Identifying the neutrino mass spectrum from a supernova neutrino burst
作者： Amol S. Dighe , Alexei Yu. Smirnov
DOI: 10.1103/PHYSREVD.62.033007
关键词:
摘要: We study the role that future detection of neutrino burst from a galactic supernova can play in reconstruction mass spectrum. consider all possible 3$\nu$ and flavor spectra which describe solar atmospheric data. For each these we find observable effects conversions both matter star earth. show studies electron anineutrino as well observations neutral current will allow us (i) to identify solution, (ii) determine type hierarchy (normal or inverted) (iii) probe mixing $|U_{e3}|^2$ values low $10^{-4} - 10^{-3}$.
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