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Student Number 91222014
Author Gang Sun(孫綱)
Author's Email Address No Public.
Statistics This thesis had been viewed 1710 times. Download 680 times.
Department Physics
Year 2004
Semester 2
Degree Master
Type of Document Master's Thesis
Language English
Title Quasilocal Conserved Quantities For General Relativity In Small Regions
Date of Defense 2005-06-21
Page Count 60
Keyword
  • quasilocal
  • small region limit
  • Abstract  Gravitational energy has been a concern for a long time. There are several ways to deal with the problem, but the best way is the quasilocal approach. The NCU group has been developing their quasilocal approach – the covariant Hamiltonian formalism, and has obtained good results for spatial and null infinity. In addition to these infinite cases; there is another limit case – the small region limit. The small region vacuum limit provides an important test of the quasilocal expression. Whereas the large scale asymptotic limit tests only the weak field linearized part of the expression, the small scale vacuum limit probes the next order non-linear part.
     In this thesis the purpose is to test the covariant Hamiltonian formalism in the small region limit. In the first chapter, we will introduce the basic ideas of the quasilocal method and some related ideas. In chapter two, we will show the readers what the covariant Hamiltonian formulism is and how to derive it. In the chapter three, we will introduce some general concepts about energy-momentum, angular momentum and center-of-mass moment, and the relation between these physical quantities and conservation. In the next chapter, the detailed procedure on how to get quasilocal values in the small region limit, including the vacuum case and matter case, using covariant Hamiltonian formulism will follow. In the final chapter, we will discuss the meaning of our results and conclude that only one of the four covariant Hamiltonian expressions gives positive energy in the first non-linear order. Finally we will comment some deficiencies.
    Table of Content Contents
    Chapter 1
    Introduction                              1
    1.1 Fundamental concepts of quasilocal                 1
    1.2 Some applications of quasilocal                   2
    1.2.1 Tidal heating                           2
    1.2.2 Positivity of the gravitational energy in the finite region    3
    1.2.3 The ADM mass and the (weak) cosmic censorship hypothesis     3
    Chapter 2                                4
    Covariant symplectic quasilocal expression               4
    2.1 From Lagrangian to Hamiltonian                   4
    2.2 Control over the Hamiltonian boundary term             6
    2.3 The choice of evolving vector                    9
    2.3.1 Asymptotically                          9
    2.3.2 In the small region                        12
    Chapter 3                                14
    Physical quantities and conservation                  14
    3.1 Physical quantities in special relativity              14
    3.1.1 Single particle                          14
    3.1.2 Matter field                           15
    3.2 Conservation Law and Noether theorem                16
    3.2.1 Killing vector field                       16  
    3.2.2 Noether theorem                          17
    3.2.3 Conservation quantities in Minkowski space            18
    3.3 Total conservation for a gravitational field            19
    3.3.1 Pseudotensor                           19
    3.3.2 Our quasilocal approach                      20
    Chapter 4                                21
    Quasilocal quantities in small region                  21
    4.1 Riemann normal coordinates                     21
    4.2 The expansion of the Hamiltonian in the small region        23
    4.3 The quasilocal values expressed by the different unit volume    32
    4.4 The values of the four quasilocal cases               36
    4.4.1 The four cases expressed by the physical volume element      36
    4.4.2 The four cases expressed by the flat volume element        38
    Chapter 5                                41
    Discussion                               41
    5.1 Discussion to the results including a matter field         41
    5.2 Discussion to those results concerning the vacuum          41
    5.2.1 The physical quantities in the small region            41
    5.2.2 Some comments on our quasilocal values in vacuum         46
    5.3 Conclusion                             50
    Reference                              53
    Appendix A                               55
    Bel-Robinson tensor and quadratic forms in Riemann curvature      55
    A.1 The definition of the Bel-Robinson tensor              55
    A.2 The relationship between the Bel-Robinson tensor and energy in a small region                                 58
    A.3 Quadratic form in Riemann curvature                 59
    Reference References
    [1] C. C. M “Quasilocal Quantities for Gravity Theories”, MSc. Thesis (National Central University, Chung-li) 1994, unpublished.
    [2] C. M. Chen, J. M. Nester and R. S. Tung, “Quasilocal Energy-Momentum for Geometric Gravity Theories”, Phys.Lett. 203A, 5-11 (1995), or gr-qc/9411048.
    [3] C. M. Chen and J. M. Nester, “Quasilocal quantities for GR and other gravity theories”, Class.Quant.Grav. 16 (1999) 1279-1304, or gr-qc/9809020.
    [4] C. C. Chang, “The Localization of Gravitational Energy: Pseudotensors and Quasilocal Expressions”, MSc. Thesis (National Central University, Chung-li) 1999, unpublished.
    [5] Dougan, A.J., and Mason, L.J., “Quasi-local mass constructions with positive energy”, Phys. Rev. Lett., 67, 2119-2122, (1991).
    [6] F. H. Ho, “Quasilocal Center-of-Mass for GR||”, MSc. Thesis (National Central University, Chung-li) 2003, unpublished.
    [7] Ivan S. Booth, Jolien D. E. Creighton, “A quasilocal calculation of tidal heating”, Phys.Rev. D62 (2000) 067503.
    [8] James M Nester, “General pseudotensors and quasilocal quantities”, Class. Quantum Grav. 21 No 3 (2004) S261-S280.
    [9]. K. H. Vu, “Quasilocal Energy-Momentum and Angular Momentum for Teleparallel Gravity”, MSc. Thesis (National Central University, Chung-li) 2000, unpublished.
    [10] Liu, C.-C.M, and Yau, S.-T., “Positivity of quasilocal mass”, Phys. Rev. Lett., 90, 231102-1-4, (2003) or http://www.arxiv.org/abs/gr-qc/0303019v2
    [11] L. B. Szabados, “Quasi-Local Energy-Momentum and Angular Momentum in GR: A Review Article”, http://www.livingreviews.org/lrr-2004-4.
    [12] Liang Canbin, “微分幾何入門與廣義相對論” (北京師範大學出版社) 2000.
    [13] Ludvigsen, M., and Vickers, J.A.G., “Momentum, Angular momentum and their quasi-local null surface extensions”, J. Phys. A, 16, 1155-1168, (1983).
    [14] L.L. So’ thesis in preparation (2005), NCU
    [15] Misner C W, Thorne K S and Wheeler J A, “Gravitation” (San Francisco: Freeman) 1973.
    [16] Marc Favata, “Energy Localization Invariance of Tidal Work in General Relativity”, Phys.Rev. D63 (2001) 064013.
    [17] Patricia Purdue, “The gauge invariance of general relativistic tidal heating”, Phys.Rev. D60 (1999) 104054.
    [18] R. M. Wald, “General Relativity” (The University of Chicago Press) 1984.
    [19] S. Deser, J.S. Franklin, D. Seminara, “Graviton-Graviton Scattering, Bel-Robinson and Energy (Pseudo)-Tensors”, Class.Quant.Grav. 16 (1999) 2815-2821, or gr-qc/9905021
    [20] Shi, Y., and Tam, L.-F., “Positive mass theorem and the boundary behaviors of compact manifolds with nonnegative scalar curvature”, J. Differ. Geom., 62, 79-125, (2002) or http://arxiv.org/abs/math.DG/0301047v1
    [21] Janusz Garecki, “Some remarks on the Bel-Robinson Tensor”, Annalen Phys. 10 (2001) 911-919, or gr-qc/0003006.
    Advisor
  • J. Nester(聶斯特)
  • Files
  • 91222014.pdf
  • approve immediately
    Date of Submission 2005-07-21

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