Circular holonomy and clock effects in stationary axisymmetric spacetimes (Articolo in rivista)

Type
Label
  • Circular holonomy and clock effects in stationary axisymmetric spacetimes (Articolo in rivista) (literal)
Anno
  • 2002-01-01T00:00:00+01:00 (literal)
Alternative label
  • Bini D., Jantzen R.T., Mashhoon B. (2002)
    Circular holonomy and clock effects in stationary axisymmetric spacetimes
    in Classical and quantum gravity (Print)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Bini D., Jantzen R.T., Mashhoon B. (literal)
Pagina inizio
  • 17 (literal)
Pagina fine
  • 37 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 19 (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#note
  • E-print: gr-qc/0111028 (literal)
Note
  • ISI Web of Science (WOS) (literal)
Titolo
  • Circular holonomy and clock effects in stationary axisymmetric spacetimes (literal)
Abstract
  • Stationary axisymmetric spacetimes containing a pair of oppositely rotating periodically intersecting circular geodesics allow us to study the various so-called 'clock effects' by comparing either observer or geodesic proper time periods of orbital circuits defined by the observer or the geodesic crossing points. This can be extended from a comparison of clocks to a comparison of parallel-transported vectors, leading to the study of special elements of the spacetime holonomy group. The band of holonomy invariance found for a dense subset of special geodesic orbits outside a certain radius in the static case does not exist in the nonstatic case. In the Kerr spacetime the dimensionless frequencies associated with parallel-transport rotations can be expressed as ratios of the proper and average coordinate periods of the circular geodesics. (literal)
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