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Description
  • Processes around astrophysical black holes are usually modeled with test (nongravitating) matter and fields. However, the very fact that the holes are %22visible%22 implies that some matter has to be present there. Even if very thin, it can influence the metric, mainly in higher derivatives, which should in turn affect its own behaviour, as well as motion of further (test) satellites. In particular, the geodesic dynamics, integrable in the fields of isolated stationary black holes, should become chaotic. Here we consider exact static, axially and reflection- symmetric space-times of a Schwarzschild black hole surrounded by a thin disc or ring, and examine how the presence of the additional source affects the dynamics of free test particles using recurence analysis.
  • Processes around astrophysical black holes are usually modeled with test (nongravitating) matter and fields. However, the very fact that the holes are %22visible%22 implies that some matter has to be present there. Even if very thin, it can influence the metric, mainly in higher derivatives, which should in turn affect its own behaviour, as well as motion of further (test) satellites. In particular, the geodesic dynamics, integrable in the fields of isolated stationary black holes, should become chaotic. Here we consider exact static, axially and reflection- symmetric space-times of a Schwarzschild black hole surrounded by a thin disc or ring, and examine how the presence of the additional source affects the dynamics of free test particles using recurence analysis. (en)
Title
  • Recurrence of geodesics in a black-hole-disc field
  • Recurrence of geodesics in a black-hole-disc field (en)
skos:prefLabel
  • Recurrence of geodesics in a black-hole-disc field
  • Recurrence of geodesics in a black-hole-disc field (en)
skos:notation
  • RIV/00216208:11320/12:10132124!RIV13-GA0-11320___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA202/09/0772), P(GD205/09/H033), S, Z(MSM0021620860)
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 164439
http://linked.open...ai/riv/idVysledku
  • RIV/00216208:11320/12:10132124
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • chaos; geodesic dynamics; accretion discs; black holes (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [7873FC479FB2]
http://linked.open...v/mistoKonaniAkce
  • Madrid, Španělsko
http://linked.open...i/riv/mistoVydani
  • MELVILLE
http://linked.open...i/riv/nazevZdroje
  • AIP Conference Proceedings
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Suková, Petra
  • Semerák, Oldřich
http://linked.open...vavai/riv/typAkce
http://linked.open...ain/vavai/riv/wos
  • 000306830600075
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
issn
  • 0094-243X
number of pages
http://bibframe.org/vocab/doi
  • 10.1063/1.4734475
http://purl.org/ne...btex#hasPublisher
  • AMER INST PHYSICS
https://schema.org/isbn
  • 978-0-7354-1060-2
http://localhost/t...ganizacniJednotka
  • 11320
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