Mostra el registre parcial de l'element
dc.contributor.author | Alberico, Wanda Maria | |
dc.contributor.author | Bernabeu Alberola, José | |
dc.contributor.author | Bilenky, Samoil M. | |
dc.contributor.author | Grimus, Walter | |
dc.date.accessioned | 2016-05-03T11:25:52Z | |
dc.date.available | 2016-05-03T11:25:52Z | |
dc.date.issued | 2000 | |
dc.identifier.citation | Alberico, Wanda Maria; Bernabeu Alberola, José; Bilenky, Samoil M.; Grimus, Walter (2000) Is it possible to determine the S-factor of the hep process from a laboratory experiment? Physics Letters B 478 1-3 208 214 | |
dc.identifier.uri | http://hdl.handle.net/10550/53315 | |
dc.description.abstract | We discuss the problem of solar hep neutrinos originating from the reaction p + 3He -> 4He + e+ + nu and obtain a relation between the astrophysical S-factor of the hep process and the cross section of the process e- + 4He -> 3H + n + nu near threshold. The relation is based on the isotopic invariance of strong interactions. The measurement of the latter cross section would allow to obtain experimental information on S(hep), the value of which, at the moment, is known only from theoretical calculations. | |
dc.language.iso | eng | |
dc.relation.ispartof | Physics Letters B, 2000, vol. 478, num. 1-3, p. 208-214 | |
dc.subject | Física | |
dc.title | Is it possible to determine the S-factor of the hep process from a laboratory experiment? | |
dc.type | journal article | es_ES |
dc.date.updated | 2016-05-03T11:25:52Z | |
dc.identifier.doi | 10.1016/S0370-2693(00)00287-2 | |
dc.identifier.idgrec | 069017 | |
dc.rights.accessRights | open access | es_ES |