Neutrinos from a core collapse supernova

Abstract

The neutrino burst from a galactic supernova can help determine the neutrino mass hierarchy and ${\theta }_{13}$, and provide crucial information about supernova astrophysics. Here we review our current understanding of the neutrino burst, flavor conversions of these neutrinos, and model independent signatures of various neutrino mixing scenarios.

5 pages, aipproc format, Plenary talk at NuFact07

References in corpus (7)

• Collective neutrino flavor transitions in supernovae and the role of trajectory averaging
• Self-induced spectral splits in supernova neutrino fluxes
• Adiabaticity and spectral splits in collective neutrino transformations
• Decoherence in supernova neutrino transformations suppressed by deleptonization
• Collective three-flavor oscillations of supernova neutrinos
• Flavor Evolution of the Neutronization Neutrino Burst from an O-Ne-Mg Core-Collapse Supernova
• Oscillation Effects and Time Variation of the Supernova Neutrino Signal

Cited by in corpus (9)

• Collective three-flavor oscillations of supernova neutrinos
• Spectral split in prompt supernova neutrino burst: Analytic three-flavor treatment
• Identifying neutrino mass hierarchy at extremely small theta(13) through Earth matter effects in a supernova signal
• Physics potential of future supernova neutrino observations
• Robust measurement of supernova ${\nu }_e$ spectra with future neutrino detectors
• Minimal Neutrino Beta Beam for Large theta_13
• Realistic Earth matter effects and a method to acquire information about small θ_{13} in the detection of supernova neutrinos
• Acquire information about neutrino parameters by detecting supernova neutrinos
• Supernova Neutrinos Detection On Earth