On radiative properties of boost-rotation symmetric, type D spacetimes

  1. R. Lazkoz Saéz 1
  2. J. A. Valiente Kroon
  1. 1 Universidad de Deusto
    info

    Universidad de Deusto

    Bilbao, España

    ROR https://ror.org/00ne6sr39

Livre:
Proceedings of the XXIII Spanish Relativity Meeting on Reference Frames and Gravitomagnetism: Valladolid, Spain, 6-9 September 2000
  1. J. F. Pascual Sánchez (ed. lit.)
  2. L. Floría (ed. lit.)
  3. A. San Miguel (coord.)
  4. F. Vicente (coord.)

Éditorial: World Scientific Publishing Company

ISBN: 9810246315

Année de publication: 2001

Pages: 327-332

Congreso: Spanish Relativity Meeting (23. 2000. Salamanca)

Type: Communication dans un congrès

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Résumé

The asymptotic properties of the solutions to the Einstein-Maxwell equations with boost-rotation symmetry and Petrov type D are studied. We find series solutions to the pertinent set of equations which are suitable for a late time descriptions in coordinates which are well adapted for the description of the radiative properties of spacetimes (Bondi coordinates). By calculating the total charge, Bondi and NUT mass and the Newman-Penrose constants of the spacetimes we provide a physical interpretation of the free parameters of the solutions. Additional relevant aspects on the asymptotics and radiative properties of the spacetimes considered, such as the possible polarization states of the gravitational and electromagnetic field, are discussed through the way.

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