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dc.contributor.author | Esteban Pretel, Andreu | |
dc.contributor.author | Tomàs, Ricard | |
dc.contributor.author | Furtado Valle, José Wagner | |
dc.date.accessioned | 2015-09-30T10:03:43Z | |
dc.date.available | 2015-09-30T10:03:43Z | |
dc.date.issued | 2007 | |
dc.identifier.citation | Esteban Pretel, Andreu Tomàs, Ricard Furtado Valle, José Wagner 2007 Probing nonstandard neutrino interactions with supernova neutrinos Physical Review D 76 5 053001 | |
dc.identifier.uri | http://hdl.handle.net/10550/47475 | |
dc.description.abstract | We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through the detection of neutrinos produced in a future galactic supernova (SN).We consider the effect of NSI on the neutrino propagation through the SN envelope within a three-neutrino framework, paying special attention to the inclusion of NSI-induced resonant conversions, which may take place in the most deleptonised inner layers. We study the possibility of detecting NSI effects in a Megaton water Cherenkov detector, either through modulation effects in the ν¯e spectrum due to (i) the passage of shock waves through the SN envelope, (ii) the time dependence of the electron fraction and (iii) the Earth matter effects; or, finally, through the possible detectability of the neutronization νe burst. We find that the ν¯e spectrum can exhibit dramatic features due to the internal NSI-induced resonant conversion. This occurs for non-universal NSI strengths of a few %, and for very small flavor-changing NSI above a few×10−5. | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review D, 2007, vol. 76, num. 5, p. 053001 | |
dc.subject | Física | |
dc.title | Probing nonstandard neutrino interactions with supernova neutrinos | |
dc.type | journal article | es_ES |
dc.date.updated | 2015-09-30T10:03:43Z | |
dc.identifier.doi | 10.1103/PhysRevD.76.053001 | |
dc.identifier.idgrec | 043139 | |
dc.rights.accessRights | open access | es_ES |