AbstractWe study νe and ν¯e signals from a supernova with strong magnetic field detected by a 100 kton liquid Ar detector. The change of neutrino flavors by resonant spin-flavor conversions, matter effects, and neutrino self-interactions are taken into account. Different neutrino signals, characterized by the total event numbers of νe and ν¯e and neutronization burst event, are expected with different neutrino oscillation parameters and neutrino magnetic moment. Observations of supernova neutrino signals by a 100 kton liquid Ar detector would constrain oscillation parameters as well as neutrino magnetic moment in either normal and inverted mass hierarchies
The νμ and ντ neutrinos (and their antiparticles) from a Galactic core-collapse supernova can be obs...
We investigate the discovery potential of a water-Cherenkov Megaton detector in the diagnostic of a ...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...
AbstractWe study νe and ν¯e signals from a supernova with strong magnetic field detected by a 100 kt...
Resonant spin-flavor (RSF) conversions of supernova neutrinos, which is induced by the interaction b...
The undetermined neutrino mass hierarchy may leave an observable imprint on the neutrino fluxes from...
The neutrino spin-flavor conversion of \bar\nu_e and \nu_\mu which is induced by the interaction of ...
We point out possible features of neutrino spectra from a future galactic core collapse supernova th...
We study supernova neutrino burst signals in large water erenkov detectors, examining the effects of...
We investigate the sensitivity of some of the proposed next-generation neutrino experiments to a gal...
We summarize our current understanding of the neutrino flavor conversions inside a core collapse sup...
AbstractThe calculations for the neutrino absorption cross sections for supernova neutrinos in 40Ar ...
We study the effect of including flavor changing neutral currents (FCNC) in the analysis of the neut...
A core-collapse supernova (SN) offers an excellent astrophysical laboratoryto test non-zero neutrino...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...
The νμ and ντ neutrinos (and their antiparticles) from a Galactic core-collapse supernova can be obs...
We investigate the discovery potential of a water-Cherenkov Megaton detector in the diagnostic of a ...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...
AbstractWe study νe and ν¯e signals from a supernova with strong magnetic field detected by a 100 kt...
Resonant spin-flavor (RSF) conversions of supernova neutrinos, which is induced by the interaction b...
The undetermined neutrino mass hierarchy may leave an observable imprint on the neutrino fluxes from...
The neutrino spin-flavor conversion of \bar\nu_e and \nu_\mu which is induced by the interaction of ...
We point out possible features of neutrino spectra from a future galactic core collapse supernova th...
We study supernova neutrino burst signals in large water erenkov detectors, examining the effects of...
We investigate the sensitivity of some of the proposed next-generation neutrino experiments to a gal...
We summarize our current understanding of the neutrino flavor conversions inside a core collapse sup...
AbstractThe calculations for the neutrino absorption cross sections for supernova neutrinos in 40Ar ...
We study the effect of including flavor changing neutral currents (FCNC) in the analysis of the neut...
A core-collapse supernova (SN) offers an excellent astrophysical laboratoryto test non-zero neutrino...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...
The νμ and ντ neutrinos (and their antiparticles) from a Galactic core-collapse supernova can be obs...
We investigate the discovery potential of a water-Cherenkov Megaton detector in the diagnostic of a ...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...