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.
Fate of quantum black holes
2 Pith papers cite this work. Polarity classification is still indexing.
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gr-qc 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Algebraic equations from Hamiltonian constraints on vacuum spherically symmetric metrics describe non-homogeneous dust collapse and bounce, applied to quantum-inspired models to recover or find new bounce results.
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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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Dust collapse and bounce in spherically symmetric quantum-inspired gravity models
Algebraic equations from Hamiltonian constraints on vacuum spherically symmetric metrics describe non-homogeneous dust collapse and bounce, applied to quantum-inspired models to recover or find new bounce results.