Diffuse supernova neutrinos at underground laboratories

作者: Cecilia Lunardini

DOI: 10.1016/J.ASTROPARTPHYS.2016.02.005

关键词:

摘要: Abstract I review the physics of Diffuse Supernova Neutrino flux (or Background, DSNB), in context future searches at next generation neutrino observatories. The theory DSNB is discussed its fundamental elements, namely cosmological rate supernovae, production inside a core collapse supernova, redshift, and flavor oscillation effects. current upper limits are also reviewed, results shown for rates energy distributions events expected liquid argon scintillator detectors O ( 10 ) kt mass, water Cherenkov up to 0.5 Mt mass. Perspectives given on significance observations DSNB, both discovery precision phases, investigation supernovae properties neutrino.

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