Mostra el registre parcial de l'element
dc.contributor.author | Coughlan, G. D. | |
dc.contributor.author | Ross, Graham G. | |
dc.contributor.author | Holman, Richard | |
dc.contributor.author | Ramond, Pierre | |
dc.contributor.author | Ruiz-Altaba, Martí | |
dc.contributor.author | Furtado Valle, José Wagner | |
dc.date.accessioned | 2015-09-24T10:24:53Z | |
dc.date.available | 2015-09-24T10:24:53Z | |
dc.date.issued | 1985 | |
dc.identifier.citation | Coughlan, G. D. Ross, Graham G. Holman, Richard Ramond, Pierre Ruiz-Altaba, Martí Furtado Valle, José Wagner 1985 Baryogenesis in supergravity inflationary models Physics Letters B 160 4-5 249 255 | |
dc.identifier.uri | http://hdl.handle.net/10550/47208 | |
dc.description.abstract | Realistic N=1 supergravity theories with a gravitino mass of order 1 TeV require a period of inflation to dilute the gravitino abundance. Moreover, if the gravitino is unstable the reheat temperature is bounded to be no greater than O(108 GeV). We show that such models may still have acceptable rates of baryosynthesis and discuss possible mechanisms. | |
dc.language.iso | eng | |
dc.relation.ispartof | Physics Letters B, 1985, vol. 160, num. 4-5, p. 249-255 | |
dc.subject | Física | |
dc.title | Baryogenesis in supergravity inflationary models | |
dc.type | journal article | es_ES |
dc.date.updated | 2015-09-24T10:24:54Z | |
dc.identifier.doi | 10.1016/0370-2693(85)91320-6 | |
dc.identifier.idgrec | 073620 | |
dc.rights.accessRights | open access | es_ES |