A new singularity theorem establishes that evaporating black holes in semiclassical gravity are singular under weaker causality assumptions and the Generalized Second Law.
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7 Pith papers cite this work. Polarity classification is still indexing.
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An Unruh-DeWitt detector interacting with a position-superposed BTZ black hole produces outcome probabilities containing a nonclassical contribution that distinguishes quantum superposition from classical mixtures, arising from singularities in the probed spectrum.
Many-body localization protects emergent holographic geometry in random tensor networks by preserving spatial entanglement structure against thermalization.
Wormhole throat area is monotonically non-increasing under NEC matter after ANEC opening, implying Q_max ≤ A_min/4G_N as a geometric bound on transmissible qubits via bit-thread max-flow.
In charged AdS black holes, the topological number W changes at a boundary membership event τ_a, while the branch response C_par diverges at a separate turning point τ_b, because the two diagnostics track different local structures of the same zero point curve.
Greybody lower bounds and absorption cross sections for massless fields of spins 0, 1, and 1/2 are computed in the Euler-Heisenberg black hole with perfect fluid dark matter, revealing monotonic increases with frequency and parameter-dependent deformations of the spectra.
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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A Quantum Singularity Theorem for the Evaporating Black Hole
A new singularity theorem establishes that evaporating black holes in semiclassical gravity are singular under weaker causality assumptions and the Generalized Second Law.
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Particle detector in a position-superposed black hole spacetime
An Unruh-DeWitt detector interacting with a position-superposed BTZ black hole produces outcome probabilities containing a nonclassical contribution that distinguishes quantum superposition from classical mixtures, arising from singularities in the probed spectrum.
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Breaking the Entanglement-Structure Trade-off: Many-Body Localization Protects Emergent Holographic Geometry in Random Tensor Networks
Many-body localization protects emergent holographic geometry in random tensor networks by preserving spatial entanglement structure against thermalization.
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Area Monotonicity of Wormhole Throats and a Geometric Bound on Information Transfer
Wormhole throat area is monotonically non-increasing under NEC matter after ANEC opening, implying Q_max ≤ A_min/4G_N as a geometric bound on transmissible qubits via bit-thread max-flow.
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Topological changes and response singularities in black hole thermodynamic branch structure
In charged AdS black holes, the topological number W changes at a boundary membership event τ_a, while the branch response C_par diverges at a separate turning point τ_b, because the two diagnostics track different local structures of the same zero point curve.
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Perturbations and greybody bounds of Euler-Heisenberg black holes surrounded by perfect fluid dark matter
Greybody lower bounds and absorption cross sections for massless fields of spins 0, 1, and 1/2 are computed in the Euler-Heisenberg black hole with perfect fluid dark matter, revealing monotonic increases with frequency and parameter-dependent deformations of the spectra.
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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.