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Physics of neutrino flavor transformation through matter - neutrino resonances

Wu, Meng-Ru ; Duan, Huaiyu ; Qian, Yong-Zhong (2016)
Physics of neutrino flavor transformation through matter - neutrino resonances.
In: Physics Letters B, 752
doi: 10.1016/j.physletb.2015.11.027
Artikel, Bibliographie

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Kurzbeschreibung (Abstract)

In astrophysical environments such as core-collapse supernovae and neutron star–neutron star or neutron star–black hole mergers where dense neutrino media are present, matter–neutrino resonances (MNRs) can occur when the neutrino propagation potentials due to neutrino–electron and neutrino–neutrino forward scattering nearly cancel each other. We show that neutrino flavor transformation through MNRs can be explained by multiple adiabatic solutions similar to the Mikheyev–Smirnov–Wolfenstein mechanism. We find that for the normal neutrino mass hierarchy, neutrino flavor evolution through MNRs can be sensitive to the shape of neutrino spectra and the adiabaticity of the system, but such sensitivity is absent for the inverted hierarchy.

Typ des Eintrags: Artikel
Erschienen: 2016
Autor(en): Wu, Meng-Ru ; Duan, Huaiyu ; Qian, Yong-Zhong
Art des Eintrags: Bibliographie
Titel: Physics of neutrino flavor transformation through matter - neutrino resonances
Sprache: Englisch
Publikationsjahr: 2016
Verlag: Elsevier
Titel der Zeitschrift, Zeitung oder Schriftenreihe: Physics Letters B
Jahrgang/Volume einer Zeitschrift: 752
DOI: 10.1016/j.physletb.2015.11.027
Zugehörige Links:
Kurzbeschreibung (Abstract):

In astrophysical environments such as core-collapse supernovae and neutron star–neutron star or neutron star–black hole mergers where dense neutrino media are present, matter–neutrino resonances (MNRs) can occur when the neutrino propagation potentials due to neutrino–electron and neutrino–neutrino forward scattering nearly cancel each other. We show that neutrino flavor transformation through MNRs can be explained by multiple adiabatic solutions similar to the Mikheyev–Smirnov–Wolfenstein mechanism. We find that for the normal neutrino mass hierarchy, neutrino flavor evolution through MNRs can be sensitive to the shape of neutrino spectra and the adiabaticity of the system, but such sensitivity is absent for the inverted hierarchy.

Zusätzliche Informationen:

Keywords: Neutrino oscillations; Dense neutrino medium; Black hole accretion disk; Core-collapse supernova

Sachgruppe der Dewey Dezimalklassifikatin (DDC): 500 Naturwissenschaften und Mathematik > 530 Physik
Fachbereich(e)/-gebiet(e): 05 Fachbereich Physik
05 Fachbereich Physik > Institut für Kernphysik
Hinterlegungsdatum: 02 Aug 2024 12:38
Letzte Änderung: 02 Aug 2024 12:38
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