Dark Matter Annihilation to Neutrinos: Current Limits and Future Prospects

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作者
Arguelles, Carlos A. [1 ]
Diaz, Alejandro [2 ,3 ]
Kheirandish, Ali [4 ,5 ]
Safa, Ibrahim [1 ,6 ,7 ]
Vincent, Aaron C. [8 ,9 ,10 ]
机构
[1] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[2] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA
[3] MIT, Dept Phys, Cambridge, MA 02139 USA
[4] Penn State Univ, Dept Phys, University Pk, PA 16802 USA
[5] Penn State Univ, Ctr Multimessenger Astrophys, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
[6] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[7] Univ Wisconsin, Wisconsin IceCube Particle Astrophys Ctr, Madison, WI 53706 USA
[8] Queens Univ, Dept Phys Engn Phys Astron, Kingston, ON K7L 3N6, Canada
[9] Arthur B McDonald Canadian Astroparticle Phys Res, Kingston, ON K7L 3N6, Canada
[10] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
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P1 [天文学];
学科分类号
0704 ;
摘要
Neutrinos can escape dense environments, otherwise opaque to photons, and travel cosmic distances unscathed by background radiation or magnetic fields. While ideal cosmic messengers, they present a unique opportunity to test physics beyond the Standard Model, especially dark matter. Moreover, there is a distinct possibility that the neutrino sector is the principal portal through which the dark matter interacts with the Standard Model. In this talk, we will discuss new opportunities offered by high-energy neutrinos and provide new model-independent limits on dark matter annihilation into neutrinos based on measurements of neutrinos. We present the most up-to-date and comprehensive results on dark matter annihilation into neutrinos using the most recently available data from neutrino telescopes, with measurements spanning a wide energy range. Finally, we will present the projections for next-generation of neutrino experiments.
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页数:8
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