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Phys. Rev. Lett. 80, 5052–5055 (1998)

Uniqueness of Scalar Field Energy and Gravitational Energy in the Radiating Regime

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Piotr T. Chruściel*
Département de Mathématiques, Faculté des Sciences, Université de Tours, Parc de Grandmont, F-37200 Tours, France

Jacek Jezierski
Department of Mathematical Methods in Physics, University of Warsaw, ulica Hoża 74, 00-682 Warszawa, Poland

Malcolm A. H. MacCallum
School of Mathematical Sciences, Queen Mary and Westfield College, University of London, Mile End Road, London E1 4NS, United Kingdom

Received 20 January 1998; published in the issue dated 8 June 1998

The usual approaches to the definition of energy give an ambiguous result for the energy of fields in the radiating regime. We show that for a massless scalar field in Minkowski spacetime the definition may be rendered unambiguously by adding the requirement that the energy cannot increase in retarded time. We present a similar theorem for the gravitational field, proved elsewhere, which establishes that the Trautman-Bondi energy is the unique (up to a multiplicative factor) functional, within a natural class, which is monotonic in time for all solutions of the vacuum Einstein equations admitting a smooth “piece” of conformal null infinity I.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.80.5052
DOI:
10.1103/PhysRevLett.80.5052
PACS:
04.20.Cv, 03.50.-z, 11.10.Ef

*Electronic address: Chrusciel@Univ-Tours.Fr

Electronic address: jjacekj@fuw.edu.pl

Electronic address: M.A.H.MacCallum@qmw.ac.uk