Probing the Temperature Profile of Energy Production in the Sun

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dc.creatorGrieb, Christian
dc.creatorRaghavan, R. S.
dc.date2006-09-04
dc.date.accessioned2026-07-07T10:25:23Z
dc.date.available2026-07-07T10:25:23Z
dc.descriptionThe particle kinetic energies of pp fusion in the sun (Gamow Energy) produce small changes in the energies of pp solar neutrinos relative to those due only to exothermal energetics. Observation of this effect may be possible via the unique tools of the upcoming LENS solar neutrino detector. The temperature profile of energy production in the sun may thus be directly probed for the first time.
dc.identifierhttps://arxiv.org/abs/hep-ph/0609030
dc.identifierhttp://arxiv.org/abs/hep-ph/0609030
dc.identifierPhys.Rev.Lett.98:141102,2007
dc.identifierdoi:10.1103/PhysRevLett.98.141102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176524
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleProbing the Temperature Profile of Energy Production in the Sun
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