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Description
  • The article written by C.M.Will (1974) describes a method how to obtain a perturbation of an (originally) Schwarzschild metric by a slowly rotating light ring. This scheme is revisited in order to adapt it to the case of a thin disc.It turns out for some class of mass distribution on the disc bounded between some radii the solution (or at least its decomposition into spherical harmonics) can be found explicitly.
  • The article written by C.M.Will (1974) describes a method how to obtain a perturbation of an (originally) Schwarzschild metric by a slowly rotating light ring. This scheme is revisited in order to adapt it to the case of a thin disc.It turns out for some class of mass distribution on the disc bounded between some radii the solution (or at least its decomposition into spherical harmonics) can be found explicitly. (en)
Title
  • Linear perturbations of a Schwarzschild black hole by thin disc
  • Linear perturbations of a Schwarzschild black hole by thin disc (en)
skos:prefLabel
  • Linear perturbations of a Schwarzschild black hole by thin disc
  • Linear perturbations of a Schwarzschild black hole by thin disc (en)
skos:notation
  • RIV/00216208:11320/11:10109542!RIV12-GA0-11320___
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  • P(GD205/09/H033), S
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  • 1
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  • 209611
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  • RIV/00216208:11320/11:10109542
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  • general relativity; Schwarzschild black hole; Linear perturbations (en)
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  • GB - Spojené království Velké Británie a Severního Irska
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  • [18BD104FDCF3]
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  • Journal of Physics: Conference Series
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  • 314
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  • Čížek, Pavel
http://linked.open...ain/vavai/riv/wos
  • 000295798700071
issn
  • 1742-6588
number of pages
http://bibframe.org/vocab/doi
  • 10.1088/1742-6596/314/1/012071
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  • 11320
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