Exploring Supernova Dynamics and Neutrino Properties via Comprehensive Spectral Analysis
ORAL
Abstract
Core-collapse supernovae release nearly all their energy as neutrinos, offering a unique view into supernova dynamics and proto-neutron star properties. We develop a pipeline to reconstruct neutrino spectra detected at Earth-based observatories, utilizing advanced machine learning techniques, which prove advantageous over traditional matrix inversion methods. This approach reveals essential features of supernova dynamics, enhancing our understanding of these powerful events and informing future studies in experimental neutrino physics.
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Presenters
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Tyler B Smith
University of California Irvine
Authors
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Tyler B Smith
University of California Irvine
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Shirley Li
University of California, Irvine
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Luke F Roberts
Los Alamos National Lab
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John F Beacom
Ohio State University
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Francesco Capozzi
University of L'Aquila, Italy