Dark matter and IceCube neutrinos

被引：2
作者：
Biondi, R. [1 ,2 ]
机构：
[1] Univ Aquila, Dipartimento Sci Fis & Chim, I-67100 Laquila, Italy
[2] Ist Nazl Fis Nucl, LNGS, I-67100 Assergi, AQ, Italy
来源：
NUOVO CIMENTO C-COLLOQUIA AND COMMUNICATIONS IN PHYSICS | 2015年 / 38卷 / 01期
关键词：
D O I：
10.1393/ncc/i2015-15031-4
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We show that the excess of high energy neutrinos observed by the IceCube collaboration at energies above 100 TeV might originate from baryon number violating decays of heavy shadow baryons from mirror sector, which in turn constitute Dark Matter. Due to tiny mixing between mirror and ordinary neutrinos, it is possible to explain the specific features of the IceCube events spectrum.
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页数：5
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