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Modular Hamiltonians for Euclidean Path Integral States

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arxiv 2002.00018 v1 pith:DYTDOPNT submitted 2020-01-31 hep-th

classification hep-th
keywords modulareuclideanformulahamiltoniansintegrallocalnulloperators
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We study half-space/Rindler modular Hamiltonians for excited states created by turning on sources for local operators in the Euclidean path integral in relativistic quantum field theories. We derive a simple, manifestly Lorentzian formula for the modular Hamiltonian to all orders in perturbation theory in the sources. We apply this formula to the case of shape-deformed half spaces in the vacuum state, and obtain the corresponding modular Hamiltonian to all orders in the shape deformation in terms of products of half-sided null energy operators, i.e., stress tensor components integrated along the future and past Rindler horizons. In the special case where the shape deformation is purely null, our perturbation series can be resummed, and agrees precisely with the known formula for vacuum modular Hamiltonians for null cuts of the Rindler horizon. Finally, we study some universal properties of modular flow (corresponding to Euclidean path integral states) of local operators inside correlation functions in conformal field theories. In particular, we show how the flow becomes the local boost in the limit where the operator being flowed approaches the entanglement cut.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Holographic Ordering and Negative entropy in Non-equilibrium Euclidean Black Hole Path Integralsl

    hep-th 2025-07 reject novelty 4.0 of 10

    Gravitational attraction is presented as the gradient of a negative entropy deficit, equal to the red-shifted shell energy divided by Hawking temperature, applied to a black hole with a static thin shell.

  2. Correlation functions of von Neumann entropy

    hep-th 2025-06 conditional novelty 4.0 of 10

    Two-point correlators of modular Hamiltonians obey entropy-like properties and equal the stress-tensor conformal block for spherical regions in CFT, including imaginary-time separations.

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