TL;DR
This paper reviews methods for detecting neutrinos from supernovae, discussing current and future detector sensitivities to understand supernova mechanisms and neutrino properties.
Contribution
It provides a comprehensive overview of experimental techniques and sensitivities for supernova neutrino detection, highlighting recent advancements and future prospects.
Findings
Current detectors can observe neutrino bursts from nearby supernovae.
Detection of cosmic supernova neutrino background is feasible with future detectors.
Enhanced sensitivity will improve understanding of supernova physics and neutrino properties.
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.
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