Self-consistent simulations reveal that reverse shocks in GRB photospheres stay radiation-mediated down to optical depths of a few tenths, with photons decoupling over a broad radial range and forming a quasi-thermal post-cursor.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
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A photospheric model calculates gamma-ray spectrum and energy from black-to-white hole transitions and estimates lunar-mass primordial black hole density.
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From Internal Collision to Photon Escape: First-Principles Modeling of Radiation-Mediated Shocks in Gamma-Ray Burst Photospheres
Self-consistent simulations reveal that reverse shocks in GRB photospheres stay radiation-mediated down to optical depths of a few tenths, with photons decoupling over a broad radial range and forming a quasi-thermal post-cursor.
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Electromagnetic emission from a black-to-white hole transition -- Photospheric emission
A photospheric model calculates gamma-ray spectrum and energy from black-to-white hole transitions and estimates lunar-mass primordial black hole density.