PPPC 4 DMv: a Poor Particle Physicist Cookbook for Neutrinos from Dark Matter annihilations in the Sun

被引：59

作者：

Baratella, Pietro ^{[1
,2
]}

Cirelli, Marco ^{[3
,4
]}

Hektor, Andi ^{[5
,6
]}

Pata, Joosep ^{[5
]}

Piibeleht, Morten ^{[5
]}

Strumia, Alessandro ^{[2
,5
,7
]}

机构：

[1] Scuola Normale Super Pisa, I-56126 Pisa, Italy

[2] Ist Nazl Fis Nucl, I-56126 Pisa, Italy

[3] CNRS, URA 2306, Inst Phys Theor, F-91191 Gif Sur Yvette, France

[4] CEA Saclay, F-91191 Gif Sur Yvette, France

[5] NICPB, Tallinn, Estonia

[6] Helsinki Inst Phys, FI-00014 Helsinki, Finland

[7] Univ Pisa, Dipartimento Fis, Pisa, Italy

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2014年 / 03期

基金：

欧洲研究理事会;

关键词：

dark matter theory; ultra high energy photons and neutrinos; SOLAR; CAPTURE; OSCILLATIONS; WIMPS; EVAPORATION; SPECTRA;

D O I：

10.1088/1475-7516/2014/03/053

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We provide ingredients and recipes for computing neutrino signals of TeV-scale Dark Matter (DM) annihilations in the Sun. For each annihilation channel and DM mass we present the energy spectra of neutrinos at production, including: state-of-the-art energy losses of primary particles in solar matter, secondary neutrinos, electroweak radiation. We then present the spectra after propagation to the Earth, including (vacuum and matter) flavor oscillations and interactions in solar matter. We also provide a numerical computation of the capture rate of DM particles in the Sun. These results are available in numerical form.

引用

页数：26

共 62 条

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