For a low-mass CCSN progenitor, rotation alone weakly and non-monotonically affects explosion energy and observables; only the fastest spin yields T/|W| spiral modes and spin-kick alignment, with core spin amplified by ~4000.
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The chapter summarizes established nuclear many-body theory formalisms for calculating low-energy neutrino cross sections in nuclear matter and their implications for astrophysics.
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Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors
For a low-mass CCSN progenitor, rotation alone weakly and non-monotonically affects explosion energy and observables; only the fastest spin yields T/|W| spiral modes and spin-kick alignment, with core spin amplified by ~4000.
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Neutrino Cross Sections: Low Energy
The chapter summarizes established nuclear many-body theory formalisms for calculating low-energy neutrino cross sections in nuclear matter and their implications for astrophysics.