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Ultra-high energy extragalactic neutrinos interacting with ultra-light dark matter
(2012-11-01)
We show the results and discussions of the study of a possible suppression of the extragalactic neutrino flux during its propagation due to a nonstandard interaction with a candidate field to dark matter. In particular, ...
Ultra-high energy extragalactic neutrinos interacting with ultra-light dark matter
(2012-11-01)
We show the results and discussions of the study of a possible suppression of the extragalactic neutrino flux during its propagation due to a nonstandard interaction with a candidate field to dark matter. In particular, ...
Confusing the extragalactic neutrino flux limit with a neutrino propagation limit
(Iop Publishing Ltd, 2011-10-01)
We study the possible suppression of the extragalactic neutrino flux due to a nonstandard interaction during its propagation. In particular, we study neutrino interaction with an ultra-light scalar field dark matter. It ...
Confusing the extragalactic neutrino flux limit with a neutrino propagation limit
(Iop Publishing Ltd, 2011-10-01)
We study the possible suppression of the extragalactic neutrino flux due to a nonstandard interaction during its propagation. In particular, we study neutrino interaction with an ultra-light scalar field dark matter. It ...
Confusing the extragalactic neutrino flux limit with a neutrino propagation limit
(Iop Publishing Ltd, 2013)
On the energy of the protons producing the very high-energy astrophysical neutrinos
(IOP Publishing, 2021-03)
We study the distribution of the energy of the protons that can produce an astrophysical neutrino with a given observed energy, in the TeV-PeV range, both through pp or pγ interactions. Due to the increasing multiplicity ...
Implications of the pseudo-Dirac scenario for ultra high energy neutrinos from GRBs
(Iop Publishing LtdBristolInglaterra, 2012)
On the relation between the astrophysical neutrino fluxes and the cosmic ray fluxes
(IOP Publishing, 2021-08)
Some generalizations of the relation between high-energy astrophysical neutrino and cosmic ray fluxes are obtained, taking into account present results on the cosmic ray spectrum and composition as well as a more realistic ...