A photospheric model calculates gamma-ray spectrum and energy from black-to-white hole transitions and estimates lunar-mass primordial black hole density.
Electromagnetic emission from a black-to-white hole transition -- Photospheric emission
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abstract
We calculate the gamma ray emission from a black-to-white hole transition. We put forward a model for the prompt emission phase, based on the photospheric emission model with the underlying idea that the number of photons and leptons emitted by the white hole will be larger than the baryon content. We calculate the spectrum of the emitted radiation and give an estimate of the total energy emitted. Finally, we estimate the cosmological density of lunar mass primordial black holes.
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gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
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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.