Physics with Supernovae
arXiv:hep-ph/0201099 · doi:10.1016/S0920-5632(02)01489-5
Abstract
Core-collapse supernovae (SNe) are powerful neutrino sources and as such important targets for the growing array of neutrino observatories. We review the current status of SN theory and the expected characteristics of the neutrino signal. After recalling what we have learned from SN 1987A and general SN properties we review the physics potential of a future galactic SN observation.
Contribution to TAUP 2001
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- Detection of Supernova Neutrinos by Neutrino-Proton Elastic Scattering
- Absolute Values of Neutrino Masses: Status and Prospects
- Multimessengers from core-collapse supernovae: multidimensionality as a key to bridge theory and observation
- Neutrino-nucleus interaction rates at a low-energy beta-beam facility
- A Network of Neutral Current Spherical TPC's for Dedicated Supernova Detection
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- Robust measurement of supernova spectra with future neutrino detectors
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- Gravitational Lensing of Supernova Neutrinos
- Supernova Neutrinos and the LSND Evidence for Neutrino Oscillations
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