Add to ORKGWe constrain high-energy neutrino fluxes with the observed cosmic ray and gamma ray fluxes, include flavor oscillations and propagation through Earth, and show that blazars could possibly be detected by cubic-kilometer neutrino telescopes
Some solutions of the hierarchy problem of particle physics can lead to significantly increased neut...
Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre A...
Using the most recent cosmic ray spectra up to 2x10 to the 20th power eV, production spectra of high...
In order to facilitate the identification of possible new physics signatures in neutrino telescopes,...
Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their concept...
We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Trans...
AbstractTop–down models of cosmic rays produce more neutrinos than photons and more photons than pro...
We introduce neutrino astronomy starting from the observational fact that Nature accelerates protons...
Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their concept...
Several cosmologically distant astrophysical sources may produce ultra-high energy cosmic neutrinos ...
Since 2010 IceCube observed around 50 high-energy neutrino events of cosmic origin above 60 TeV, but...
Ongoing experimental efforts to detect cosmic sources of high energy neutrinos are guided by the exp...
Recent results from high-energy cosmic ray and gamma detectors indicate the occurrence of hadron acc...
This is a (very) personal attempt to summarize the status of neutrino astronomy: its scientific moti...
IceCube has detected a cumulative flux of PeV neutrinos, which origin is unknown. Blazars, active ga...
Some solutions of the hierarchy problem of particle physics can lead to significantly increased neut...
Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre A...
Using the most recent cosmic ray spectra up to 2x10 to the 20th power eV, production spectra of high...
In order to facilitate the identification of possible new physics signatures in neutrino telescopes,...
Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their concept...
We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Trans...
AbstractTop–down models of cosmic rays produce more neutrinos than photons and more photons than pro...
We introduce neutrino astronomy starting from the observational fact that Nature accelerates protons...
Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their concept...
Several cosmologically distant astrophysical sources may produce ultra-high energy cosmic neutrinos ...
Since 2010 IceCube observed around 50 high-energy neutrino events of cosmic origin above 60 TeV, but...
Ongoing experimental efforts to detect cosmic sources of high energy neutrinos are guided by the exp...
Recent results from high-energy cosmic ray and gamma detectors indicate the occurrence of hadron acc...
This is a (very) personal attempt to summarize the status of neutrino astronomy: its scientific moti...
IceCube has detected a cumulative flux of PeV neutrinos, which origin is unknown. Blazars, active ga...
Some solutions of the hierarchy problem of particle physics can lead to significantly increased neut...
Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre A...
Using the most recent cosmic ray spectra up to 2x10 to the 20th power eV, production spectra of high...