v2: 17 pages, 6 eps figures. Typos removed, matches the published version. Online tool to calculate the Earth shadowing probabilities available at http://www.mppmu.mpg.de/supernova/shadowing . High-resolution color version of fig_2a and fig_2b available at http://www.mppmu.mpg.de/supernova/shadowing/ma
The neutrino oscillations in Earth matter introduce modulations in the supernova neutrino spectra. T...
A future galactic SN can be located several hours before the optical explosion through the MeV-neutr...
IceCube, a future km^3 antarctic ice Cherenkov neutrino telescope, is highly sensitive to a galactic...
A model-independent experimental signature for flavor oscillations in the neutrino signal from the n...
A model-independent experimental signature for flavor oscillations in the neutrino signal from the n...
Abstract. A model-independent experimental signature for flavour oscillations in the neutrino signal...
Matter effects on neutrino oscillations in both, a supernova and the Earth, change the observed sup...
A future galactic SN can be located several hours before the optical explosion through the MeV-neut...
(14 pages, 5 ps figures)International audienceNeutrino oscillations in the Earth matter may introduc...
(14 pages, 5 ps figures)International audienceNeutrino oscillations in the Earth matter may introduc...
The Earth matter effects on supernova (SN) neutrinos can be identified at a single detector through ...
A core-collapse supernova will emit a neutrino burst that can be detected on Earth. If the neutrinos...
The neutrino oscillations in Earth matter introduce modulations in the supernova neutrino spectra. T...
A future galactic SN can be located several hours before the optical explosion through the MeV-neutr...
We investigate the sensitivity of some of the proposed next-generation neutrino experiments to a gal...
The neutrino oscillations in Earth matter introduce modulations in the supernova neutrino spectra. T...
A future galactic SN can be located several hours before the optical explosion through the MeV-neutr...
IceCube, a future km^3 antarctic ice Cherenkov neutrino telescope, is highly sensitive to a galactic...
A model-independent experimental signature for flavor oscillations in the neutrino signal from the n...
A model-independent experimental signature for flavor oscillations in the neutrino signal from the n...
Abstract. A model-independent experimental signature for flavour oscillations in the neutrino signal...
Matter effects on neutrino oscillations in both, a supernova and the Earth, change the observed sup...
A future galactic SN can be located several hours before the optical explosion through the MeV-neut...
(14 pages, 5 ps figures)International audienceNeutrino oscillations in the Earth matter may introduc...
(14 pages, 5 ps figures)International audienceNeutrino oscillations in the Earth matter may introduc...
The Earth matter effects on supernova (SN) neutrinos can be identified at a single detector through ...
A core-collapse supernova will emit a neutrino burst that can be detected on Earth. If the neutrinos...
The neutrino oscillations in Earth matter introduce modulations in the supernova neutrino spectra. T...
A future galactic SN can be located several hours before the optical explosion through the MeV-neutr...
We investigate the sensitivity of some of the proposed next-generation neutrino experiments to a gal...
The neutrino oscillations in Earth matter introduce modulations in the supernova neutrino spectra. T...
A future galactic SN can be located several hours before the optical explosion through the MeV-neutr...
IceCube, a future km^3 antarctic ice Cherenkov neutrino telescope, is highly sensitive to a galactic...
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