Earth matter effects on the supernova neutrino spectra
| dc.creator | Dighe, Amol S. | |
| dc.date | 2001-06-28 | |
| dc.date.accessioned | 2026-07-07T03:44:52Z | |
| dc.date.available | 2026-07-07T03:44:52Z | |
| dc.description | We explore the earth matter effects on the energy spectra of neutrinos from a supernova. We show that the observations of the energy spectra of $ν_e$ and $\barν_e$ from a galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $Δm^2_{32}$, and to probe the mixing matrix element $|U_{e3}|^2$ to values as low as $10^{-3}$. We point out scenarios in which the matter effects can even be established through the observation of the spectrum at a single detector. | |
| dc.description | 8 pages LaTeX, 2 eps figures, uses Rinton-P9x6.cls. Talk given at CICHEP '2001, Cairo, Egypt, January 2001 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0106325 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0106325 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40738 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Earth matter effects on the supernova neutrino spectra | |
| dc.type | text |