problems are related, and review some theoretical scenarios which offer common solutions. A simple possibility is that the dark matter particle emerges in minimal realizations of the seesaw mechanism, as in the majoron and sterile neutrino scenarios. We present the theoretical motivation for both models and discuss their phenomenology, confronting the predictions of these scenarios with cosmological and astrophysical observations. Finally, we discuss the possibility that the stability of dark matter originates from a flavor symmetry of the leptonic sector. We review a proposal based on an A(4) flavor symmetry.
引用
收藏
页数：19
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