Treating select nuclear isomers as independent states with temperature-dependent rates in r-process networks yields predictions that the 743.3 keV Nb-97m and 555.6 keV Y-91m lines may be detectable at galactic distances by COSI, AMEGO, or LOX.
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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.
This is a review chapter summarizing the established framework of scattering theory in particle physics.
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Scattering Theory
This is a review chapter summarizing the established framework of scattering theory in particle physics.