TY - JOUR
T1 - Disentangling neutrino-nucleon cross section and high energy neutrino flux with a km3 neutrino telescope
AU - Borriello, E.
AU - Cuoco, A.
AU - Mangano, G.
AU - Miele, G.
AU - Pastor, S.
AU - Pisanti, O.
AU - Serpico, P. D.
PY - 2008/2/13
Y1 - 2008/2/13
N2 - The energy-zenith angular event distribution in a neutrino telescope provides a unique tool to determine at the same time the neutrino-nucleon cross section at extreme kinematical regions, and the high-energy neutrino flux. By using a simple parametrization for fluxes and cross sections, we present a sensitivity analysis for the case of a km3 neutrino telescope. In particular, we consider the specific case of an underwater Mediterranean telescope placed at the NEMO site, although most of our results also apply to an under-ice detector such as IceCube. We determine the sensitivity to departures from standard values of the cross sections above 1 PeV which can be probed independently from an a priori knowledge of the normalization and energy dependence of the flux. We also stress that the capability to tag downgoing neutrino showers in the PeV range against the cosmic-ray induced background of penetrating muons appears to be a crucial requirement to derive meaningful constraints on the cross section.
AB - The energy-zenith angular event distribution in a neutrino telescope provides a unique tool to determine at the same time the neutrino-nucleon cross section at extreme kinematical regions, and the high-energy neutrino flux. By using a simple parametrization for fluxes and cross sections, we present a sensitivity analysis for the case of a km3 neutrino telescope. In particular, we consider the specific case of an underwater Mediterranean telescope placed at the NEMO site, although most of our results also apply to an under-ice detector such as IceCube. We determine the sensitivity to departures from standard values of the cross sections above 1 PeV which can be probed independently from an a priori knowledge of the normalization and energy dependence of the flux. We also stress that the capability to tag downgoing neutrino showers in the PeV range against the cosmic-ray induced background of penetrating muons appears to be a crucial requirement to derive meaningful constraints on the cross section.
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U2 - 10.1103/PhysRevD.77.045019
DO - 10.1103/PhysRevD.77.045019
M3 - Article
AN - SCOPUS:41049094190
SN - 1550-7998
VL - 77
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 4
M1 - 045019
ER -