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  • Influence of cosmological constant on toroidal fluid configurations around charged spherically symmetric black holes and naked singularities is demostrated by study of perfect fluid tori with uniform distribution of specific angular momentum orbiting in the Reissner-Nordstrom-(anti-)de Sitter spacetimes. Toroidal configurations are allowed only in the space times admitting existence of stable circular geodesics. Configurations with marginally closed equipotential (equipressure) surfaces crossing itself in a cusp allow accretion (through the inner cusp) and/or excretion (through the outer cusp) of matter from the toroidal configuration. Detailed classification of the Reissner-Nordstrom-(anti-)de Sitter spacetimes according to properties of the marginally stable tori is given. It is demonstrated that in the Reissner-Nordstrom-de Sitter naked-singularity spacetimes an interesting phenomenon of doubled tori can exist enabling exchange of matter between two tori in both inward and outward directions. In naked-singularity spacetimes the accretion onto the central singularity is impossible due to existence of a potential barrier.
  • Influence of cosmological constant on toroidal fluid configurations around charged spherically symmetric black holes and naked singularities is demostrated by study of perfect fluid tori with uniform distribution of specific angular momentum orbiting in the Reissner-Nordstrom-(anti-)de Sitter spacetimes. Toroidal configurations are allowed only in the space times admitting existence of stable circular geodesics. Configurations with marginally closed equipotential (equipressure) surfaces crossing itself in a cusp allow accretion (through the inner cusp) and/or excretion (through the outer cusp) of matter from the toroidal configuration. Detailed classification of the Reissner-Nordstrom-(anti-)de Sitter spacetimes according to properties of the marginally stable tori is given. It is demonstrated that in the Reissner-Nordstrom-de Sitter naked-singularity spacetimes an interesting phenomenon of doubled tori can exist enabling exchange of matter between two tori in both inward and outward directions. In naked-singularity spacetimes the accretion onto the central singularity is impossible due to existence of a potential barrier. (en)
Title
  • Toroidal configurations of perfect fluid in the Reissner-Nordstrom-(anti-)de Sitter spacetimes
  • Toroidal configurations of perfect fluid in the Reissner-Nordstrom-(anti-)de Sitter spacetimes (en)
skos:prefLabel
  • Toroidal configurations of perfect fluid in the Reissner-Nordstrom-(anti-)de Sitter spacetimes
  • Toroidal configurations of perfect fluid in the Reissner-Nordstrom-(anti-)de Sitter spacetimes (en)
skos:notation
  • RIV/47813059:19240/11:#0003872!RIV12-MSM-19240___
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  • P(LC06014), Z(MSM4781305903)
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  • 1
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  • 235563
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  • RIV/47813059:19240/11:#0003872
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  • astrophysical fluid dynamics, GR black holes, accretion, dark energy theory (en)
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  • GB - Spojené království Velké Británie a Severního Irska
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  • [940301299424]
http://linked.open...i/riv/nazevZdroje
  • JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
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  • Kučáková, Hana
  • Stuchlík, Zdeněk
  • Slaný, Petr
http://linked.open...n/vavai/riv/zamer
issn
  • 1475-7516
number of pages
http://bibframe.org/vocab/doi
  • 10.1088/1475-7516/2011/01/033
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  • 19240
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