Masses of active neutrinos in the νMSM from x-ray astronomy

被引：71

作者：

Boyarsky, A ^{[1
]}

Neronov, A

Ruchayskiy, O

Shaposhnikov, M

机构：

[1] CERN, Div Theory, CH-1211 Geneva 23, Switzerland

[2] Observ Geneva, CH-1290 Sauveray, Switzerland

[3] INTEGRAL Sci Data Ctr, CH-1290 Versoix, Switzerland

[4] Inst Hautes Etud Sci, F-91440 Bures Sur Yvette, France

[5] Ecole Polytech Fed Lausanne, Inst Theoret Phys, FSB, ITP,LPPC, CH-1015 Lausanne, Switzerland

来源：

JETP LETTERS | 2006年 / 83卷 / 04期

关键词：

D O I：

10.1134/S0021364006040011

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In an extension of the Standard Model by three relatively light right-handed neutrinos (the vMSM model) the role of the dark matter particle is played by the lightest sterile neutrino. We demonstrate that the observations of the extragalactic x-ray background allow us to put a strong upper bound on the mass of the lightest active neutrino and predict the absolute values of the mass of the two heavier active neutrinos in the vMSM provided that the mass of the dark matter sterile neutrino is larger than 1.8 keV.

引用

页码：133 / 135

页数：3

共 27 条

[1] Direct detection of warm dark matter in the X-ray [J].