Massless field perturbations of the spinning C metric (Articolo in rivista)

Type
Label
  • Massless field perturbations of the spinning C metric (Articolo in rivista) (literal)
Anno
  • 2008-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1063/1.2938699 (literal)
Alternative label
  • Bini D., Cherubini C., Geralico A. (2008)
    Massless field perturbations of the spinning C metric
    in Journal of mathematical physics; American Institute Of Physics (AIP), Melville (Stati Uniti d'America)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Bini D., Cherubini C., Geralico A. (literal)
Pagina inizio
  • 062502 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 49 (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroFascicolo
  • 6 (literal)
Note
  • Scopu (literal)
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • Istituto per le Applicazioni del Calcolo \"M. Picone,\" CNR, I-00161 Rome, Italy ICRA, University of Rome \"La Sapienza,\" I-00185 Rome, Italy INFN-Sezione di Firenze, Polo Scientifico, Via Sansone 1, Sesto Fiorentino, Firenze I-50019, Italy Facoltà di Ingegneria, Università Campus Biomedico, Via Alvaro del Portillo 21, I-00128 Roma, Italy Physics Department, University of Rome \"La Sapienza,\" I-00185 Rome, Italy (literal)
Titolo
  • Massless field perturbations of the spinning C metric (literal)
Abstract
  • A single master equation is given describing spin s=2 test fields that are gaugeand tetrad-invariant perturbations of the spinning C metric space-time representing a source with mass M, uniformly rotating with angular momentum per unit mass a, and uniformly accelerated with acceleration A. This equation can be separated into its radial and angular parts. The behavior of the radial functions near the black hole outer horizon is studied to examine the influence of A on the phenomenon of super-radiance, while the angular equation leads to modified spin-weighted spheroidal harmonic solutions generalizing those of the Kerr space-time. Finally the coupling between the spin of the perturbing field and the acceleration parameter A is discussed. (literal)
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