Add to ORKGA suppression in the spectrum of ultrahigh-energy (UHE, {ge} 10{sup 18} eV) neutrinos will be present in extra-dimensional scenarios, due to enhanced neutrino-antineutrino annihilation processes with the supernova relic neutrinos. In this scenario, neutrinos can not be responsible for the highest energy events observed in the UHE cosmic ray spectrum. A direct implication of these extra-dimensional interactions would be the absence of UHE neutrinos in ongoing and future neutrino telescopes
International audienceFast-spinning newborn pulsars are intriguing candidate sources of ultrahigh-en...
Neutrinos with energies above 10¹⁷ eV are detectable with the Surface Detector Array of the Pierre A...
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With ...
A suppression in the spectrum of ultrahigh-energy (UHE, greater than or similar to 10(18) eV) neutri...
Recent measurements of the spectrum and composition of ultrahigh energy cosmic rays suggest that the...
Proceedings of the 3rd International Workshop on a Very Large Volume Neutrino Telescope for the Medi...
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the injection sp...
Observation of Ultra High Energy Cosmic Rays (UHECR) -whose energy exceeds $10^20$eV- is still a puz...
UHE neutrinos may transfer highest cosmic-rays energies overcoming $2.75K^\circ$ BBR and radio-waves...
International audienceThe observation of neutrinos from cosmic accelerators will be revolutionary. H...
We show the results and discussions of the study of a possible suppression of the extragalactic neut...
We discuss the prospect of observing high energy neutrinos from the annihilation or decay of superhe...
Applying our recently developed propagation code we review extragalactic neutrino fluxes above 10^{1...
We outline the current situation in ultrahigh energy (UHE) cosmic ray physics, pointing out the rema...
Neutrinos are the best candidates to test the extreme Universe and ideas beyond the Standard Model o...
International audienceFast-spinning newborn pulsars are intriguing candidate sources of ultrahigh-en...
Neutrinos with energies above 10¹⁷ eV are detectable with the Surface Detector Array of the Pierre A...
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With ...
A suppression in the spectrum of ultrahigh-energy (UHE, greater than or similar to 10(18) eV) neutri...
Recent measurements of the spectrum and composition of ultrahigh energy cosmic rays suggest that the...
Proceedings of the 3rd International Workshop on a Very Large Volume Neutrino Telescope for the Medi...
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the injection sp...
Observation of Ultra High Energy Cosmic Rays (UHECR) -whose energy exceeds $10^20$eV- is still a puz...
UHE neutrinos may transfer highest cosmic-rays energies overcoming $2.75K^\circ$ BBR and radio-waves...
International audienceThe observation of neutrinos from cosmic accelerators will be revolutionary. H...
We show the results and discussions of the study of a possible suppression of the extragalactic neut...
We discuss the prospect of observing high energy neutrinos from the annihilation or decay of superhe...
Applying our recently developed propagation code we review extragalactic neutrino fluxes above 10^{1...
We outline the current situation in ultrahigh energy (UHE) cosmic ray physics, pointing out the rema...
Neutrinos are the best candidates to test the extreme Universe and ideas beyond the Standard Model o...
International audienceFast-spinning newborn pulsars are intriguing candidate sources of ultrahigh-en...
Neutrinos with energies above 10¹⁷ eV are detectable with the Surface Detector Array of the Pierre A...
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With ...