Boltzmann Neutrino Transport Simulation of Core-Collapse Supernovae and the Collective Neutrino Flavor Instability

Boltzmann Neutrino Transport Simulation of Core-Collapse Supernovae and the Collective Neutrino Flavor Instability

Explore the intricacies of core-collapse supernovae and collective neutrino flavor instability in this 37-minute lecture by R. Akaho at the Galileo Galilei Institute. Delve into the complexities of Boltzmann neutrino transport simulations and their application to understanding these cosmic phenomena. Gain insights into the latest research and methodologies used to study neutrino behavior in extreme astrophysical environments. Learn about the challenges and advancements in modeling neutrino transport during supernova explosions, and discover how these simulations contribute to our understanding of stellar evolution and the universe's most energetic events.