http://www.cnr.it/ontology/cnr/individuo/prodotto/ID6116
Effects of neutrino oscillations on the Supernova signal in LVD (Articolo in rivista)
- Type
- Label
- Effects of neutrino oscillations on the Supernova signal in LVD (Articolo in rivista) (literal)
- Anno
- 2002-01-01T00:00:00+01:00 (literal)
- Alternative label
Aglietta M., Fulgione W., Ghia P.L., Antonioli P., Castagnoli C., Galeotti, P., Picchi P., Ryazzhskya O., Vigorito C., Sartorelli G., Vissani F., Votano F., Zichichi A. et al. (2002)
Effects of neutrino oscillations on the Supernova signal in LVD
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Aglietta M., Fulgione W., Ghia P.L., Antonioli P., Castagnoli C., Galeotti, P., Picchi P., Ryazzhskya O., Vigorito C., Sartorelli G., Vissani F., Votano F., Zichichi A. et al. (literal)
- Pagina inizio
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#altreInformazioni
- Impact Factor 0,947 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
- Note
- ISI Web of Science (WOS) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- Institute of Cosmo-Geophysics, CNR, Torino,
University of Torino and INFN-Torino, Italy
University of Bologna and INFN-Bologna, Italy
University of Campinas, Campinas, Brazil
Institute for Nuclear Research, Russian Academy of
Sciences, Moscow, Russia
INFN-LNGS, and University of L'Aquila, Italy
Massachusetts Institute of Technology, Cambridge, USA
INFN-LNF, Frascati, Italy (literal)
- Titolo
- Effects of neutrino oscillations on the Supernova signal in LVD (literal)
- Abstract
- We study the impact of neutrino oscillations
on the supernova neutrino signal
in the Large Volume Detector (LVD).
The number of expected events for a galactic supernova ($D=10$ Kpc)
is calculated, assuming neutrino masses and mixing that
explain solar and atmospheric neutrino results.
The possibility to detect neutrinos in different channels
makes LVD sensitive to different
scenarios for $\nu$ properties, such as
normal or inverted $\nu$ mass hierarchy, and/or
adiabatic or non adiabatic MSW resonances associated to $U_{\rm e3}.$
Of particular importance are the charged current (c.c.) reactions on
$^{12}{\rm C}$: oscillations increase by almost one order of
magnitude the number of events expected from this channel.
%We study the implications on the supernova neutrino signal in liquid
%scintillator detectors due to the discovery of neutrino oscillations in
%atmospheric and solar neutrinos.\
%The combined detection of neutrinos through different interaction channels
%can help to distinguish between direct or inverse mass hierarchy and between
%adiabatic or non adiabatic conditions at the resonance
%($U_{\rm e3}^2\ll\gg 5\cdot 10^{-4}$). (literal)
- Autore CNR
- Insieme di parole chiave
Incoming links:
- Autore CNR di
- Prodotto
- Insieme di parole chiave di
