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dc.contributor.authorColoma, Pilar
dc.contributor.authorFernández Martínez, L. Enrique 
dc.contributor.otherUAM. Departamento de Física Teóricaes_ES
dc.date.accessioned2014-10-29T15:56:25Z
dc.date.available2014-10-29T15:56:25Z
dc.date.issued2012-04-18
dc.identifier.citationJournal of High Energy Physics 2012.4 (2012): 089en_US
dc.identifier.issn1126-6708 (print)es_ES
dc.identifier.issn1029-8479 (online)es_ES
dc.identifier.urihttp://hdl.handle.net/10486/662347
dc.descriptionJournal of High Energy Physics 2012.4 (2012): 089 reproduced by permission of Scuola Internazionale Superiore di Studi Avanzati (SISSA)en_US
dc.description.abstractUp to now, future neutrino beam experiments have been designed and optimized in order to look for CP violation, θ13 and the mass hierarchy under the conservative assumption that θ13 is very small. However, the recent results from T2K and MINOS favor a θ13 which could be as large as 8°. In this work, we propose a re-optimization for neutrino beam experiments in case this hint is confirmed. By switching from the first to the second oscillation peak, we find that the CP discovery potential of future oscillation experiments would not only be enhanced, but it would also be less affected by systematic uncertainties. In order to illustrate the effect, we present our results for a Super-Beam experiment, comparing the results obtained at the first and the second oscillation peaks for several values of the systematic errors. We also study its combination with a β-beam facility and show that the synergy between both experiments would also be enhanced due to the larger L/E. Moreover, the increased matter effects at the longer baseline also significantly improve the sensitivity to the mass hierarchyen_US
dc.description.sponsorshipWe acknowledge financial support from the European Community under the European Comission Framework Programme 7, Design Study: EUROnu, Project Number 212372. The EU is not liable for any use that may be made of the information contained herein. PC has been supported by Comunidad Autónoma de Madrid, and through projects FPA2009-09017 (DGI del MCyT, Spain) and HEPHACOS S2009/ESP-1473 (Comunidad Autónoma de Madrid), as well as from the Spanish Government under the Consolider-Ingenio 2010 programme CUP, Canfranc Underground Physics, project number CSD00C-08-44022en_US
dc.format.extent19es_ES
dc.format.mimetypeapplication/pdfen
dc.language.isoengen
dc.publisherSpringer Verlagen_US
dc.relation.ispartofJournal of High Energy Physicsen_US
dc.rights© SISSA 2012.en_US
dc.subject.otherCP violationes_ES
dc.subject.otherNeutrino physicses_ES
dc.subject.otherStandard modeles_ES
dc.titleOptimization of neutrino oscillation facilities for large θ13es_ES
dc.typearticlees_ES
dc.subject.ecienciaFísicaes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1007/JHEP04(2012)089es_ES
dc.identifier.doi10.1007/JHEP04(2012)089es_ES
dc.identifier.publicationfirstpage089es_ES
dc.identifier.publicationissue4es_ES
dc.identifier.publicationlastpage089es_ES
dc.identifier.publicationvolume2012es_ES
dc.relation.projectIDComunidad de Madrid. S2009/ESP-1473/HEPHACOSes_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/FP7/212372es_ES
dc.type.versioninfo:eu-repo/semantics/publishedVersionen
dc.rights.ccReconocimiento
dc.rights.accessRightsopenAccesses_ES
dc.facultadUAMFacultad de Ciencias


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