scholarly journals Indirect dark matter searches at ultrahigh energy neutrino detectors

2021 ◽  
Vol 104 (8) ◽  
Author(s):  
Claire Guépin ◽  
Roberto Aloisio ◽  
Austin Cummings ◽  
Luis A. Anchordoqui ◽  
John F. Krizmanic ◽  
...  
2016 ◽  
Vol 2016 (12) ◽  
pp. 017-017 ◽  
Author(s):  
Ke Fang ◽  
Kumiko Kotera ◽  
M. Coleman Miller ◽  
Kohta Murase ◽  
Foteini Oikonomou

2003 ◽  
Vol 18 (22) ◽  
pp. 4085-4096 ◽  
Author(s):  
SHARADA IYER DUTTA ◽  
MARY HALL RENO ◽  
INA SARCEVIC

The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino energies up to 1012 GeV, Tests of neutrino oscillations (νμ ↔ ντ) from extragalactic sources of neutrinos are possible with large underground detectors. Measurements of horizontal air shower event rates at neutrino energies above 1010 GeV will be able to constrain nonstandard model contributions to the neutrino-nucleon cross section, e.g., from mini-black hole production.


2008 ◽  
Vol 77 (2) ◽  
Author(s):  
Sergio Palomares-Ruiz ◽  
Silvia Pascoli

1999 ◽  
Vol 11 (3) ◽  
pp. 327-334 ◽  
Author(s):  
M. Glück ◽  
S. Kretzer ◽  
E. Reya

2019 ◽  
Vol 222 ◽  
pp. 04002
Author(s):  
Vitaly Beylin ◽  
Maxim Bezuglov ◽  
Egor Tretiakov

In the framework of hypercolor extension of the Standard Model we consider cosmic rays scattering off hidden mass candidates. Specifically, there are two components of the Dark Matter in this model having close masses but different origin. As a result, neutrino production in the processes of scattering ofhigh energy electrons on these DM candidates is substantially different, and the secondary neutrino canbe seen, in principle, at neutrino detectors. We also note other interesting aspects of these type reactions.


Pramana ◽  
2012 ◽  
Vol 79 (5) ◽  
pp. 1331-1335 ◽  
Author(s):  
A K SOMA ◽  
L SINGH ◽  
M K SINGH ◽  
V SINGH ◽  
H T WONG

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