Haar random qubit states show vanishing fermionic non-Gaussianity for subsystems smaller than half the total size without symmetry, small but finite non-Gaussianity with U(1) symmetry, and extensive non-Gaussianity for larger subsystems.
Entanglement Wedge Reconstruction and the Information Paradox
6 Pith papers cite this work. Polarity classification is still indexing.
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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.
In the microcanonical ensemble for additive bipartite systems, entanglement capacity is governed by energy-sharing fluctuations and yields a Page-like curve in a Schwarzian black hole plus CFT radiation toy model.
A new action for entanglement entropy in AdS3/CFT2 derives gravity equations, reduces to a string worldsheet, reproduces bit threads, and unifies several quantum gravity conjectures.
The bounded discrete thermal weight suppresses black-hole Hawking luminosity near the cutoff and supports an exact Jarzynski identity for work but not a simple Crooks relation.
Krylov complexity is a canonical, parameter-independent measure of operator spreading that probes chaotic dynamics to late times and admits a geometric interpretation in holographic duals.
citing papers explorer
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Non-Gaussianity of random quantum states
Haar random qubit states show vanishing fermionic non-Gaussianity for subsystems smaller than half the total size without symmetry, small but finite non-Gaussianity with U(1) symmetry, and extensive non-Gaussianity for larger subsystems.
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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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Microcanonical Energy Sharing and a Page-like Curve for the Capacity of Entanglement
In the microcanonical ensemble for additive bipartite systems, entanglement capacity is governed by energy-sharing fluctuations and yields a Page-like curve in a Schwarzian black hole plus CFT radiation toy model.
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Toward a worldsheet theory of entanglement entropy
A new action for entanglement entropy in AdS3/CFT2 derives gravity equations, reduces to a string worldsheet, reproduces bit threads, and unifies several quantum gravity conjectures.
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Bounded thermal weights from a discrete Boltzmann factor
The bounded discrete thermal weight suppresses black-hole Hawking luminosity near the cutoff and supports an exact Jarzynski identity for work but not a simple Crooks relation.
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Krylov Complexity
Krylov complexity is a canonical, parameter-independent measure of operator spreading that probes chaotic dynamics to late times and admits a geometric interpretation in holographic duals.