Two loop neutrino model with dark matter and leptogenesis

被引：16

作者：

Kashiwase, Shoichi ^{[1
]}

Okada, Hiroshi ^{[2
,3
]}

Orikasa, Yuta ^{[2
,4
]}

Toma, Takashi ^{[5
]}

机构：

[1] Kanazawa Univ, Inst Theoret Phys, Kanazawa, Ishikawa 9201192, Japan

[2] KIAS, Sch Phys, Seoul 130722, South Korea

[3] Natl Ctr Theoret Sci, Div Phys, Hsinchu 300, Taiwan

[4] Seoul Natl Univ, Dept Phys & Astron, Seoul 151742, South Korea

[5] Univ Paris 11, CNRS UMR 8627, Phys Theor Lab, F-91405 Orsay, France

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 2016年 / 31卷 / 20-21期

关键词：

Radiative seesaw; global U(1) symmetry; dark matter; resonant leptogenesis; MASS MODEL; BARYOGENESIS;

D O I：

10.1142/S0217751X16501219

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

In this paper, we study a two-loop induced radiative neutrino model at TeV scale with global U(1) symmetry, in which we analyze dark matter and resonant leptogenesis. The model includes two kinds of dark matter candidates. We discuss what kind of dark matter can satisfy the observed relic density as well as the current direct detection bound, and be simultaneously compatible with the leptogenesis. We also discuss whether our resonant leptogenesis can be differentiated from the other scenarios at TeV scale or not.

引用

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