Abstract

The present status of the quasi-local mass, energy-momentum and angular-momentum constructions in general relativity is reviewed. First, the general ideas, concepts, and strategies, as well as the necessary tools to construct and analyze the quasi-local quantities, are recalled. Then, the various specific constructions and their properties (both successes and deficiencies are discussed. Finally, some of the (actual and potential) applications of the quasi-local concepts and specific constructions are briefly mentioned.

Highlights

  • The present status of the quasi-local mass, energy-momentum and angular-momentum constructions in general relativity is reviewed

  • PSa and JSa b may be interpreted as the quasi-local energy-momentum and angular momentum of the matter fields associated with the spacelike two-surface S, or, equivalently, to D(Σ)

  • Let the spacetime be asymptotically flat at future null infinity in the sense of Penrose [413, 414, 415, 426], i.e., the physical spacetime can be conformally compactified by an appropriate boundary I +

Read more

Summary

December 2012

Recent developments of the field are included. A few subsections and more than fifty new references are added, minor improvements and corrections of the text are made at several points, and the bibliography is updated. Page 28: A new paragraph on a candidate for the total mass of closed universes is added. Page 50: A discussion of the monotonicity properties of the quasi-local mass expressions near spatial infinity, motivated by the compatibility with the post Newtonian limit is added. Page 51: A new paragraph on the incompatibility of the monotonicity of the quasi-local mass expressions and two ‘standard’ requirements is added. Page 102: New references on the initial boundary value problem and its potential connection with the quasi-local Hamiltonian approach are added. Page 103: The more detailed discussion of the role of the area 2-form (as a part of the boundary conditions) is given and new references are added. Page 118: A new paragraph on (and the reference to) a recent reformulation and its proof of Thorne’s hoop conjecture for spherically symmetric configurations is given. Page 123: A new Subsection 13.4.3 on a new entropy bound for uncollapsed bodies is added

Introduction
The symmetric energy-momentum tensor
Quasi-local energy-momentum and angular momentum of the matter fields
The definition of quasi-local quantities
Hamiltonian introduction of the quasi-local quantities
Properties of the quasi-local quantities
Global energy-momenta and angular momenta
The root of the difficulties
Pseudotensors
Strategies to avoid pseudotensors I
Strategies to avoid pseudotensors II
Strategies to avoid pseudotensors III
On the global energy-momentum and angular momentum of gravitating systems
Spatial infinity
Null infinity
Nonlocality of the gravitational energy-momentum and angular momentum
Domains for quasi-local quantities
Strategies to construct quasi-local quantities
Tools to Construct and Analyze Quasi-Local Quantities
The geometry of spacelike two-surfaces
The Lorentzian vector bundle
Connections
Embeddings and convexity conditions
The spinor bundle
Fabcd 2
Curvature identities
The GHP formalism
Irreducible parts of the derivative operators
Standard situations to evaluate the quasi-local quantities
Round spheres
Small surfaces
Large spheres near spatial infinity
Large spheres near null infinity
Other special situations
On lists of criteria of reasonableness of the quasi-local quantities
General expectations
Pragmatic criteria
Incompatibility of certain ‘natural’ expectations
The main idea
The computability of the Bartnik mass
Bray’s modifications
The definition
Hawking energy for spheres
Positivity and monotonicity properties
Two generalizations
Monotonicity properties
The Hayward energy
How do the twistors emerge?
Twistor space and the kinematical twistor
Two-surface twistors and the kinematical twistor
The Hamiltonian interpretation of the kinematical twistor
The Hermitian scalar product and the infinity twistor
The various limits
The quasi-local mass of specific two-surfaces
The modified constructions
The ‘improved’ construction with the determinant
Modification through Tod’s expression
Mason’s suggestions
Remarks on the validity of the construction
The Dougan–Mason constructions
The genericity of the generic two-surfaces
Positivity properties
A specific construction for the Kerr spacetime
Quasi-Local Spin Angular Momentum
The Ludvigsen–Vickers angular momentum
10 The Hamilton–Jacobi Method
10.1.1 The main idea
10.1.2 The variation of the action and the surface stress-energy tensor
10.1.3 The general form of the Brown–York quasi-local energy
10.1.4 Further properties of the general expressions
10.1.5 The Hamiltonians
10.1.6 The flat space and light cone references
10.1.7 Further properties and the various limits
10.1.8 Other prescriptions for the reference configuration
10.2.1 The role of the boundary conditions
10.3.1 The general form of Epp’s expression
10.3.2 The definition of the reference configuration
10.3.3 The various limits
10.4.1 The Liu–Yau definition
10.4.3 Generalizations of the original construction
10.5 The expression of Wang and Yau
11 Towards a Full Hamiltonian Approach
11.1.1 The quasi-local constraint algebra and the basic Hamiltonian
11.1.2 The two-surface observables
11.2 Approaches based on the double-null foliations
11.3.1 The covariant phase space methods
11.3.4 Covariant quasi-local Hamiltonians with general reference terms
11.3.5 Pseudotensors and quasi-local quantities
12.1 The Komar integral for spacetimes with Killing vectors
12.3.1 Tolman’s energy for static spacetimes
12.3.2 The Katz–Lynden-Bell–Israel energy for static spacetimes
12.3.3 Static spacetimes and post-Newtonian approximation
13 Applications in General Relativity
13.1 Calculation of tidal heating
13.2.1 On the Penrose inequality
13.2.2 On the hoop conjecture
13.2.3 On the Dain inequality
13.3.1 Quasi-local thermodynamics of black holes
13.3.2 On isolated and dynamic horizons
13.4.1 On Bekenstein’s bounds for the entropy
13.4.2 On the holographic hypothesis
13.4.3 Entropy bounds of Abreu and Visser for uncollapsed bodies
13.5 Quasi-local radiative modes of general relativity
13.6 Potential applications in cosmology
14.1 On the Bartnik mass and Hawking energy
14.2 On the Penrose mass
14.4 On the Brown–York–type expressions
15 Acknowledgments
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call