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  Charges for linearized gravity

Aksteiner, S., & Andersson, L. (2013). Charges for linearized gravity. Classical and quantum gravity, 30(15): 155016. doi:10.1088/0264-9381/30/15/155016.

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1301.2674 (Preprint), 313KB
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 Creators:
Aksteiner, Steffen, Author
Andersson, Lars1, Author           
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1Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24012              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Mathematical Physics, math-ph,Mathematics, Mathematical Physics, math.MP
 Abstract: Maxwell test fields as well as solutions of linearized gravity on the Kerr exterior admit non-radiating modes, i.e. non-trivial time-independent solutions. These are closely related to conserved charges. In this paper we discuss the non-radiating modes for linearized gravity, which may be seen to correspond to the Poincare Lie-algebra. The 2-dimensional isometry group of Kerr corresponds to a 2-parameter family of gauge-invariant non-radiating modes representing infinitesimal perturbations of mass and azimuthal angular momentum. We calculate the linearized mass charge in terms of linearized Newman-Penrose scalars.

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 Dates: 2013-01-122013-02-0420132013
 Publication Status: Issued
 Pages: 19 pages. v3: Added comments and references
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 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 1301.2674
DOI: 10.1088/0264-9381/30/15/155016
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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics
Pages: - Volume / Issue: 30 (15) Sequence Number: 155016 Start / End Page: - Identifier: ISSN: 0264-9381
CoNE: https://pure.mpg.de/cone/journals/resource/954925513480_1