RHINE emulates r-process heating in NSM hydro simulations via neural networks trained on full nuclear trajectories, achieving <10% agreement with post-processing and boosting BH-torus ejecta mass by 40%.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
Ultraheavy nuclei have longer energy loss lengths at ≲300 EeV than lighter nuclei, allowing them to explain UHECRs above 100 EeV from sources like collapsars and neutron star mergers while predicting distinct shower maxima.
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.
citing papers explorer
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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.