Calculations indicate low probabilities (up to 11% for 89Sr, 5% for 22Na) of COSI detecting gamma-ray lines from i-process isotopes in nearby post-AGB stars or white dwarfs.
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Kilonova-like emissions after long GRBs GRB211211A and GRB230307A are consistent with collapsar nucleosynthesis using a single weak r-process component without lanthanide-rich material.
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Can COSI detect $\gamma$-ray lines from rare isotopes produced in the astrophysical intermediate neutron-capture process?
Calculations indicate low probabilities (up to 11% for 89Sr, 5% for 22Na) of COSI detecting gamma-ray lines from i-process isotopes in nearby post-AGB stars or white dwarfs.
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Kilonovae and Long-duration Gamma-ray Bursts
Kilonova-like emissions after long GRBs GRB211211A and GRB230307A are consistent with collapsar nucleosynthesis using a single weak r-process component without lanthanide-rich material.