Add to ORKGObserving a high-statistics neutrino signal from a galactic supernova (SN) would allow one to test the standard delayed explosion scenario and may allow one to distinguish between the normal and inverted neutrino mass ordering due to the effects of flavor oscillations in the SN envelope. One may even observe a signature of SN shock-wave propagation in the detailed time-evolution of the neutrino spectra. A clear identification of flavor oscillation effects in a water Cherenkov detector probably requires a megatonne-class experiment
Neutrinos and antineutrinos of all three flavours are emitted during the post bounce phase of a core...
Twenty years after SN 1987A, the vast international programme of experimental neutrino physics and n...
We review how a high-statistics observation of the neutrino signal from a future galactic core-colla...
After a brief review of our current understanding of neutrino flavor conversions inside a core colla...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
I shall review some of the recent results concerning the astrophysics of a core collapse supernova (...
IceCube, a future km^3 antarctic ice Cherenkov neutrino telescope, is highly sensitive to a galactic...
The neutrinos from a type II supernova provide perhaps our best opportunity to probe cosmologically ...
The neutrinos from a type II supernova provide perhaps our best opportunity to probe cosmologically ...
IceCube, a future km3 antarctic ice Cherenkov neutrino telescope, is highly sensitive to a galactic ...
The high-statistics neutrino signal from the next nearby supernova (SN) would provide a bonanza of a...
The neutrinos from a type II supernova provide perhaps our best opportunity to probe cosmologically ...
We carry out a detailed analysis of the supernova (SN) neutrino flavor evolution during the accretio...
Neutrinos and antineutrinos of all three flavours are emitted during the post bounce phase of a core...
Twenty years after SN 1987A, the vast international programme of experimental neutrino physics and n...
We review how a high-statistics observation of the neutrino signal from a future galactic core-colla...
After a brief review of our current understanding of neutrino flavor conversions inside a core colla...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
I shall review some of the recent results concerning the astrophysics of a core collapse supernova (...
IceCube, a future km^3 antarctic ice Cherenkov neutrino telescope, is highly sensitive to a galactic...
The neutrinos from a type II supernova provide perhaps our best opportunity to probe cosmologically ...
The neutrinos from a type II supernova provide perhaps our best opportunity to probe cosmologically ...
IceCube, a future km3 antarctic ice Cherenkov neutrino telescope, is highly sensitive to a galactic ...
The high-statistics neutrino signal from the next nearby supernova (SN) would provide a bonanza of a...
The neutrinos from a type II supernova provide perhaps our best opportunity to probe cosmologically ...
We carry out a detailed analysis of the supernova (SN) neutrino flavor evolution during the accretio...
Neutrinos and antineutrinos of all three flavours are emitted during the post bounce phase of a core...
Twenty years after SN 1987A, the vast international programme of experimental neutrino physics and n...
We review how a high-statistics observation of the neutrino signal from a future galactic core-colla...