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Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos
We analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. We find that the observations of the energy spectra of neutrinos from a future galactic supernova may enable us to identify the solar neutrino solution...
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| Lenguaje: | eng |
| Publicado: |
1999
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| Acceso en línea: | https://dx.doi.org/10.1016/S0920-5632(00)00694-0 http://cds.cern.ch/record/412637 |
| _version_ | 1780894677772271616 |
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| author | Dighe, Amol S. |
| author_facet | Dighe, Amol S. |
| author_sort | Dighe, Amol S. |
| collection | CERN |
| description | We analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. We find that the observations of the energy spectra of neutrinos from a future galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $\Delta m^2_{32}$, and to probe the mixing matrix element |U_{e3}|^2 to values as low as 10^{-4}-10^{-3}. |
| id | cern-412637 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 1999 |
| record_format | invenio |
| spelling | cern-4126372023-03-14T18:59:49Zdoi:10.1016/S0920-5632(00)00694-0http://cds.cern.ch/record/412637engDighe, Amol S.Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinosParticle Physics - PhenomenologyWe analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. We find that the observations of the energy spectra of neutrinos from a future galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $\Delta m^2_{32}$, and to probe the mixing matrix element |U_{e3}|^2 to values as low as 10^{-4}-10^{-3}.We analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. We find that the observations of the energy spectra of neutrinos from a future galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $\Delta m^2_{32}$, and to probe the mixing matrix element |U_{e3}|^2 to values as low as 10^{-4}-10^{-3}.hep-ph/9912414CERN-TH-99-382CERN-TH-99-382oai:cds.cern.ch:4126371999-12-21 |
| spellingShingle | Particle Physics - Phenomenology Dighe, Amol S. Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos |
| title | Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos |
| title_full | Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos |
| title_fullStr | Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos |
| title_full_unstemmed | Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos |
| title_short | Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos |
| title_sort | resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos |
| topic | Particle Physics - Phenomenology |
| url | https://dx.doi.org/10.1016/S0920-5632(00)00694-0 http://cds.cern.ch/record/412637 |
| work_keys_str_mv | AT digheamols resolvingambiguitiesintheneutrinomassflavourspectrumfromsupernovaneutrinos |