Mimar Sinan Güzel Sanatlar Üniversitesi Açık Bilim, Sanat Arşivi

Açık Bilim, Sanat Arşivi, Mimar Sinan Güzel Sanatlar Üniversitesi tarafından doğrudan ve dolaylı olarak yayınlanan; kitap, makale, tez, bildiri, rapor gibi tüm akademik kaynakları uluslararası standartlarda dijital ortamda depolar, Üniversitenin akademik performansını izlemeye aracılık eder, kaynakları uzun süreli saklar ve yayınların etkisini artırmak için telif haklarına uygun olarak Açık Erişime sunar.

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On the Neutrino Self Refraction Problem from a Many-Body Perspective

dc.contributor.authorPehlivan, Y.
dc.contributor.authorKajino, Toshitaka
dc.contributor.authorBalantekin, A. B.
dc.contributor.authorYoshida, Takashi
dc.contributor.authorMaruyama, Tomoyuki
dc.date.accessioned2025-01-09T20:12:05Z
dc.date.available2025-01-09T20:12:05Z
dc.date.issued2010
dc.identifier.isbn978-0-7354-0819-7
dc.identifier.issn0094-243X
dc.identifier.urihttps://doi.org/10.1063/1.3485133
dc.identifier.urihttps://hdl.handle.net/20.500.14124/8348
dc.description10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10) -- MAR 08-10, 2010 -- Osaka Univ, Res Ctr Nucl Phys, Osaka, JAPANen_US
dc.description.abstractWe consider a dense neutrino gas as a many body system by taking into account both vacuum oscillations and self interactions of neutrinos. We show that the exact many body Hamiltonian which describes the flavor oscillations of such a dense neutrino gas has many constants of motion whose eigenvalues represent a set of good quantum numbers. However, if one adopts the random phase approximation as an effective one particle description, these operators are no longer conserved (i.e., they cease to represent good quantum numbers) although their expectation values are still conserved.en_US
dc.description.sponsorshipRIKEN Nishina Ctr,Univ Tokyo, Ctr Nucl Study,Natl Astron Observ Japan, Div Theoret Astrophys,High Energy Accelerator Res Org,Japan Atom Energy Agcy,Konan Univen_US
dc.description.sponsorshipScientific Research of JSPS [20244035]; JSPS; U.S. National Science Foundation [PHY-0855082]; Scientific Research from MEXT [20540284, 21540412]; [20105004]; Grants-in-Aid for Scientific Research [20540284] Funding Source: KAKEN; Direct For Mathematical & Physical Scien; Division Of Physics [0855082] Funding Source: National Science Foundationen_US
dc.description.sponsorshipThis work was supported in part by Grant-in-Aid for Scientific Research of JSPS (20244035), in part by JSPS Core-to-Core Program EFES, in part by the U.S. National Science Foundation Grant No. PHY-0855082, in part by Grants-in-Aid for the Scientific Research on InnovativeAreas (20105004) and Scientific Research (20540284, 21540412) from MEXT.en_US
dc.language.isoengen_US
dc.publisherAmer Inst Physicsen_US
dc.relation.ispartof10th International Symposium on Origin of Matter and Evolution of Galaxiesen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectSupernovaeen_US
dc.subjectnonlinear effects in neutrino propagationen_US
dc.subjectneutrinos in matteren_US
dc.subjectintegrable dynamicsen_US
dc.titleOn the Neutrino Self Refraction Problem from a Many-Body Perspectiveen_US
dc.typeconferenceObjecten_US
dc.authoridYoshida, Takashi/0000-0002-8967-7063
dc.departmentMimar Sinan Güzel Sanatlar Üniversitesien_US
dc.identifier.doi10.1063/1.3485133
dc.identifier.volume1269en_US
dc.identifier.startpage189en_US
dc.identifier.endpage+en_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US
dc.identifier.wosqualityN/A
dc.identifier.wosWOS:000281986900027
dc.identifier.scopus2-s2.0-77956633369
dc.identifier.scopusqualityQ4
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.snmzKA_20250105


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