NAGIOS: RODERIC FUNCIONANDO

Bounds on very low reheating scenarios after Planck

Repositori DSpace/Manakin

Valencià Castellano

Inici
Investigació
e-prints
22 - Física
Visualitza element

IMPORTANT: Aquest repositori està en una versió antiga des del 3/12/2023. La nova instal.lació está en https://roderic.uv.es/

Bounds on very low reheating scenarios after Planck

Mostra el registre parcial de l'element

dc.contributor.author	Fernández de Salas, Pablo
dc.contributor.author	Lattanzi, Massimiliano
dc.contributor.author	Mangano, Gianpiero
dc.contributor.author	Miele, Gennaro
dc.contributor.author	Pastor Carpi, Sergio
dc.contributor.author	Pisanti, Ofelia
dc.date.accessioned	2016-04-18T12:36:14Z
dc.date.available	2016-04-18T12:36:14Z
dc.date.issued	2015
dc.identifier.citation	Fernández de Salas, Pablo Lattanzi, Massimiliano Mangano, Gianpiero Miele, Gennaro Pastor Carpi, Sergio Pisanti, Ofelia 2015 Bounds on very low reheating scenarios after Planck Physical Review D 92 123534-1 123534-9
dc.identifier.uri	http://hdl.handle.net/10550/52787
dc.description.abstract	We consider the case of very low reheating scenarios (TRH∼(MeV)) with a better calculation of the production of the relic neutrino background (with three-flavor oscillations). At 95% confidence level, a lower bound on the reheating temperature TRH>4.1 MeV is obtained from Big Bang Nucleosynthesis, while TRH>4.3 MeV from Planck data for very light (∑mi=0.06 eV) neutrinos. If neutrino masses are allowed to vary, Planck data yield TRH>4.7 MeV, the most stringent bound on the reheating temperature to date. Neutrino masses as large as 1 eV are possible for very low reheating temperatures
dc.language.iso	eng
dc.relation.ispartof	Physical Review D, 2015, vol. 92, p. 123534-1-123534-9
dc.subject	Física
dc.title	Bounds on very low reheating scenarios after Planck
dc.type	journal article	es_ES
dc.date.updated	2016-04-18T12:36:15Z
dc.identifier.doi	10.1103/PhysRevD.92.123534
dc.identifier.idgrec	109171
dc.rights.accessRights	open access	es_ES