Add to ORKGSome solutions of the hierarchy problem of particle physics can lead to significantly increased neutrino cross sections beyond the electroweak scale. We discuss some consequences for and constraints resulting from cosmic ray physics
Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their concept...
We introduce neutrino astronomy starting from the observational fact that Nature accelerates protons...
The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino en...
New physics beyond the electroweak scale may increase weak interaction crosssections beyond the Stan...
AbstractTop–down models of cosmic rays produce more neutrinos than photons and more photons than pro...
A new strong-interaction has been postulated for neutrinos above ~10^{19} eV to explain the producti...
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...
Ultrahigh energy neutrinos can be used to explore the physics at the TeV scale. We study the neutrin...
After a short review of the ultrahigh energy cosmic ray puzzle - the apparent observation of cosmic ...
I give a brief discussion of possible sources of high energy neutrinos of astrophysical origin over ...
Ultrahigh energy cosmic neutrinos may reveal aspects of nature hidden to us so far. They probe the e...
The Standard Model neutrino-nucleon cross section at ultrahigh energies may be lower than was previo...
Scenarios in which the knee of the cosmic ray spectrum depends on the particle rigidities usually pr...
After a short review of the ultrahigh energy cosmic ray puzzle - the apparent observation of cosmic ...
Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their concept...
We introduce neutrino astronomy starting from the observational fact that Nature accelerates protons...
The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino en...
New physics beyond the electroweak scale may increase weak interaction crosssections beyond the Stan...
AbstractTop–down models of cosmic rays produce more neutrinos than photons and more photons than pro...
A new strong-interaction has been postulated for neutrinos above ~10^{19} eV to explain the producti...
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...
Ultrahigh energy neutrinos can be used to explore the physics at the TeV scale. We study the neutrin...
After a short review of the ultrahigh energy cosmic ray puzzle - the apparent observation of cosmic ...
I give a brief discussion of possible sources of high energy neutrinos of astrophysical origin over ...
Ultrahigh energy cosmic neutrinos may reveal aspects of nature hidden to us so far. They probe the e...
The Standard Model neutrino-nucleon cross section at ultrahigh energies may be lower than was previo...
Scenarios in which the knee of the cosmic ray spectrum depends on the particle rigidities usually pr...
After a short review of the ultrahigh energy cosmic ray puzzle - the apparent observation of cosmic ...
Although kilometer-scale neutrino detectors such as IceCube are discovery instruments, their concept...
We introduce neutrino astronomy starting from the observational fact that Nature accelerates protons...
The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino en...