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dc.contributor.authorSubaşı, Ahmet Levent
dc.contributor.authorBirol, Savaş
dc.contributor.authorGhazanfari, N.
dc.contributor.authorYuksel, H.
dc.contributor.authorPehlivan, Y.
dc.date.accessioned2021-03-05T10:28:18Z
dc.date.available2021-03-05T10:28:18Z
dc.date.issued2017
dc.identifier.citationPehlivan Y., Subaşı A. L. , Ghazanfari N., Birol S., Yuksel H., "Spectral splits of neutrinos as a BCS-BEC crossover type phenomenon", PHYSICAL REVIEW D, cilt.95, 2017
dc.identifier.issn2470-0010
dc.identifier.otherav_a33ffae8-94b1-420e-b860-943163fb577d
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/109274
dc.identifier.urihttps://doi.org/10.1103/physrevd.95.063022
dc.description.abstractWe show that the spectral split of a neutrino ensemble, which initially consists of electron type neutrinos, is analogous to the Bardeen-Cooper-Schrieffer-Bose-Einstein condensate (BCS-BEC) crossover already observed in ultracold atomic gas experiments. Such a neutrino ensemble mimics the deleptonization burst of a core collapse supernova. Although these two phenomena belong to very different domains of physics, the propagation of neutrinos from highly interacting inner regions of the supernova to the vacuum is reminiscent of the evolution of Cooper pairs between weak and strong interaction regimes during the crossover. The Hamiltonians and the corresponding many-body states undergo very similar transformations if one replaces the pair quasispin of the latter with the neutrino isospin of the former.
dc.language.isoeng
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectFizik
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleSpectral splits of neutrinos as a BCS-BEC crossover type phenomenon
dc.typeMakale
dc.relation.journalPHYSICAL REVIEW D
dc.contributor.departmentMimar Sinan Güzel Sanatlar Üniversitesi , ,
dc.identifier.volume95
dc.identifier.issue6
dc.contributor.firstauthorID86574


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