Ultrahigh-energy neutrino emission from cosmic ray sources

1978 ◽  
Vol 222 ◽  
pp. 1109 ◽  
Author(s):  
D. Eichler
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.


2009 ◽  
Vol 79 (8) ◽  
Author(s):  
Xiao-Jun Bi ◽  
Zhen Cao ◽  
Ye Li ◽  
Qiang Yuan

2019 ◽  
Author(s):  
Kenji Yoshida ◽  
Maria Petropoulou ◽  
Meg Urry ◽  
Paolo Coppi ◽  
Charles Bailyn ◽  
...  

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

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