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Neutrino oscillations refitted
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| dc.contributor.author | Vanegas Forero, David | |
| dc.contributor.author | Tórtola Baixauli, María Amparo | |
| dc.contributor.author | Furtado Valle, José Wagner | |
| dc.date.accessioned | 2016-04-22T12:31:19Z | |
| dc.date.available | 2016-04-22T12:31:19Z | |
| dc.date.issued | 2014 | |
| dc.identifier.citation | Vanegas Forero, David Tórtola Baixauli, María Amparo Furtado Valle, José Wagner 2014 Neutrino oscillations refitted Physical Review D 90 9 093006 | |
| dc.identifier.uri | http://hdl.handle.net/10550/53011 | |
| dc.description.abstract | Here, we update our previous global fit of neutrino oscillations by including the recent results that have appeared since the Neutrino 2012 conference. These include the measurements of reactor antineutrino disappearance reported by Daya Bay and RENO, together with latest T2K and MINOS data including both disappearance and appearance channels. We also include the revised results from the third solar phase of Super-Kamiokande, SK-III, as well as new solar results from the fourth phase of Super-Kamiokande, SK-IV. We find that the preferred global determination of the atmospheric angle theta(23) is consistent with maximal mixing. We also determine the impact of the new data upon all the other neutrino oscillation parameters with an emphasis on the increasing sensitivity to the CP phase, thanks to the interplay between accelerator and reactor data. In the Appendix, we present the updated results obtained after the inclusion of new reactor data presented at the Neutrino 2014 conference. We discuss their impact on the global neutrino analysis. | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Physical Review D, 2014, vol. 90, num. 9, p. 093006 | |
| dc.subject | Física | |
| dc.title | Neutrino oscillations refitted | |
| dc.type | journal article | es_ES |
| dc.date.updated | 2016-04-22T12:31:19Z | |
| dc.identifier.doi | 10.1103/PhysRevD.90.093006 | |
| dc.identifier.idgrec | 101046 | |
| dc.rights.accessRights | open access | es_ES |
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