Overview
Explore the intricacies of spin-flavor precession phase effects in supernovae through this 46-minute lecture delivered by Y. Pehlivan at the Galileo Galilei Institute. Delve into the complex physics behind these phenomena and their implications for our understanding of stellar explosions. Gain insights into the latest research and theoretical developments in the field of astrophysics, focusing on the role of neutrino oscillations and their impact on supernova dynamics. Enhance your knowledge of particle physics and cosmology as you examine the interplay between neutrino properties and the extreme conditions present during a supernova event.
Syllabus
Y. Pehlivan: "Spin-flavor precession phase effects in supernova"
Taught by
Galileo Galilei Institute