Supernova Neutrino Detection
arXiv:1205.6003 · doi:10.1146/annurev-nucl-102711-095006
Abstract
A core-collapse supernova will produce an enormous burst of neutrinos of all flavors in the few-tens-of-MeV range. Measurement of the flavor, time and energy structure of a nearby core-collapse neutrino burst will yield answers to many physics and astrophysics questions. The neutrinos left over from past cosmic supernovae are also observable, and their detection will improve knowledge of core collapse rates and average neutrino emission. This review describes experimental techniques for detection of core-collapse neutrinos, as well as the sensitivities of current and future detectors.
Review article to be published in the Annual Review of Nuclear and Particle Science, October 2012
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Cited by in corpus (5)
- The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
- Searching for prompt signatures of nearby core-collapse supernovae by a joint analysis of neutrino and gravitational-wave data
- Charged current neutrino interactions in core-collapse supernovae in a virial expansion
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- Discovering the New Standard Model: Fundamental Symmetries and Neutrinos