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Line Expansion Opacity in Relativistically Expanding Media · 1910 · DOI 10.3847/1538-4357/ab5306

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astro-ph.HE 1

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2026 1

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UNVERDICTED 1

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Signatures of $^{56}$Ni Mixing and Neutron-rich Ejecta in Supernovae

astro-ph.HE · 2026-06-22 · unverdicted · novelty 5.0

Multi-shell modeling shows outward 56Ni mixing produces faster brighter rises and biases one-zone fits to lower ejecta mass and higher nickel fraction, while r-process signatures in collapsars depend on placement, distribution, and viewing angle rather than always showing NIR excess.

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  • Signatures of $^{56}$Ni Mixing and Neutron-rich Ejecta in Supernovae astro-ph.HE · 2026-06-22 · unverdicted · none · ref 78

    Multi-shell modeling shows outward 56Ni mixing produces faster brighter rises and biases one-zone fits to lower ejecta mass and higher nickel fraction, while r-process signatures in collapsars depend on placement, distribution, and viewing angle rather than always showing NIR excess.