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.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
fields
gr-qc 4years
2026 4verdicts
UNVERDICTED 4representative citing papers
Derives exact charged black hole solutions in quasi-topological gravity with Born-Infeld electrodynamics, showing model-dependent regularity with some cases having finite-radius singularities and others replacing de Sitter cores with anti-de Sitter cores.
Regular ultracompact objects with anti-de Sitter cores arise as unique polymerized vacuum solutions in dust-deparameterized spherical symmetry from loop quantum gravity effective dynamics.
The primordial dark matter scale suppresses Hawking temperature and spectral energy emission rate relative to Schwarzschild while the heat capacity stays negative and the sparsity parameter receives a small negative correction.
citing papers explorer
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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.
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Charged Black Holes in Quasi-Topological Gravity Coupled to Born-Infeld Nonlinear Electrodynamics
Derives exact charged black hole solutions in quasi-topological gravity with Born-Infeld electrodynamics, showing model-dependent regularity with some cases having finite-radius singularities and others replacing de Sitter cores with anti-de Sitter cores.
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Regular ultracompact objects with anti-de Sitter cores as polymerized vacuum solutions
Regular ultracompact objects with anti-de Sitter cores arise as unique polymerized vacuum solutions in dust-deparameterized spherical symmetry from loop quantum gravity effective dynamics.
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Hawking Temperature, Sparsity and Energy Emission Rate of Regular Black Holes Supported by Primordial Dark Matter
The primordial dark matter scale suppresses Hawking temperature and spectral energy emission rate relative to Schwarzschild while the heat capacity stays negative and the sparsity parameter receives a small negative correction.