8Li electron spectrum versus 8B neutrino spectrum: implications for the Sudbury Neutrino Observatory

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dc.creatorJonkmans, G.
dc.creatorTowner, I. S.
dc.creatorSur, B.
dc.date1998-02-25
dc.date.accessioned2026-07-07T11:11:35Z
dc.date.available2026-07-07T11:11:35Z
dc.descriptionThe sensitivity of the Sudbury Neutrino Observatory (SNO) to measure the shape of the recoil electron spectrum in the charged-current reaction of $^{8}$B solar neutrinos interacting with deuterium can be improved if the results of a $^{8}$Li beta-decay calibration experiment are included in the test. We calculate an improvement in sensitivity, under certain idealistic assumptions, of about a factor of 2, sufficient to resolve different neutrino-oscillation solutions to the solar-neutrino problem. We further examine the role of recoil and radiative corrections on both the $^{8}$B neutrino spectrum and the $^{8}$Li electron spectrum and conclude that the influence of these effects on the ratio of the two spectra as measured by SNO is very small.
dc.descriptionrevtex
dc.identifierhttps://arxiv.org/abs/nucl-th/9802078
dc.identifierhttp://arxiv.org/abs/nucl-th/9802078
dc.identifierPhys.Rev.C58:1278-1287,1998
dc.identifierdoi:10.1103/PhysRevC.58.1278
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191143
dc.subjectNuclear Theory
dc.title8Li electron spectrum versus 8B neutrino spectrum: implications for the Sudbury Neutrino Observatory
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