3D GRMHD simulations of accretion onto a JMN-1 horizonless singularity produce a magnetically arrested disk with an accretion rate of ~3e-6 Eddington matching M87* observations and EHT-consistent images, plus central brightness inside the shadow as a discriminant from black holes.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Inner-extremal regular black holes in polymerized LQG vacuum exist only for tuned masses and mass inflation is probed via null-shell collisions, with dependence on the minimal length scale.
citing papers explorer
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GRMHD accretion beyond the black hole paradigm: Light from within the shadow
3D GRMHD simulations of accretion onto a JMN-1 horizonless singularity produce a magnetically arrested disk with an accretion rate of ~3e-6 Eddington matching M87* observations and EHT-consistent images, plus central brightness inside the shadow as a discriminant from black holes.
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Probing mass inflation in polymerized vacuum regular black holes via colliding null shells
Inner-extremal regular black holes in polymerized LQG vacuum exist only for tuned masses and mass inflation is probed via null-shell collisions, with dependence on the minimal length scale.