A Lithium Experiment as the Stringent Test of the Theory of Stellar Evolution

dc.creatorKopylov, Anatoly
dc.creatorPetukhov, Valery
dc.date2003-01-04
dc.date2003-01-20
dc.date.accessioned2026-07-07T03:48:58Z
dc.date.available2026-07-07T03:48:58Z
dc.descriptionWe show that a lithium experiment has a potential to confirm or reject the value 1.5% of the solar luminosity attributed to a CNO-cycle by the SSM and to prove that the difference between total energy release of the Sun and what is produced in a hydrogen sequence is really produced in CNO cycle. This will be the stringent test of the theory of stellar evolution and the termination of the long-standing goal - the neutrino spectroscopy of the interior of the Sun. At the present time one can see no other way to solve this task, it can be accomplished only with a lithium detector utilizing its high sensitivity to CNO-neutrinos and very high accuracy in the theoretical evaluation of the cross-section of neutrino capture by 7Li. The analyses shows that although a lithium detector is a radiochemical one, principally it is possible to find separately the fluxes of 13N- and 15O-neutrinos.
dc.description8 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0301016
dc.identifierhttp://arxiv.org/abs/hep-ph/0301016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/42227
dc.subjectHigh Energy Physics - Phenomenology
dc.titleA Lithium Experiment as the Stringent Test of the Theory of Stellar Evolution
dc.typetext

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