scholarly journals Quantifying uncertainties in the high-energy neutrino cross-section

Pramana ◽  
2012 ◽  
Vol 79 (5) ◽  
pp. 1301-1308 ◽  
Author(s):  
A COOPER-SARKAR ◽  
P MERTSCH ◽  
S SARKAR
Keyword(s):  
Cross Section ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Neutrino Cross Section

scholarly journals Measurement ofK+production cross section by 8 GeV protons using high-energy neutrino interactions in the SciBooNE detector

2011 ◽  
Vol 84 (1) ◽  
Author(s):  
G. Cheng ◽  
C. Mariani ◽  
J. L. Alcaraz-Aunion ◽  
S. J. Brice ◽  
L. Bugel ◽  
...  
Keyword(s):  
Cross Section ◽  
Production Cross Section ◽  
Production Cross ◽  
High Energy ◽  
High Energy Neutrino ◽  
Neutrino Interactions ◽  
Energy Neutrino

scholarly journals Disentangling neutrino-nucleon cross section and high energy neutrino flux with akm3neutrino telescope

2008 ◽  
Vol 77 (4) ◽  
Author(s):  
E. Borriello ◽  
A. Cuoco ◽  
G. Mangano ◽  
G. Miele ◽  
S. Pastor ◽  
...  
Keyword(s):  
Cross Section ◽  
Neutrino Flux ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino

scholarly journals High-energy neutrino-nucleus interactions

2019 ◽  
Vol 208 ◽  
pp. 07003
Author(s):  
Shunzo Kumano
Keyword(s):  
Neutrino Physics ◽  
Cross Section ◽  
Neutrino Oscillation ◽  
High Energy ◽  
Neutrino Beam ◽  
Current Status ◽  
Ultra High Energy ◽  
High Energy Neutrino ◽  
Neutrino Interactions ◽  
Energy Neutrino

High-energy neutrino-nucleus interactions are discussed by considering neutrino-oscillation experiments and ultra-high-energy cosmic neutrino interactions. The largest systematic error for the current neutrino oscillation measurements comes from the neutrino-nucleus interaction part, and its accurate understanding is essential for high-precision neutrino physics, namely for studying CP violation in the lepton sector. Depending on neutrino beam energies, quasi-elastic, resonance, Regge, or/and deep inelastic scattering (DIS) processes contribute to the neutrino cross section. It is desirable to have a code to calculate the neutrino-nucleus cross section in any kinematical range by combining various theoretical descriptions. On the other hand, the IceCube collaboration started obtaining cross section data up to the 1015 eV range, so that it became necessary to understand ultra-high-energy neutrino interactions beyond the artificial lepton-accelerator energy range. For future precise neutrino physics including the CP measurement, it is also necessary to understand accurate nuclear corrections. The current status is explained for nuclear corrections in DIS structure functions. The possibility is also discussed to find gravitational sources within nucleons and nuclei, namely matrix elements of quark-gluon energy-momentum tensor. They could be probed by neutrino interactions without replying on direct ultra-weak “gravitational interactions” with high-intensity neutrino beams, possibly at a future neutrino factory, by using techniques of hadron tomography.

High energy neutrino scattering at low Q2: Strong or weak PCAC?

1973 ◽  
Vol 64 ◽  
pp. 253-268
Author(s):  
M. De Vincenzi ◽  
G. Preparata
Keyword(s):  
High Energy ◽  
High Energy Neutrino ◽  
Neutrino Scattering ◽  
Energy Neutrino
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