Identifying the neutrino mass spectrum from a supernova neutrino burst

Abstract

We study the role that the future detection of the neutrino burst from a galactic supernova can play in the reconstruction of the neutrino mass spectrum. We consider all possible 3$\nu$ mass and flavor spectra which describe the solar and atmospheric neutrino data. For each of these spectra we find the observable effects of the supernova neutrino conversions both in the matter of the star and the earth. We show that studies of the electron neutrino and anineutrino spectra as well as observations of the neutral current effects from supernova will allow us (i) to identify the solar neutrino solution, (ii) to determine the type of mass hierarchy (normal or inverted) and (iii) to probe the mixing $|U_{e3}{|}^2$ to values as low as $10^{-4}-10^{-3}$.

53 pages, 13eps figures. Substantial changes made, new results, figures and tables added

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Cited by in corpus (380)

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• Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
• The Diffuse Supernova Neutrino Background
• Another possible way to determine the Neutrino Mass Hierarchy
• Leptonic CP violation
• Self-induced spectral splits in supernova neutrino fluxes
• Role of dense matter in collective supernova neutrino transformations
• Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
• Probing the neutrino mass hierarchy and the 13-mixing with supernovae
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• Linearized flavor-stability analysis of dense neutrino streams
• Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations
• Adiabaticity and spectral splits in collective neutrino transformations
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• Neutrino mass spectrum and neutrinoless double beta decay
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• Neutrino Mass Hierarchy and Stepwise Spectral Swapping of Supernova Neutrino Flavors
• Fast neutrino flavor conversions near the supernova core with realistic flavor-dependent angular distributions
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• Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies
• A dynamical collective calculation of supernova neutrino signals
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• No collective neutrino flavor conversions during the supernova accretion phase
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• (3+1)-spectrum of neutrino masses: A chance for LSND?
• Physics Potentials with the Second Hyper-Kamiokande Detector in Korea
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• Probing supernova shock waves and neutrino flavor transitions in next-generation water-Cherenkov detectors
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• Avoiding BBN Constraints on Mirror Models for Sterile Neutrinos
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• Supernova Neutrino Oscillations
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• Probing the Origins of Neutrino Mass with Supernova Data
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• Sensitivity Study of Supernova Neutrinos for Mass Hierarchy
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• Supernova $\nu$ flavour conversions in DUNE: the slow, the fast and the standard
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