activity
20232025
most citedNull states and time evolution in a toy model of black hole dynamics

3 citations · 7 across the 6 of their papers we have counts for

collaborators

6 papers

hep-th2025

Are wormholes generic with large sources?

Xiaoyi Liu, Donald Marolf, Jorge E. Santos

Euclidean path integrals can be used to prepare states of a Lorentzian QFT. So long as any sources are turned off on the surface, the resulting Lorentzian states all belong t…

gr-qc2025★ 1 cited

Ill-posedness of the Cauchy problem for linearized gravity in a cavity with conformal boundary conditions

Xiaoyi Liu, Harvey S. Reall, Jorge E. Santos +1

We consider Lorentzian General Relativity in a cavity with a timelike boundary, with conformal boundary conditions and also a generalization of these boundary conditions. We focus…

hep-th2024★ 1 cited

Euclidean and complex geometries from real-time computations of gravitational Rényi entropies

Jesse Held, Xiaoyi Liu, Donald Marolf +1

Gravitational Rényi computations have traditionally been described in the language of Euclidean path integrals. In the semiclassical limit, such calculations are governed by Euclid…

hep-th2024★ 3 cited

Null states and time evolution in a toy model of black hole dynamics

Xi Dong, Maciej Kolanowski, Xiaoyi Liu +2

Spacetime wormholes can provide non-perturbative contributions to the gravitational path integral that make the actual number of states in a gravitational system much smaller…

hep-th2024★ 2 cited

New Well-Posed Boundary Conditions for Semi-Classical Euclidean Gravity

Xiaoyi Liu, Jorge E. Santos, Toby Wiseman

We consider four-dimensional Euclidean gravity in a finite cavity. Dirichlet conditions do not yield a well-posed elliptic system, and Anderson has suggested boundary conditions th…

hep-th2023

Stability of saddles and choices of contour in the Euclidean path integral for linearized gravity: Dependence on the DeWitt Parameter

Xiaoyi Liu, Donald Marolf, Jorge E. Santos

Due to the conformal factor problem, the definition of the Euclidean gravitational path integral requires a non-trivial choice of contour. The present work examines a generalizatio…