Tidal indicators in the spacetime of a rotating deformed mass (Articolo in rivista)

Type
Label
  • Tidal indicators in the spacetime of a rotating deformed mass (Articolo in rivista) (literal)
Anno
  • 2012-01-01T00:00:00+01:00 (literal)
Alternative label
  • Bini D., Kuantay B., Geralico A. (2012)
    Tidal indicators in the spacetime of a rotating deformed mass
    in Classical and quantum gravity (Print)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Bini D., Kuantay B., Geralico A. (literal)
Pagina inizio
  • 145003 (literal)
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  • 29 (literal)
Rivista
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  • D. Bini Istituto per le Applicazioni del Calcolo ``M. Picone,'' CNR, I--00185 Rome, Italy ICRA, University of Rome ``La Sapienza,'' I--00185 Rome, Italy INFN, Sezione di Firenze, I--00185, Sesto Fiorentino (FI), Italy Kuantay B. Physics Department, University of Rome ``La Sapienza,'' I--00185 Rome, Italy ICRANet, Piazzale della Repubblica 10, I-65122 Pescara, Italy Geralico A. Physics Department, University of Rome ``La Sapienza,'' I--00185 Rome, Italy ICRA, University of Rome ``La Sapienza,'' I--00185 Rome, Italy (literal)
Titolo
  • Tidal indicators in the spacetime of a rotating deformed mass (literal)
Abstract
  • Tidal indicators are commonly associated with the electric and magnetic parts of the Riemann tensor (and its covariant derivatives) with respect to a given family of observers in a given spacetime. Recently, observer-dependent tidal effects have been extensively investigated with respect to a variety of special observers in the equatorial plane of the Kerr spacetime. This analysis is extended here by considering a more general background solution to include the case of matter which is also endowed with an arbitrary mass quadrupole moment. Relation with curvature invariants and Bel-Robinson tensor, i.e., observer-dependent super-energy density and super-Poynting vector, are investigated too. (literal)
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