About: Aschenbach Effect for Brany Kerr Black Holes and Naked Singularities     Goto   Sponge   NotDistinct   Permalink

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  • We study the non-monotonic Keplerian velocity profiles related to locally nonrotating frames (LNRF) in the field of near-extreme braneworld Kerr black holes and naked singularities in which the non-local gravitational effects of the bulk are represented by a braneworld tidal charge b and the 4D geometry of the spacetime structure is governed by the Kerr–Newman geometry. We show that positive tidal charge has a tendency to restrict the values of the black hole dimensionless spin a admitting existence of the non-monotonic Keplerian LNRF-velocity profiles; the non-monotonic profiles exist in the black hole spacetimes with tidal charge smaller than b D 0:41005 (and spin larger than a D 0:76808). With decreasing value of the tidal charge (which need not be only positive), both the region of spin allowing the non-monotonicity in the LNRF-velocity profile around braneworld Kerr black hole and the velocity difference in the minimum-maximum parts of the velocity profile increase implying growing astrophysical relevance of this phenomenon.
  • We study the non-monotonic Keplerian velocity profiles related to locally nonrotating frames (LNRF) in the field of near-extreme braneworld Kerr black holes and naked singularities in which the non-local gravitational effects of the bulk are represented by a braneworld tidal charge b and the 4D geometry of the spacetime structure is governed by the Kerr–Newman geometry. We show that positive tidal charge has a tendency to restrict the values of the black hole dimensionless spin a admitting existence of the non-monotonic Keplerian LNRF-velocity profiles; the non-monotonic profiles exist in the black hole spacetimes with tidal charge smaller than b D 0:41005 (and spin larger than a D 0:76808). With decreasing value of the tidal charge (which need not be only positive), both the region of spin allowing the non-monotonicity in the LNRF-velocity profile around braneworld Kerr black hole and the velocity difference in the minimum-maximum parts of the velocity profile increase implying growing astrophysical relevance of this phenomenon. (en)
Title
  • Aschenbach Effect for Brany Kerr Black Holes and Naked Singularities
  • Aschenbach Effect for Brany Kerr Black Holes and Naked Singularities (en)
skos:prefLabel
  • Aschenbach Effect for Brany Kerr Black Holes and Naked Singularities
  • Aschenbach Effect for Brany Kerr Black Holes and Naked Singularities (en)
skos:notation
  • RIV/47813059:19240/14:#0005095!RIV15-MSM-19240___
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  • I, P(EE2.3.20.0071), P(GB14-37086G), S
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  • 4168
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  • RIV/47813059:19240/14:#0005095
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  • Aschenbach effect; Randall Sundrum; Brane-world (en)
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  • [997CDE55160E]
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  • Opava, Czech Republic
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  • Opava
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  • Proceedings of RAGtime 10-13: Workshops on black holes and neutron stars
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  • Stuchlík, Zdeněk
  • Blaschke, Martin
  • Slaný, Petr
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issn
  • 2336-5668
number of pages
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  • Slezská univerzita v Opavě
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  • 978-80-7510-124-2
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  • 19240
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