A phenomenological loop-quantum-gravity-inspired model resolves black hole singularities by creating a dynamical anti-trapped region that ejects all stellar mass as a stable outgoing solitary wave.
Particle Creation by Black Holes
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Universal compact entanglement islands are obstructed by an entropy bound violation, implying region-dependent interior reconstruction.
A spherically symmetric charged black hole evaporating via Hawking radiation can remain regular, with neither a singularity nor a Cauchy horizon, due to electromagnetic repulsion and energy-condition violation.
citing papers explorer
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Fuzzy-novae
A phenomenological loop-quantum-gravity-inspired model resolves black hole singularities by creating a dynamical anti-trapped region that ejects all stellar mass as a stable outgoing solitary wave.
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Entropy bound and the non-universality of entanglement islands
Universal compact entanglement islands are obstructed by an entropy bound violation, implying region-dependent interior reconstruction.
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Radiating black holes in general relativity need not be singular
A spherically symmetric charged black hole evaporating via Hawking radiation can remain regular, with neither a singularity nor a Cauchy horizon, due to electromagnetic repulsion and energy-condition violation.