Numerical models of fast radiation-mediated shocks and planar shock breakout show that including bound-free and bound-bound opacities from solar-composition heavy elements maintains local thermal equilibrium to higher velocities and reduces breakout emission temperatures by factors of two to ten.
arXiv:2504.00098
3 Pith papers cite this work, alongside 1 external citations. Polarity classification is still indexing.
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astro-ph.HE 3years
2025 3representative citing papers
The authors derive and calibrate analytical criteria, using a hydrogen-oxygen toy model and Cloudy simulations, that classify X-ray absorption states in photoionized gas across Thomson-thin and moderate-thick regimes, including scattering and boundary effects.
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.
citing papers explorer
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Radiation Mediated Shock and Planar Shock Breakout in the Presence of Atomic Transition Lines
Numerical models of fast radiation-mediated shocks and planar shock breakout show that including bound-free and bound-bound opacities from solar-composition heavy elements maintains local thermal equilibrium to higher velocities and reduces breakout emission temperatures by factors of two to ten.
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X-ray Transmission Through Photoionized Gas with Moderate Thomson Optical Depth
The authors derive and calibrate analytical criteria, using a hydrogen-oxygen toy model and Cloudy simulations, that classify X-ray absorption states in photoionized gas across Thomson-thin and moderate-thick regimes, including scattering and boundary effects.
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The Type IIn SN 2025cbj coincidence with the high-energy neutrino IceCube-250421A
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.