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Neutrino magnetic moment, CP violation, and flavor oscillations in matter
dc.contributor.author | Pehlivan, Y. | |
dc.contributor.author | Balantekin, A. B. | |
dc.contributor.author | Kajino, Toshitaka | |
dc.date.accessioned | 2025-01-09T20:12:19Z | |
dc.date.available | 2025-01-09T20:12:19Z | |
dc.date.issued | 2014 | |
dc.identifier.issn | 1550-7998 | |
dc.identifier.issn | 1550-2368 | |
dc.identifier.uri | https://doi.org/10.1103/PhysRevD.90.065011 | |
dc.identifier.uri | https://hdl.handle.net/20.500.14124/8554 | |
dc.description.abstract | We consider collective oscillations of neutrinos, which are emergent nonlinear flavor evolution phenomena instigated by neutrino-neutrino interactions in astrophysical environments with sufficiently high neutrino densities. We investigate the symmetries of the problem in the full three-flavor mixing scheme and in the exact many-body formulation by including the effects of CP violation and the neutrino magnetic moment. We show that, similar to the two-flavor scheme, several dynamical symmetries exist for three flavors in the single-angle approximation if the net electron background in the environment and the effects of the neutrino magnetic moment are negligible. Moreover, we show that these dynamical symmetries are present even when the CP symmetry is violated in neutrino oscillations. We explicitly write down the constants of motion through which these dynamical symmetries manifest themselves in terms of the generators of the SU(3) flavor transformations. We also show that the effects due to the CP-violating Dirac phase factor out of the many-body evolution operator and evolve independently of nonlinear flavor transformations if neutrino electromagnetic interactions are ignored. In the presence of a strong magnetic field, CP-violating effects can still be considered independently provided that an effective definition for the neutrino magnetic moment is used. | en_US |
dc.description.sponsorship | Scientific and Technological Research Council of Turkey (TUBITAK) [112T952]; U. S. National Science Foundation [PHY-1205024]; University of Wisconsin Research Committee; Wisconsin Alumni Research Foundation; JSPS of the Ministry of Education, Culture, Sports, Science and Technology of Japan [26105517, 24340060]; Division Of Physics; Direct For Mathematical & Physical Scien [1205024] Funding Source: National Science Foundation; Grants-in-Aid for Scientific Research [26105517] Funding Source: KAKEN | en_US |
dc.description.sponsorship | Y. P. is grateful to the University of Wisconsin for their hospitality where part of this work was completed and to the American Physical Society for the International Travel Grant Award which allowed her visit. Y. P. and A. B. B. thank the National Astronomical Observatory of Japan for their hospitality. We also thank CETUP* 2013 organizers for allowing a stimulating environment for critical discussion of some of our results. This work was supported in part by the Scientific and Technological Research Council of Turkey (TUBITAK) under Project No. 112T952, in part by the U. S. National Science Foundation Grant No. PHY-1205024, in part by the University of Wisconsin Research Committee with funds granted by the Wisconsin Alumni Research Foundation, and in part by Grants-in-Aid for Scientific Research of JSPS (Grants No. 26105517, No. 24340060) of the Ministry of Education, Culture, Sports, Science and Technology of Japan. | en_US |
dc.language.iso | eng | en_US |
dc.publisher | Amer Physical Soc | en_US |
dc.relation.ispartof | Physical Review D | en_US |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.title | Neutrino magnetic moment, CP violation, and flavor oscillations in matter | en_US |
dc.type | article | en_US |
dc.authorid | Balantekin, Akif/0000-0002-2999-0111 | |
dc.department | Mimar Sinan Güzel Sanatlar Üniversitesi | en_US |
dc.identifier.doi | 10.1103/PhysRevD.90.065011 | |
dc.identifier.volume | 90 | en_US |
dc.identifier.issue | 6 | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.identifier.wosquality | Q1 | |
dc.identifier.wos | WOS:000343759200008 | |
dc.indekslendigikaynak | Web of Science | en_US |
dc.snmz | KA_20250105 |
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