Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/85257
Full metadata record
DC FieldValueLanguage
dc.contributor.CRUESPUNIVERSIDADE DE ESTADUAL DE CAMPINASpt_BR
dc.identifier.isbnpt
dc.typeArtigo de periódicopt_BR
dc.titleNon-unitary Neutrino Propagation From Neutrino Decaypt_BR
dc.contributor.authorBerryman J.M.pt_BR
dc.contributor.authorde Gouvea A.pt_BR
dc.contributor.authorHernandez D.pt_BR
dc.contributor.authorOliveira R.L.N.pt_BR
unicamp.authorOliveira, R.L.N., Northwestern University, Department of Physics and Astronomy, 2145 Sheridan RoadEvanston, IL, United States, Instituto de Física Gleb Wataghin Universidade Estadual de Campinas, UNICAMP 13083-970Campinas, São Paulo, Brazilpt_BR
unicamp.author.externalBerryman, J.M., Northwestern University, Department of Physics and Astronomy, 2145 Sheridan RoadEvanston, IL, United Statespt
unicamp.author.externalde Gouvêa, A., Northwestern University, Department of Physics and Astronomy, 2145 Sheridan RoadEvanston, IL, United Statespt
unicamp.author.externalHernández, D., Northwestern University, Department of Physics and Astronomy, 2145 Sheridan RoadEvanston, IL, United Statespt
dc.description.abstractNeutrino propagation in space-time is not constrained to be unitary if very light states - lighter than the active neutrinos - exist into which neutrinos may decay. If this is the case, neutrino flavor-change is governed by a handful of extra mixing and "oscillation" parameters, including new sources of CP-invariance violation. We compute the transition probabilities in the two- and three-flavor scenarios and discuss the different phenomenological consequences of the new physics. These are qualitatively different from other sources of unitarity violation discussed in the literature.en
dc.relation.ispartofPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physicspt_BR
dc.publisherElsevierpt_BR
dc.date.issued2015pt_BR
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle And High-energy Physics. Elsevier, v. 742, n. , p. 74 - 79, 2015.pt_BR
dc.language.isoenpt_BR
dc.description.volume742pt_BR
dc.description.issuenumberpt_BR
dc.description.initialpage74pt_BR
dc.description.lastpage79pt_BR
dc.rightsabertopt_BR
dc.sourceScopuspt_BR
dc.identifier.issn3702693pt_BR
dc.identifier.doi10.1016/j.physletb.2015.01.002pt_BR
dc.identifier.urlhttp://www.scopus.com/inward/record.url?eid=2-s2.0-84921447035&partnerID=40&md5=6a065624d5476de5f4ea3c3d2844179bpt_BR
dc.date.available2015-06-25T12:51:30Z
dc.date.available2015-11-26T15:01:46Z-
dc.date.accessioned2015-06-25T12:51:30Z
dc.date.accessioned2015-11-26T15:01:46Z-
dc.description.provenanceMade available in DSpace on 2015-06-25T12:51:30Z (GMT). No. of bitstreams: 1 2-s2.0-84921447035.pdf: 298802 bytes, checksum: 8e5a422f21674d45d933a818131ed366 (MD5) Previous issue date: 2015en
dc.description.provenanceMade available in DSpace on 2015-11-26T15:01:46Z (GMT). No. of bitstreams: 2 2-s2.0-84921447035.pdf: 298802 bytes, checksum: 8e5a422f21674d45d933a818131ed366 (MD5) 2-s2.0-84921447035.pdf.txt: 31993 bytes, checksum: 374e633d38728468ccff3dba9a6723f0 (MD5) Previous issue date: 2015en
dc.identifier.urihttp://www.repositorio.unicamp.br/handle/REPOSIP/85257
dc.identifier.urihttp://repositorio.unicamp.br/jspui/handle/REPOSIP/85257-
dc.identifier.idScopus2-s2.0-84921447035pt_BR
dc.description.referenceWolfenstein, L., (1978) Phys. Rev. D, 17, p. 2369pt_BR
dc.description.referenceLee, B.W., Pakvasa, S., Shrock, R.E., Sugawara, H., (1977) Phys. Rev. Lett., 38, p. 937pt_BR
dc.description.referenceLee, B.W., Pakvasa, S., Shrock, R.E., Sugawara, H., (1977) Phys. Rev. Lett., 38, p. 1230. , (Erratum)pt_BR
