http://www.cnr.it/ontology/cnr/individuo/prodotto/ID191863
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
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Bini D., Kuantay B., Geralico A. (literal)
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- Rivista
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- 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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- Autore CNR
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