Mass limits for dark-matter particles derived from high-energy neutrinos from the Sun

1991 ◽  
Vol 44 (8) ◽  
pp. 2220-2240 ◽  
Author(s):  
N. Sato ◽  
K. S. Hirata ◽  
T. Kajita ◽  
T. Kifune ◽  
K. Kihara ◽  
...  
Keyword(s):  
Dark Matter ◽  
High Energy ◽  
The Sun ◽  
High Energy Neutrinos

High-energy neutrinos from the sun and cold dark matter

1987 ◽  
Vol 279 (3-4) ◽  
pp. 804-823 ◽  
Author(s):  
Mark Srednicki ◽  
Keith A. Olive ◽  
Joseph Silk
Keyword(s):  
Dark Matter ◽  
Cold Dark Matter ◽  
High Energy ◽  
The Sun ◽  
High Energy Neutrinos

scholarly journals Indirect search for neutralino dark matter with high energy neutrinos

2002 ◽  
Vol 65 (7) ◽  
Author(s):  
V. Barger ◽  
Francis Halzen ◽  
Dan Hooper ◽  
Chung Kao
Keyword(s):  
Dark Matter ◽  
High Energy ◽  
High Energy Neutrinos

scholarly journals High energy neutrinos from superheavy dark matter annihilation

2001 ◽  
Vol 64 (8) ◽  
Author(s):  
Ivone F. M. Albuquerque ◽  
Lam Hui ◽  
Edward W. Kolb
Keyword(s):  
Dark Matter ◽  
High Energy ◽  
Dark Matter Annihilation ◽  
High Energy Neutrinos ◽  
Superheavy Dark Matter

High-energy neutrinos from WIMP annihilations in the Sun

2010 ◽  
pp. 507-520
Author(s):  
F. Halzen ◽  
D. Hooper
Keyword(s):  
High Energy ◽  
The Sun ◽  
High Energy Neutrinos

scholarly journals Propagation of high-energy neutrinos in a background of ultralight scalar dark matter

2016 ◽  
Vol 82 ◽  
pp. 10-20 ◽  
Author(s):  
Matías M. Reynoso ◽  
Oscar A. Sampayo
Keyword(s):  
Dark Matter ◽  
High Energy ◽  
High Energy Neutrinos

scholarly journals Estimation of baryon asymmetry from dark matter decaying into IceCube neutrinos

2021 ◽  
pp. 2150078
Author(s):  
Tista Mukherjee ◽  
Madhurima Pandey ◽  
Debasish Majumdar ◽  
Ashadul Halder
Keyword(s):  
Dark Matter ◽  
Early Universe ◽  
Power Law ◽  
Lower Energy ◽  
High Energy ◽  
Baryon Asymmetry ◽  
The Other ◽  
Astrophysical Source ◽  
High Energy Neutrinos ◽  
The Universe

The recent results of IceCube Neutrino Observatory include an excess of PeV neutrino events which appear to follow a broken power-law different from the other lower energy neutrinos detected by IceCube. The possible astrophysical source of these neutrinos is still unknown. One possible source of such neutrinos could be the decay of nonthermal, long-lived heavy mass dark matter, whose mass should be [Formula: see text] GeV and could have produced at the very early Universe. They can undergo cascading decay via both hadronic and leptonic channels to finally produce such high energy neutrinos. This possibility has been explored in this work by studying the decay flux of these dark matter candidates. The mass and lifetime of such dark matter particles have been obtained by performing a [Formula: see text] fit with the PeV neutrino data of IceCube. We finally estimate the baryon asymmetry produced in the Universe due to such dark matter decay.

scholarly journals High Energy Neutrinos from Dark Matter Decay

2017 ◽  
Author(s):  
Zurab Berezhiani ◽  
Riccardo Biondi ◽  
Askhat Gazizov
Keyword(s):  
Dark Matter ◽  
High Energy ◽  
High Energy Neutrinos
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