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Collective flavor transitions of supernova neutrinos

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Conference object , Other literature type 01 Mar 2009Embargo end date: 01 Jan 2009 English Publisher:Elsevier BVJournal:Nuclear Physics B - Proceedings Supplements, volume 188, pages 101-106 (issn: 0920-5632,

Authors: Pasquale D. Serpico; Alessandro Mirizzi; Andreu Esteban-Pretel; Guenter Sigl; Ricard Tomàs; Georg G. Raffelt; Sergio Pastor;

doi: 10.1016/j.nuclphysbps.2009.02.023 , 10.48550/arxiv.0901.0725

arXiv: http://arxiv.org/abs/0901.0725

handle: 10261/21418

Collective flavor transitions of supernova neutrinos

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Abstract

We give a very brief overview of collective effects in neutrino oscillations in core collapse supernovae where refractive effects of neutrinos on themselves can considerably modify flavor oscillations, with possible repercussions for future supernova neutrino detection. We discuss synchronized and bipolar oscillations, the role of energy and angular neutrino modes, as well as three-flavor effects. We close with a short summary and some open questions.

6 pages, 2 figures, proceedings for plenary talk by G.Sigl at NOW2008, Conca Specchiulla, Otranto, Italy, September 2008; added reference for the CP-phase

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Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena

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