About: Circular geodesics of naked singularities in the Kehagias-Sfetsos metric of Hořava’s gravity     Goto   Sponge   NotDistinct   Permalink

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Description
  • We discuss photon and test-particle orbits in the Kehagias-Sfetsos (KS) metric of Hořava’s gravity. For any value of the Hořava parameter \omega, there are values of the gravitational mass M for which the metric describes a naked singularity, and this is always accompanied by a vacuum “antigravity sphere” on whose surface a test particle can remain at rest (in a zero angular momentum geodesic), and inside which no circular geodesics exist. The observational appearance of an accreting KS naked singularity in a binary system would be that of a quasistatic spherical fluid shell surrounded by an accretion disk, whose properties depend on the value of M, but are always very different from accretion disks familiar from the Kerr-metric solutions. The properties of the corresponding circular orbits are qualitatively similar to those of the Reissner-Nordström naked singularities. When event horizons are present, the orbits outside the Kehagias-Sfetsos black hole are qualitatively similar to those of the Schwarzschild metric.
  • We discuss photon and test-particle orbits in the Kehagias-Sfetsos (KS) metric of Hořava’s gravity. For any value of the Hořava parameter \omega, there are values of the gravitational mass M for which the metric describes a naked singularity, and this is always accompanied by a vacuum “antigravity sphere” on whose surface a test particle can remain at rest (in a zero angular momentum geodesic), and inside which no circular geodesics exist. The observational appearance of an accreting KS naked singularity in a binary system would be that of a quasistatic spherical fluid shell surrounded by an accretion disk, whose properties depend on the value of M, but are always very different from accretion disks familiar from the Kerr-metric solutions. The properties of the corresponding circular orbits are qualitatively similar to those of the Reissner-Nordström naked singularities. When event horizons are present, the orbits outside the Kehagias-Sfetsos black hole are qualitatively similar to those of the Schwarzschild metric. (en)
Title
  • Circular geodesics of naked singularities in the Kehagias-Sfetsos metric of Hořava’s gravity
  • Circular geodesics of naked singularities in the Kehagias-Sfetsos metric of Hořava’s gravity (en)
skos:prefLabel
  • Circular geodesics of naked singularities in the Kehagias-Sfetsos metric of Hořava’s gravity
  • Circular geodesics of naked singularities in the Kehagias-Sfetsos metric of Hořava’s gravity (en)
skos:notation
  • RIV/47813059:19240/14:#0005069!RIV15-MSM-19240___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(EE2.3.20.0071), P(GB14-37086G)
http://linked.open...iv/cisloPeriodika
  • 2
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http://linked.open...aciTvurceVysledku
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  • 7318
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  • RIV/47813059:19240/14:#0005069
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  • Hořava's gravity (en)
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  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [FA0CF52CB36C]
http://linked.open...i/riv/nazevZdroje
  • Physical Review D
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http://linked.open...v/svazekPeriodika
  • 90
http://linked.open...iv/tvurceVysledku
  • Stuchlík, Zdeněk
  • Schee, Jan
  • Abramowicz, Marek Artur
  • Kluźniak, Włodek
  • Vieira, Ronaldo Savioli Sumé
http://linked.open...ain/vavai/riv/wos
  • 000339447600005
issn
  • 1550-7998
number of pages
http://bibframe.org/vocab/doi
  • 10.1103/PhysRevD.90.024035
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  • 19240
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