The reduced Hamiltonian of general relativity and the σ-constant of conformal geometry

被引:0
|
作者
Fischer, AE [1 ]
Moncrief, V [1 ]
机构
[1] Univ Calif Santa Cruz, Dept Math, Santa Cruz, CA 95064 USA
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 H-reduced : R- X P-reduced -> R where the reduced Hamiltonian is given by H-reduced(tau,gamma ,p(TT)) = -tau (3) integral (M) phi (6) mu (gamma) = -tau (3) integral (M) mug = -tau (3)vol(M,g). For compact connected oriented 3-manifolds of Yamabe type -1, we establish the following properties for this reduced system: 1. H-reduced(tau,gamma ,p(TT)) is a monotonically decreasing function of t unless p(TT) = 0 and gamma = <(<gamma>)over bar> is hyperbolic, at which point H-reduced(tau, <(<gamma>)over tilde>, 0) is constant in time. 2. For tau epsilon R- fixed, H-reduced(tau,gamma ,p(TT)) has a unique (up to isometry) critical point at (<(<gamma>)over tilde>, 0) which is a strict local minimum tin the non-isometric directions). 3. For tau epsilon R- fixed, the sigma -constant of M is related to H-reduced by sigma (M) = -1/2 (((gamma ,pTT)epsilon Preduced) inf H-reduced (tau,gamma ,p(TT)))(2/3). If M is a hyperbolic manifold, then we conjecture that (<(<gamma>)over tilde>, 0) is a strict global minimum of H-reduced(tau,gamma ,p(TT)) which, as part of our work, is equivalent to the conjecture that the sigma -constant of M is realized by the unique hyperbolic geometry on M. If M is not a hyperbolic manifold, then the sigma -constant is never realized by a metric on M but is only approached as a limit. In this case, the Einstein flow seeks to attain the sigma -constant asymptotically insofar as the reduced Hamiltonian is monotonically seeking to decay to its infimum, although possible obstructions, such as the formation of black holes, may prevent any particular solution from approaching the sigma -constant asymptotically. Further applications and developments in higher dimensions are discussed.
引用
下载
收藏
页码:70 / 101
页数:32
相关论文
共 50 条
  • [21] Hamiltonian analysis in new general relativity
    Blixt, Daniel
    Hohmann, Manuel
    Krssak, Martin
    Pfeifer, Christian
    15TH MARCEL GROSSMANN MEETING, PT A, 2022, : 352 - 357
  • [22] Conformal and projective structures in general relativity
    John Stachel
    General Relativity and Gravitation, 2011, 43 : 3399 - 3409
  • [23] CONFORMAL GROUPS IN GENERAL-RELATIVITY
    BRAY, M
    ANNALES DE L INSTITUT HENRI POINCARE SECTION A PHYSIQUE THEORIQUE, 1979, 30 (03): : 231 - 250
  • [24] Hyperbolicity of Hamiltonian formulations in General Relativity
    Richter, Ronny
    Hilditch, David
    SPANISH RELATIVITY MEETING (ERE 2010): GRAVITY AS A CROSSROAD IN PHYSICS, 2011, 314
  • [25] CONFORMAL GEODESICS IN GENERAL-RELATIVITY
    FRIEDRICH, H
    SCHMIDT, BG
    PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 1987, 414 (1846): : 171 - 195
  • [26] CONFORMAL CHANGES OF METRICS IN GENERAL RELATIVITY
    MIELKE, EW
    BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1974, 19 (04): : 508 - 509
  • [27] Polynomial Hamiltonian form of general relativity
    Katanaev, M. O.
    THEORETICAL AND MATHEMATICAL PHYSICS, 2006, 148 (03) : 1264 - 1294
  • [28] Emergent Time in Hamiltonian General Relativity
    Kaushal, Anurag
    Prabhakar, Naveen S.
    Wadia, Spenta R.
    arXiv,
  • [29] COVARIANT HAMILTONIAN EQUATIONS IN GENERAL RELATIVITY
    ROCHE, C
    ANNALES DE L INSTITUT HENRI POINCARE SECTION A PHYSIQUE THEORIQUE, 1969, 10 (03): : 271 - &
  • [30] Polynomial Hamiltonian form of general relativity
    M. O. Katanaev
    Theoretical and Mathematical Physics, 2006, 148 : 1264 - 1294