Detection of Atmospheric Neutrinos and Relativistic Nuclear Structure Effects

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dc.creatorKim, H.
dc.creatorSchramm, S.
dc.creatorHorowitz, C. J.
dc.date1996-02-07
dc.date.accessioned2026-07-07T11:15:38Z
dc.date.available2026-07-07T11:15:38Z
dc.descriptionNeutrino-nucleus cross sections for the detection of atmospheric neutrinos are calculated in relativistic impulse and random phase approximations. Pion production is estimated via inclusive Delta-hole nuclear excitations. The number of pion events can confuse the identification of the neutrino flavor. As a further source of pions we calculate coherent pion production (where the nucleus remains in the ground state). We examine how these nuclear structure effects influence atmospheric neutrino experiments and study possible improvements in the present detector simulations.
dc.descriptionLaTeX file, 15 pages + 4 figures (postscript), submitted to Phys. Rev. C
dc.identifierhttps://arxiv.org/abs/nucl-th/9602009
dc.identifierhttp://arxiv.org/abs/nucl-th/9602009
dc.identifierPhys.Rev.C53:3131-3138,1996
dc.identifierdoi:10.1103/PhysRevC.53.3131
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/192450
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleDetection of Atmospheric Neutrinos and Relativistic Nuclear Structure Effects
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