Indirect dark matter detection in the light of sterile neutrinos

被引:4
|
作者
Esmaili, Arman [1 ]
Peres, O. L. G. [1 ,2 ,3 ]
机构
[1] Univ Estadual Campinas, Inst Fis Gleb Wataghin, BR-13083859 Campinas, SP, Brazil
[2] Arizona State Univ, Tempe, AZ 85287 USA
[3] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2012年 / 05期
基金
巴西圣保罗研究基金会;
关键词
dark matter theory; neutrino properties; OSCILLATIONS; SOLAR;
D O I
10.1088/1475-7516/2012/05/002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The recent global fit of short baseline neutrino oscillation data favors the presence of one (or more) sterile neutrino state which leads to new mass splitting Delta m(2) similar to 1eV(2). We consider the effect of this new states on the evolution of neutrinos from the dark matter annihilation inside the Sun. We show that neutrinos with energy E-nu greater than or similar to 100 GeV undergo resonant active-sterile oscillation which depletes the flux of neutrinos arriving at the Earth. As an example of this effect, we present the oscillation probabilities for the case of monochromatic neutrinos front the direct annihilation of dark matter particles to neutrinos and the depletion due to the presence of sterile neutrinos. We discuss the seasonal variation of oscillation probabilities which is expected for the case of monochromatic neutrinos.
引用
收藏
页数:14
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