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.
Notes on black hole evaporation
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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.
citing papers explorer
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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.
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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.
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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.
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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.