Stress-energy tensor of quantized massive scalar fields in thermal states on zero-tidal wormholes satisfies Morris-Thorne conditions only for bounded masses and temperatures below a mass-dependent critical value.
Notes on black hole evaporation
8 Pith papers cite this work. Polarity classification is still indexing.
8
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
years
2026 8verdicts
UNVERDICTED 8roles
background 2polarities
background 2representative citing papers
Introduces a universal dimensionless instability parameter based on quantum-state evolution speed versus spectral-gap protection, plus a self-limitation theorem for nonlinear regulators in driven quantum systems.
The Newton-Cartan limit of Klein-Gordon AQFT on static spacetimes produces Galilean Haag-Kastler nets without Reeh-Schlieder property or modular flow on local algebras, with the field mass as Bargmann central charge.
Post-selection on a Chern-Simons soliton in minisuperspace quantum cosmology yields an accelerating trajectory from a free radiation Hamiltonian with zero cosmological constant.
Semiclassical black hole evaporation in four dimensions produces a thunderbolt singularity signaling breakdown of the effective theory at large distances.
A black hole can be converted into a visible quantum system of D-branes and strings by moving it slowly through a suitably chosen varying-dilaton background that avoids adiabatic breakdown, spacetime collapse, and premature evaporation.
Generalizes Verlinde-van der Heijden protocol to type III factors in QFT, yielding thermodynamic interpretation and charge quantization via index-statistics theorem.
Radiation from hyperbolic motion escapes the Rindler wedge with zero flux at infinity inside it in both frames.
citing papers explorer
-
Stress-energy tensor of quantized scalar fields in thermal states on a zero-tidal wormhole
Stress-energy tensor of quantized massive scalar fields in thermal states on zero-tidal wormholes satisfies Morris-Thorne conditions only for bounded masses and temperatures below a mass-dependent critical value.
-
Geometric Instability and Self-Limitation in Driven Quantum Systems
Introduces a universal dimensionless instability parameter based on quantum-state evolution speed versus spectral-gap protection, plus a self-limitation theorem for nonlinear regulators in driven quantum systems.
-
Newton-Cartan limit of Klein-Gordon AQFT and the collapse of Galilean modular structure
The Newton-Cartan limit of Klein-Gordon AQFT on static spacetimes produces Galilean Haag-Kastler nets without Reeh-Schlieder property or modular flow on local algebras, with the field mass as Bargmann central charge.
-
Teleocosmology and quantum post-selection
Post-selection on a Chern-Simons soliton in minisuperspace quantum cosmology yields an accelerating trajectory from a free radiation Hamiltonian with zero cosmological constant.
-
Breakdown of Semiclassical Gravity in Four-Dimensional Black Hole Evaporation
Semiclassical black hole evaporation in four dimensions produces a thunderbolt singularity signaling breakdown of the effective theory at large distances.
-
How to Expose a Black Hole
A black hole can be converted into a visible quantum system of D-branes and strings by moving it slowly through a suitably chosen varying-dilaton background that avoids adiabatic breakdown, spacetime collapse, and premature evaporation.
-
A QFT information protocol for charged black holes
Generalizes Verlinde-van der Heijden protocol to type III factors in QFT, yielding thermodynamic interpretation and charge quantization via index-statistics theorem.
-
On radiation from hyperbolic motion, behavior of electromagnetic fields, and coordinate transformations at infinity
Radiation from hyperbolic motion escapes the Rindler wedge with zero flux at infinity inside it in both frames.