Pith

open record

sign in

arxiv: 1805.11559 · v3 · pith:IQZOBL54 · submitted 2018-05-29 · hep-th

A Note On Boundary Conditions In Euclidean Gravity

Reviewed by Pith T0 review T1 audit T2 compute T3 formal T4 reserved pith:IQZOBL54record.jsonopen to challenge →

classification hep-th
keywords boundaryconditionconditionscurvatureellipticeuclideanextrinsicgeneral
0
0 comments X
read the original abstract

We review what is known about boundary conditions in General Relativity on a spacetime of Euclidean signature. The obvious Dirichlet boundary condition, in which one specifies the boundary geometry, is actually not elliptic and in general does not lead to a well-defined perturbation theory. It is better-behaved if the extrinsic curvature of the boundary is suitably constrained, for instance if it is positive- or negative-definite. A different boundary condition, in which one specifies the conformal geometry of the boundary and the trace of the extrinsic curvature, is elliptic and always leads formally to a satisfactory perturbation theory. These facts might have interesting implications for semiclassical approaches to quantum gravity. (Submitted to a volume in honor of Roman Jackiw.)

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 9 Pith papers

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

  1. Holographic Tests of the $\mu$ Ensemble

    hep-th 2026-07 conditional novelty 7.0

    Fixed-μ ensemble computations in 11d supergravity reproduce ABJM partition functions (squashed S³, SCI, TTI) as Airy functions via a Laplace transform whose measure is fixed by bulk zero-mode counting.

  2. A Tale of Two Hartle-Hawking Wave Functions: Fully Gravitational vs Partially Frozen

    hep-th 2026-05 unverdicted novelty 7.0

    In AdS the fully gravitational Hartle-Hawking wave function acquires a nontrivial one-loop phase while the partially frozen version stays real and positive; a partially frozen de Sitter sphere shows phase cancellation.

  3. Quantum State of a Gravitating Region

    hep-th 2026-05 unverdicted novelty 6.0

    Proposal that compact d-manifolds with elliptic data prepare boundary quantum states |J>, with Rényi entropies from path integrals agreeing with minimal-surface formulas after analytic continuation.

  4. GR from RG, $2d$ Example: JT-Gravity Induced from Renormalization Group Flow

    hep-th 2026-05 unverdicted novelty 6.0

    Holographic RG flow on a 2D CFT induces JT gravity with bulk lapse as dilaton and recovers TTbar deformation in the Fefferman-Graham limit.

  5. Undulating Conformal Boundaries in 3D Gravity

    hep-th 2026-05 unverdicted novelty 6.0

    Inhomogeneous torus boundaries in 3D gravity are thermodynamically favourable for AdS in the range 2 < K |Λ|^{-1/2} < 3/√2 and support macroscopic entropy for all Λ.

  6. Deforming the Double-Scaled SYK & Reaching the Stretched Horizon From Finite Cutoff Holography

    hep-th 2026-02 unverdicted novelty 6.0

    Deformations of the double-scaled SYK model via finite-cutoff holography produce Krylov complexity as wormhole length and realize Susskind's stretched horizon proposal through targeted T² deformations in the high-ener...

  7. Timelike Liouville theory and AdS$_3$ gravity at finite cutoff

    hep-th 2025-08 unverdicted novelty 6.0

    Proposes that AdS3 gravity at finite cutoff is dual to a CFT2 coupled to timelike Liouville theory deformed by a marginal operator, with checks via semiclassical partition functions and EOM matching.

  8. On Black Holes Surrounded by Radiation II: Thermodynamics

    hep-th 2026-06 unverdicted novelty 5.0

    Hillingar black holes thermodynamically mimic ordinary black holes of mass M, sharing temperature and entropy under thermal equilibrium.

  9. Holographic pressure and volume for black holes

    hep-th 2026-02 unverdicted novelty 5.0

    Introduces a holographic pressure and volume for static spherically symmetric black holes via quasi-local thermodynamics, showing large black holes become extensive in the large-system limit while small ones do not.