NAGIOS: RODERIC FUNCIONANDO

Low-energy elastic neutrino-nucleon and nuclear scattering and its relevance for supernovae

Repositori DSpace/Manakin

dc.contributor.author	Bernabeu Alberola, José
dc.date.accessioned	2016-05-03T12:03:35Z
dc.date.available	2016-05-03T12:03:35Z
dc.date.issued	1976
dc.identifier.citation	Bernabeu Alberola, José (1976) Low-energy elastic neutrino-nucleon and nuclear scattering and its relevance for supernovae Astronomy and Astrophysics 47 3 375 379
dc.identifier.uri	http://hdl.handle.net/10550/53332
dc.description.abstract	Low-energy (E/sub v/10, spin- (if any) and isospin-dependent effects are comfortably below 10% of the coherent scattering. In the case of the neutron, the cross-section for momentum transfer, when compared to that of the isoscalar current, is: i) more than one order of magnitude larger in model I; ii) about twice larger in model II. It is noted that the vector model gives more dramatic effects in the supernova 'strategy' both lowering the cross-section in the inner core and increasing it in the outer region. (16 refs).
dc.language.iso	eng
dc.relation.ispartof	Astronomy and Astrophysics, 1976, vol. 47, num. 3, p. 375-379
dc.subject	Física
dc.title	Low-energy elastic neutrino-nucleon and nuclear scattering and its relevance for supernovae
dc.type	journal article	es_ES
dc.date.updated	2016-05-03T12:03:35Z
dc.identifier.idgrec	069111
dc.rights.accessRights	open access	es_ES