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Hamiltonian Field Theory in the Radiating Regime 2002 ed. [Kietas viršelis]

  • Formatas: Hardback, 174 pages, aukštis x plotis: 235x155 mm, weight: 970 g, VI, 174 p., 1 Hardback
  • Serija: Lecture Notes in Physics Monographs 70
  • Išleidimo metai: 04-Dec-2001
  • Leidėjas: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3540428844
  • ISBN-13: 9783540428848
Kitos knygos pagal šią temą:
  • Formatas: Hardback, 174 pages, aukštis x plotis: 235x155 mm, weight: 970 g, VI, 174 p., 1 Hardback
  • Serija: Lecture Notes in Physics Monographs 70
  • Išleidimo metai: 04-Dec-2001
  • Leidėjas: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3540428844
  • ISBN-13: 9783540428848
Kitos knygos pagal šią temą:
In one ofthe fundamental notions is that any physical theory of of energy the hand: in mechanics at one considers the objects energy of, say, moving in fieldtheories is one interested inthe offield masses; energy configurations. A unified treatment of this which both to mechanics question, applies and to field Hamiltonian a formalism. We will theory, proceeds through shortly reviewbelowhowsuch iscarried aprocedure out inthe ofscalarfields theory Minkowski let at this on mention that an space time; us, stage, important often inthe isthat ofthe issue, ignored conditions sat textbooks, boundary isfied the set of fields under consideration. While by this issuecanbe safely for when the ignored usual field many purposes considering theories, such scalar fields or the = as on electromagnetism, ft constj hypersurfaces, where t is a it sometimes critical Minkowski time, a rolewhen other plays of classes are considered. Inthe of the hypersurfaces case situation is gravity for t= worse: even Minkowskian slicesthe f constj asymptotically boundary terms crucial. is ofthe are one main differencesbetweentheArnowitt (This Deser Misner for Sect. 5. 4 mass which is (ADM) gravity (cf. below), given a andthe usual for by boundary integral, field theories in energyexpression Minkowski wheretheHamiltonian is volume space time, a usually integral. ) in field the itsmost role in Now, theory plays important theradiation energy where it can be radiated the field.

Recenzijos

"The text is addressed to physicists and is not written in theorem-proof style, nor are the function spaces introduced equipped with explicit topologies and differentiable structures. However, all concepts are very carefully defined and necessary deviations from a rigorous treatment are clearly identified." (Mathematical Reviews 2003f)



"This monograph gives a comprehensive overview about Hamiltonian field theory with main application to the Einstein field equation. [ ...] Carefully prepared appendices and bibliography close this very readable book." (Zentralblatt MATH, 1002/02, 2003)

Introduction
1(6)
Preliminaries
7(16)
Hamiltonian dynamics
7(3)
The role of boundary conditions in Hamiltonian field theory
10(3)
Tangential translations as a Hamiltonian system
13(2)
The Hamiltonian description of a mixed Cauchy - characteristic initial value problem
15(5)
The Trautman-Bondi energy for the scalar field
20(3)
Hamiltonian flows for geometric field theories
23(18)
The framework
23(6)
Hamiltonian dynamics for Lagrangian theories
29(5)
Space-time integrals
34(4)
Changes of Ψ and of the Lagrangian
38(3)
Radiating scalar fields
41(24)
Preliminaries
41(4)
Energy: convergence of integrals
45(4)
The phase space p (- ∞,0]
49(2)
The phase space p [ - 1,0]
51(1)
The phase space p [ - 1,0]
52(2)
The preferred Hamiltonian role of the Trautman-Bondi energy for scalar fields
54(3)
The Poincare group
57(4)
``Supertranslated'' hyperbolae
61(4)
The energy of the gravitational field
65(40)
Preliminaries
65(5)
Moving space like hypersurfaces
70(4)
Cosmological space-times
74(2)
Space-times asymptotically flat in spacelike directions
76(4)
Space-times with anti-de Sitter asymptotic behaviour
80(9)
Energy in the radiation regime: convergence of integrals
89(8)
Phase spaces: the space p
97(5)
The phase space p [ - 1,0]
102(1)
The phase space p [ - 1,0]
103(1)
Preferred role of the Trautman-Bondi energy
104(1)
Hamiltonians associated with the BMS group
105(34)
The Poincare group: convergence of integrals
105(6)
Supertranslations (and space translations): convergence of integrals
111(5)
The abstract Scri
116(3)
Lorentz charges
119(2)
A Hamiltonian definition of angular momentum of sections of j
121(5)
An example: Schwarzschild space-time
126(3)
An example: stationary space-time
129(2)
Lorentz covariance of global charges
131(3)
BMS invariance of energy-momentum
134(2)
Polyhomogeneous Scri's
136(3)
A. Odd forms (densities) 139(2)
B. Solutions of the wave equation smoothly extendable to j 141(2)
C. Gravitational field: some auxiliary results 143(24)
The canonical gravitational variables in Bondi coordinates
143(3)
Smooth Scri's
143(2)
Polyhomogeneous asymptotics
145(1)
Solutions of the vacuum Einstein equations containing hyperboloidal initial data
146(6)
Bondi coordinates vs hyperboloidal initial data
152(5)
The calculation of the Wxμ,s
157(2)
Transformation rules of the Bondi functions under supertranslations
159(3)
Transformation rules of the Bondi functions under boosts
162(1)
Bondi coordinates in the Kerr space-time
163(3)
Conformal recalings of ADM Cauchy data
166(1)
References 167