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000315070 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2016-05/16
000315070 0247_ $$2ISSN$$a1435-8077
000315070 020__ $$a978-3-945931-08-0
000315070 037__ $$aPUBDB-2016-05605
000315070 041__ $$aEnglish
000315070 1001_ $$0P:(DE-H253)PIP1013186$$aSaviano, Ninetta$$b0$$eCorresponding author
000315070 1112_ $$0C16-03-17$$2inspire$$aMagellan Workshop$$cHamburg$$d2016-03-17 - 2016-03-18$$wGermany
000315070 245__ $$aPhysics Opportunities with Supernova Neutrinos
000315070 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2016
000315070 29510 $$aSaviano, Ninetta "Physics Opportunities with Supernova Neutrinos" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg
000315070 300__ $$a3-10
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000315070 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000315070 520__ $$aCore-collapse supernovae (SN) represent a unique laboratory to probe neutrino properties in the extreme conditions offered by a stellar gravitational collapse. The role of astrophysical messengers played by neutrinos during a stellar collapse is largely associated with the signatures imprinted on the observable SN neutrino burst by flavor conversions occurring deep inside the star. At this regard, the dense SN core represents a crucial environment to investigate neutrino flavor mixing in high-density conditions. Indeed, within a radius of a few hundred kilometers, the neutrino gas is so dense to become a 'background to itself', making the neutrino flavor evolution highly non-linear and leading in some situations to surprising and counterintuitive collective phenomena.
000315070 536__ $$0G:(EU-Grant)637506$$anuDirections - New Directions in Theoretical Neutrino Physics (637506)$$c637506$$fERC-2014-STG$$x0
000315070 7870_ $$0PUBDB-2016-05604$$aDahmke, Stefan K.G. et. al.$$dDeutsches Elektronen-Synchrotron, DESY$$iisPartOf$$rDESY-PROC-2016-05$$tProceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy: Hamburg, Germany, March 17-18, 2016
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000315070 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1013186$$aPRISMA Cluster of Excellence and Mainz Institute for Theoretical Physics - Johannes Gutenberg-Universit\"{a}t Mainz - 55099 Mainz - Germany$$b0$$kExtern
000315070 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1013186$$aU. Mainz, PRISMA$$b0
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