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Witten,Why does quantum field theory in curved spacetime make sense? And what happens to the algebra of observables in the thermodynamic limit?2022.arXiv:2112.11614 [hep-th]

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it

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hep-th 4

years

2026 4

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UNVERDICTED 4

representative citing papers

Carrollian quantum states and flat space holography

hep-th · 2026-04-24 · unverdicted · novelty 7.0

Carrollian QFTs from scalar limits admit regular invariant vacua and KMS states only in the massive electric sector; a factorizing quasifree state is constructed for flat-space holography isolating nonseparable zero modes.

Excitability in quantum field theory

hep-th · 2026-04-21 · unverdicted · novelty 6.0

For zero-mean Gaussian states in generalized free field theories, one-way local excitability always implies two-way excitability, generalizing the quasiequivalence theorems of Powers, Stormer, van Daele, Araki, and Yamagami.

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Showing 4 of 4 citing papers.

  • Carrollian quantum states and flat space holography hep-th · 2026-04-24 · unverdicted · none · ref 47

    Carrollian QFTs from scalar limits admit regular invariant vacua and KMS states only in the massive electric sector; a factorizing quasifree state is constructed for flat-space holography isolating nonseparable zero modes.

  • Excitability in quantum field theory hep-th · 2026-04-21 · unverdicted · none · ref 10

    For zero-mean Gaussian states in generalized free field theories, one-way local excitability always implies two-way excitability, generalizing the quasiequivalence theorems of Powers, Stormer, van Daele, Araki, and Yamagami.

  • Real-Time Quantum Dynamics on the Fuzzy Sphere: Chaos and Entanglement hep-th · 2026-05-07 · unverdicted · none · ref 47

    In this fuzzy-sphere matrix model the largest Lyapunov exponent drops to zero at finite temperature, respecting the Maldacena-Shenker-Stanford bound while entanglement shows fast scrambling.

  • Implication of dressed form of relational observable on von Neumann algebra hep-th · 2026-03-27 · unverdicted · none · ref 49

    Dressed relational observables imply quasi-de Sitter space corresponds to Type II_∞ von Neumann algebra with diverging trace in the gravity decoupling limit, unlike the finite-trace Type II_1 algebra for de Sitter space.