Dust from refractory r-process elements forms efficiently in kilonova ejecta and explains the observed late-time infrared spectra.
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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.
citing papers explorer
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Heavy element dust explains the late-time spectra of kilonovae
Dust from refractory r-process elements forms efficiently in kilonova ejecta and explains the observed late-time infrared spectra.
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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.