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.

*This material is based on work supported by the UCI-LANL-SoCal Hub Graduate Fellowship. TBS is supported by the Na-tional Science Foundation Graduate Research Fellowship Program under Grant No. 1839285.

Presenters

  • Tyler B Smith

    • University of California Irvine

Authors

  • Tyler B Smith

    • University of California Irvine
  • Shirley Li

    • University of California, Irvine
  • Luke F Roberts

    • Los Alamos National Lab
  • John F Beacom

    • Ohio State University
  • Francesco Capozzi

    • University of L'Aquila, Italy