dc.description.referenceLee, B.W., Shrock, R.E., (1977) Phys. Rev. D, 16, p. 1444pt_BR
dc.description.referenceAppelquist, T., Piai, M., Shrock, R., (2004) Phys. Rev. D, 69, p. 015002. , arxiv:hep-ph/0308061pt_BR
dc.description.referenceAntusch, S., Biggio, C., Fernandez-Martinez, E., Gavela, M.B., Lopez-Pavon, J., (2006) J. High Energy Phys., 610, p. 084. , arxiv:hep-ph/0607020pt_BR
dc.description.referencede Gouvêa, A., arxiv:1310.4340, For a recent overview see, for example, Intensity Frontier Neutrino Working Group CollaborationIntensity Frontier Neutrino Working Group CollaborationKostelecky, V.A., Mewes, M., (2004) Phys. Rev. D, 69, p. 016005. , arxiv:hep-ph/0309025, See, for examplept_BR
dc.description.referenceKostelecky, V.A., Mewes, M., (2004) Phys. Rev. D, 70, p. 031902. , arxiv:hep-ph/0308300pt_BR
dc.description.referenceMurayama, H., Yanagida, T., (2001) Phys. Lett. B, 520, p. 263. , arxiv:hep-ph/0010178pt_BR
dc.description.referenceLisi, E., Marrone, A., Montanino, D., (2000) Phys. Rev. Lett., 85, p. 1166pt_BR
dc.description.referenceBenatti, F., Floreanini, R., (2000) J. High Energy Phys., 2, p. 32pt_BR
dc.description.referenceBranco, G.C., Lavoura, L., Silva, J.P., (1999) CP Violation, , Oxford University Presspt_BR
dc.description.referenceBigi, I.I., Sanda, A.I., (2000) CP Violation, , Cambridge University Presspt_BR
dc.description.referencePilaftsis, A., (1997) Phys. Rev. D, 56, p. 5431. , arxiv:hep-ph/9707235pt_BR
dc.description.referenceKabir, P.K., (1968) The CP Puzzle, Strange Decays of the Neutral Kaon, , Academic Presspt_BR
dc.description.referenceStodolsky, L., (1970) Phys. Rev. D, 1, p. 2683pt_BR
dc.description.referenceFrieman, J.A., Haber, H.E., Freese, K., (1988) Phys. Lett. B, 200, p. 115pt_BR
dc.description.referenceBarger, V.D., Learned, J.G., Pakvasa, S., Weiler, T.J., (1999) Phys. Rev. Lett., 82, p. 2640. , arxiv:astro-ph/9810121pt_BR
dc.description.referenceLindner, M., Ohlsson, T., Winter, W., (2001) Nucl. Phys. B, 607, p. 326. , arxiv:hep-ph/0103170pt_BR
dc.description.referenceBerryman, J.M., in preparationBeacom, J.F., Bell, N.F., Dodelson, S., (2004) Phys. Rev. Lett., 93, p. 121302. , arxiv:astro-ph/0404585pt_BR
dc.description.referenceHannestad, S., Raffelt, G., (2005) Phys. Rev. D, 72, p. 103514. , arxiv:hep-ph/0509278pt_BR
dc.description.referenceSerpico, P.D., (2007) Phys. Rev. Lett., 98, p. 171301. , arxiv:astro-ph/0701699pt_BR
dc.description.referenceAartsen, M.G., (2013) Phys. Rev. Lett., 111, p. 021103. , arxiv:1304.5356, IceCube Collaborationpt_BR
dc.description.referenceBeacom, J.F., Bell, N.F., Hooper, D., Pakvasa, S., Weiler, T.J., (2003) Phys. Rev. Lett., 90, p. 181301. , arxiv:hep-ph/0211305pt_BR
dc.description.referenceMeloni, D., Ohlsson, T., (2007) Phys. Rev. D, 75, p. 125017. , arxiv:hep-ph/0612279pt_BR
dc.description.referenceBaerwald, P., Bustamante, M., Winter, W., (2012) J. Cosmol. Astropart. Phys., 1210, p. 020. , arxiv:1208.4600pt_BR
dc.description.referencePakvasa, S., Joshipura, A., Mohanty, S., (2013) Phys. Rev. Lett., 110, p. 171802. , arxiv:1209.5630pt_BR
dc.description.referenceDorame, L., Miranda, O.G., Valle, J.W.F., arxiv:1303.4891Fu, L., Ho, C.M., arxiv:1407.1090Beacom, J.F., Bell, N.F., (2002) Phys. Rev. D, 65, p. 113009. , arxiv:hep-ph/0204111pt_BR
dc.description.referenceGonzalez-Garcia, M.C., Maltoni, M., (2008) Phys. Lett. B, 663, p. 405. , arxiv:0802.3699pt_BR
dc.description.referenceGomes, R.A., Gomes, A.L.G., Perez, O.L.G., arxiv:1407.5640pt_BR
Appears in Collections:Unicamp - Artigos e Outros Documentos

Files in This Item:
File Description SizeFormat 
2-s2.0-84921447035.pdf291.8 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.