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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3 Pith papers cite this work, alongside 39 external citations. Polarity classification is still indexing.
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Simulations of the BSD instrument for POLAR-2 show it can localize faint GRBs like GRB 170817A to about 1.5 degrees accuracy, meeting requirements for supporting GRB polarimetry.
Future MeV telescopes could constrain axion-photon couplings to 1.61 × 10^{-13} GeV^{-1} for ALP masses below 10^{-9} eV using signals from galactic supernovae.
citing papers explorer
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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.
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Design and preliminary performance study of the broad-band spectrometer detector for POLAR-2
Simulations of the BSD instrument for POLAR-2 show it can localize faint GRBs like GRB 170817A to about 1.5 degrees accuracy, meeting requirements for supporting GRB polarimetry.
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Unveiling axion signals in galactic supernovae with future MeV telescopes
Future MeV telescopes could constrain axion-photon couplings to 1.61 × 10^{-13} GeV^{-1} for ALP masses below 10^{-9} eV using signals from galactic supernovae.