An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for sensitivity to the neutrino mass hierarchy is presented. Confidence intervals for Δ m 2 32 , sin 2 θ 23 , sin 2 θ 13 and δ C P are presented for normal neutrino mass hierarchy and inverted neutrino mass hierarchy hypotheses, based on atmospheric neutrino data alone. Additional constraints from reactor data on θ 13 and from published binned T2K data on muon neutrino disappearance and electron neutrino appearance are added to the atmospheric neutrino fit to give enhanced constraints on the above parameters. Over the range of parameters allowed at 90% confidence level, the normal mass hierarchy is favored by betwee...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
A new event reconstruction algorithm based on a maximum likelihood method has been developed for Sup...
A new event reconstruction algorithm based on a maximum likelihood method has been developed for Sup...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
Using 5326 days of atmospheric neutrino data, a search for atmospheric tau neutrino appearance has b...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...
Using 5326 days of atmospheric neutrino data, a search for atmospheric tau neutrino appearance has b...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
A new event reconstruction algorithm based on a maximum likelihood method has been developed for Sup...
A new event reconstruction algorithm based on a maximum likelihood method has been developed for Sup...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
Using 5326 days of atmospheric neutrino data, a search for atmospheric tau neutrino appearance has b...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...
Using 5326 days of atmospheric neutrino data, a search for atmospheric tau neutrino appearance has b...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...
We report a search for astronomical neutrinos in the energy region from several GeV to TeV in the di...