Cited by 22Geometric Analysis and Curvature FlowsAdvanced Differential Geometry ResearchRelativity and Gravitational Theory

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The Einstein flow, the sigma-constant and the geometrization of 3-manifolds

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Fischer, Arthur E, Moncrief, Vincent·1999·Classical and Quantum Gravity

Abstract

For the problem of the Hamiltonian reduction of Einstein's equations on a (3 + 1) vacuum spacetime that admits a foliation by constant mean curvature (CMC) compact spacelike hypersurfaces M that satisfy certain topological restrictions, we introduce a dimensionless non-local time-dependent reduced Hamiltonian system where and P reduced is the reduced phase space. For this system, we establish the following properties: (1) H reduced has a unique critical point at the hyperbolic point which is a strict local minimum; (2) H reduced is a strictly monotonically decreasing function along the Einstein flow unless , in which case H reduced is constant in time; and (3) the infimum of H reduced is related to the -constant of M by Further applications and developments relating the Einstein flow to ( M ) and to the geometrization conjecture for 3-manifolds are discussed.

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Crossref · 10.1088/0264-9381/16/11/102

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  • [12] proved a global existence theorem for expanding solutions in the same gauge by controlling the Dirichlet energy of an associated harmonic map for any τ in (-∞,0).

    “In addition to the local well-posedness, [12] proved a global existence theorem for the expanding solutions in the same gauge by controlling the Dirichlet energy of an associated harmonic map for any τ ∈ ( -∞ , 0) .”

    From Big-bang limit of 2 + 1 gravity and Thurston boundary of Teichmüller space (2023) · cites this paper as [12]

    The Letter to the Editor describes τ ∈ (−∞, 0) as the expected maximal range, not a range established by a global-existence theorem. Section 5.1 discusses long-time existence as a potential future application. Searches for Dirichlet energy, harmonic maps, and a global-existence theorem found no passage establishing the attributed result. (LLM, conf=0.76)

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  • In(τ) and S(τ) are continuous functions of τ by existence-uniqueness-continuity (well-posedness) of Einstein's equations.

    “Both I n ( τ ) and S ( τ ) are continuous functions of τ by existence-uniqueness-continuity (or well-posedness) of the Einstein's equations [12].”

    From Big-bang limit of 2 + 1 gravity and Thurston boundary of Teichmüller space (2023) · cites this paper as [12]

    The Letter to the Editor defines a time-dependent Hamiltonian in terms of τ, and section 4 discusses its infimum, but neither passage identifies I_n(τ) or S(τ) or establishes their continuity. Searches for those functions and for well-posedness, existence, uniqueness, and continuous dependence found no passage making the attributed argument. (LLM, conf=0.74)

    Experimental — accuracy not yet measured

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Research works printed but not linked: 7

  1. 10.1016/S0920-5632(97)00363-0 · DOI · Paper page
  2. 10.1063/1.528475 · DOI · Paper page
  3. Löbell F, 1931, Ber. Verhandl. Sächs. Akad. Wiss. Leipzig, Math. Phys. Kl., 83, 167
  4. Eardley D, 1986, Commun. Math. Phys., 106, 137, 10.1007/BF01210929 · DOI
  5. Hamilton R, 1982, J. Diff. Geom., 17, 255, 10.4310/jdg/1214436922 · DOI
  6. Hamilton R, 1999, Commun. Anal. Geom., 7, 695, 10.4310/CAG.1999.v7.n4.a2 · DOI
  7. 10.1090/S0273-0979-99-00773-9 · DOI

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Metadata

Authors
Fischer, A. E., & Moncrief, V.
Affiliations
  • University of California, Santa Cruz (US)
  • Yale University (US)
Venue
Classical and Quantum Gravity
Published
1999-10-08
Volume
16
Issue
11
Pages
L79-L87
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2057406392
Cited by
22
References
0
Citations by year
2025: 1 · 2023: 1 · 2015: 1
FWCI
6.11
Type
journal article
Language
en
Open access
Locations
Classical and Quantum Gravity (publishedVersion)
Topics
  • Physical Sciences › Mathematics › Applied Mathematics › Geometric Analysis and Curvature Flows
  • Physical Sciences › Mathematics › Geometry and Topology › Advanced Differential Geometry Research
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
Keywords
sigma constants, Hamiltonian reduction, vacuum Einstein equations, constant mean curvature hypersurfaces, spacelike hypersurfaces, geometrization conjecture, critical point analysis, hyperbolic geometry

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