Cited by 81Black Holes and Theoretical PhysicsRelativity and Gravitational TheoryGeometric Analysis and Curvature Flows

(2+1)-dimensional pure gravity for an arbitrary closed initial surface

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Hosoya, A, Nakao, K·1990·Classical and Quantum Gravity

Abstract

The (2+1)-dimensional pure Einstein gravity is studied in the ADM formalism. The authors solve the initial value and the time evolution problems with a closed Riemann surface being an initial surface, choosing the time slicing so that the trace of the extrinsic curvature is independent of spatial coordinates. The possible topology of the 2-surface is either a torus or a Riemann surface of genus g>or=2. It is shown that the moduli parameters of the torus follow the geodesic curve in the moduli space.

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Crossref · 10.1088/0264-9381/7/2/010

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  • The metric formalism can be used to give a full description of the solutions of the vacuum field equations, at least for spacetimes with topology R×Σ.

    “As Moncrief [206] and Hosoya and Nakao [159] have shown, this metric formalism can also be used to give a full description of the solutions of the vacuum field equations, at least for spacetimes with the topology ℝ × Σ.”

    From Quantum Gravity in 2 + 1 Dimensions: The Case of a Closed Universe (2005) · cites this paper as [159]

    The Introduction describes an ADM metric approach for vacuum spacetimes with topology Σ × ℝ, and the Summary says the authors have completely solved the classical equations. But the Summary also says they could not explicitly demonstrate the motion of the moduli in the general case, so the claim of a full description for all such spacetimes overstates what the paper establishes. (LLM, conf=0.82)

    Experimental — accuracy not yet measured
  • The semicircular curve is a geodesic in the natural Weil-Petersson (or Poincaré) metric on the torus moduli space.

    “Such a curve is a geodesic in the natural Weil-Petersson (or Poincaré) metric on the torus moduli space [159, 135].”

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Cites

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Research works printed but not linked: 4

  1. The topological Chern-Simons formulation is first given by Horowitz G T 1988 preprint NSF-ITP-88-178
  2. Arnowitt R, Deser S and Misner C W 1962 GraDitation ed L Witten (New York: Wiley)
  3. Farkas H M and Kra I 1980 Riemann Surfaces (Berlin: Springer)
  4. Achucarro A and Townsend P 1986 Phys. Lett. 180B 85 to a Hamiltonian system over Teichmuller space Yale preprint

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Authors
Hosoya, A., & Nakao, K.
Affiliations
Hiroshima University (JP)
Venue
Classical and Quantum Gravity
Published
1990-02-01
Volume
7
Issue
2
Pages
163-176
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2037306905
Cited by
81
References
1
Citations by year
2026: 1 · 2024: 1 · 2023: 2 · 2020: 5 · 2018: 1
FWCI
5.61
Type
journal article
Language
en
Open access
Locations
  • Classical and Quantum Gravity (publishedVersion)
  • Institutional Repositories DataBase (IRDB) (submittedVersion)
  • Tokyo Tech Research Repository (Tokyo Institute of Technology) (submittedVersion)
Funders
Aspen Center for Physics
Topics
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
  • Physical Sciences › Mathematics › Applied Mathematics › Geometric Analysis and Curvature Flows
Keywords
three-dimensional gravity, compact Riemann surfaces, initial value problems, time evolution, ADM formalism, extrinsic curvature, torus topology, moduli spaces, geodesic curves, higher genus surfaces

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