Pith. sign in

Lashkari,Modular zero modes and sewing the states of QFT,JHEP21(2020) 189, [1911.11153]

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

3 Pith papers citing it

fields

hep-th 3

years

2025 2 2022 1

representative citing papers

An Algebra of Observables for de Sitter Space

hep-th · 2022-06-22 · accept · novelty 7.0

Defines a Type II₁ algebra of gravitationally dressed observables in de Sitter static patch whose entropy matches generalized entropy up to a state-independent additive constant.

Modular Witten Diagrams and Quantum Extremality

hep-th · 2025-12-12 · unverdicted · novelty 6.0

Modular Witten diagrams reproduce the O(λ² G_N) correction to holographic entanglement entropy, matching the canonical energy term in the quantum Ryu-Takayanagi formula with wedge shape deformation.

Covariant phase space and the semi-classical Einstein equation

hep-th · 2025-10-22 · unverdicted · novelty 6.0

A semi-classical symplectic two-form is defined as the sum of the gravitational symplectic form and the Berry curvature of the quantum matter state; it is shown to be independent of the Cauchy slice and to satisfy a quantum generalization of the Hollands-Iyer-Wald identity.

citing papers explorer

Showing 3 of 3 citing papers.

  • An Algebra of Observables for de Sitter Space hep-th · 2022-06-22 · accept · none · ref 48

    Defines a Type II₁ algebra of gravitationally dressed observables in de Sitter static patch whose entropy matches generalized entropy up to a state-independent additive constant.

  • Modular Witten Diagrams and Quantum Extremality hep-th · 2025-12-12 · unverdicted · none · ref 43

    Modular Witten diagrams reproduce the O(λ² G_N) correction to holographic entanglement entropy, matching the canonical energy term in the quantum Ryu-Takayanagi formula with wedge shape deformation.

  • Covariant phase space and the semi-classical Einstein equation hep-th · 2025-10-22 · unverdicted · none · ref 67

    A semi-classical symplectic two-form is defined as the sum of the gravitational symplectic form and the Berry curvature of the quantum matter state; it is shown to be independent of the Cauchy slice and to satisfy a quantum generalization of the Hollands-Iyer-Wald identity.