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[PENDING] SUPERNOVAE THEORY: STUDY OF ELECTRO-WEAK PROCESSES DURING GRAVITATIONAL COLLAPSE OF MASSIVE STARS

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Figure 1.1: Schematic representation of the initial phases of the collapse of the core (here a cut of the core is shown, in spherical symmetry)
Figure 1.3: Schematic representation of the shock stagnation and neutrino heating and cooling (as in Fig
Figure 1.4: Scheme of electron capture and β decay processes. Fermi (F) and Gamow-Teller (GT) transitions are displayed
Figure 2.1: Theoretical and computational methods used to solve the many-body problem
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