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.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 3verdicts
UNVERDICTED 3roles
background 1polarities
background 1representative citing papers
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.
citing papers explorer
-
Nuclear Isomers and Their Impact on Gamma-Ray Emission in Binary Neutron Star Mergers
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.
-
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.
-
Scattering Theory
This is a review chapter summarizing the established framework of scattering theory in particle physics.