We examine the dependence of event rates at neutrino telescopes on the neutrino-nucleon cross section for neutrinos with energy above 1 PeV, and contrast the results with those for cosmic ray experiments. Scaling of the standard model cross sections leaves the rate of upward events essentially unchanged. Details, such as detector depth and cross section inelasticity, can influence rates. Numerical estimates of upward shower, muon, and tau event rates in the IceCube detector confirm these results
We evaluate neutrino-nucleon cross section for energies up to $10^{21} eV$ in light of new informati...
The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino en...
IceCube, a cubic kilometer neutrino telescope will be capable to probe neutrino-nucleon interactions...
We examine the dependence of event rates at neutrino telescopes on the neutrino-nucleon cross sectio...
One of the major goals of neutrino astronomy is to explore the otherwise unknown fluxes and interact...
The Standard Model neutrino-nucleon cross section at ultrahigh energies may be lower than was previo...
Extremely high energy neutrinos propagating in the atmosphere or in the Earth can originate horizont...
Now that PeV neutrinos have been discovered by IceCube, we optimistically entertain the possibility ...
AbstractNow that PeV neutrinos have been discovered by IceCube, we optimistically entertain the poss...
The IceCube Neutrino Observatory detects neutrinos at energies orders of magnitude higher than those...
Although they are best known for studying astrophysical neutrinos, neutrino telescopes like IceCube ...
Whether studying neutrinos for their own sake or as a messenger particle, neutrino cross sections ar...
The energy-zenith angular event distribution in a neutrino telescope provides a unique tool to deter...
The energy-zenith angular event distribution in a neutrino telescope provides a unique tool to deter...
Abstract: Cherenkov telescopes could have the capability of detecting high energy tau neutrinos by s...
We evaluate neutrino-nucleon cross section for energies up to $10^{21} eV$ in light of new informati...
The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino en...
IceCube, a cubic kilometer neutrino telescope will be capable to probe neutrino-nucleon interactions...
We examine the dependence of event rates at neutrino telescopes on the neutrino-nucleon cross sectio...
One of the major goals of neutrino astronomy is to explore the otherwise unknown fluxes and interact...
The Standard Model neutrino-nucleon cross section at ultrahigh energies may be lower than was previo...
Extremely high energy neutrinos propagating in the atmosphere or in the Earth can originate horizont...
Now that PeV neutrinos have been discovered by IceCube, we optimistically entertain the possibility ...
AbstractNow that PeV neutrinos have been discovered by IceCube, we optimistically entertain the poss...
The IceCube Neutrino Observatory detects neutrinos at energies orders of magnitude higher than those...
Although they are best known for studying astrophysical neutrinos, neutrino telescopes like IceCube ...
Whether studying neutrinos for their own sake or as a messenger particle, neutrino cross sections ar...
The energy-zenith angular event distribution in a neutrino telescope provides a unique tool to deter...
The energy-zenith angular event distribution in a neutrino telescope provides a unique tool to deter...
Abstract: Cherenkov telescopes could have the capability of detecting high energy tau neutrinos by s...
We evaluate neutrino-nucleon cross section for energies up to $10^{21} eV$ in light of new informati...
The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino en...
IceCube, a cubic kilometer neutrino telescope will be capable to probe neutrino-nucleon interactions...