Astronomy with energy dependent flavour ratios of extragalactic neutrinos

被引：7
作者：
Karmakar, Siddhartha [1 ]
Pandey, Sujata [1 ]
Rakshit, Subhendu [1 ]
机构：
[1] Indian Inst Technol Indore, Discipline Phys, Khandwa Rd, Indore 453552, India
来源：
JOURNAL OF HIGH ENERGY PHYSICS | 2021年 / 2021卷 / 10期
关键词：
Beyond Standard Model; Neutrino Physics; COLD DARK-MATTER; OSCILLATIONS; GALAXIES; MODELS; HALO;
D O I：
10.1007/JHEP10(2021)004
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
High energy astrophysical neutrinos interacting with ultralight dark matter (DM) can undergo flavour oscillations that induce an energy dependence in the flavour ratios. Such a dependence on the neutrino energy will reflect in the track to shower ratio in neutrino telescopes like IceCube or KM3NeT. This opens up a possibility to study DM density profiles of astrophysical objects like AGN, GRB etc., which are the suspected sources of such neutrinos.
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收藏
页数：22
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