Toroidal source around a static black hole

Article

Toroidal source around a static black hole

Šácha, J.; Semerák, O.

Czech. J. Phys. 55(2), 139-155 (2005)

Abstract

A sequence of exact solutions of Einstein equations is obtained describing the fields of a Schwarzschild black hole surrounded by static, axially symmetric, thick toroids. Its properties are illustrated by plotting the shape of the gravitational field, the deformation of the black-hole horizon and several types of time-like geodesics, in dependence on parameters of the toroid.

Institute authors

Semerák, Oldřich

Supported by

GACR 202/02/0735 — Relativistic physics and astrophysics 2002-04
GACR 205/03/0902 — Relativistická astrofyzika: vybrané problémy

BibTeX

@article{UTF776,
  author        = {Šácha, J. and Semerák, O.},
  title         = {{Toroidal source around a static black hole}},
  journal       = {Czech. J. Phys.},
  volume        = {55},
  number        = {2},
  pages         = {139-155},
  year          = {2005},
  month         = {2},
  doi           = {10.1007/s10582-005-0026-x},
  url           = {https://link.springer.com/article/10.1007\%2Fs10582-005-0026-x},
}