Forces at the Kerr singularity

Article

Forces at the Kerr singularity

Semerák, O.

Ap&SS 250(2), 235-243 (1997)

Abstract

In a classical-like language introduced in a previous paper, the fact that the ring singularity of the Kerr spacetime cannot be left/reached by timelike geodesic which is not bound to the equatorial plane is interpreted as a result of the interplay of the gravitational and – mainly – the centrifugal forces.

Institute authors

Semerák, Oldřich

Supported by

GACR 202/96/0206 — Relativistic physics and astrophysics
GAUK 230/1996 — Relativistická teorie gravitace, astrofyzika a kosmologie

BibTeX

@article{UTF748,
  author        = {Semerák, O.},
  title         = {{Forces at the Kerr singularity}},
  journal       = {Ap\&SS},
  volume        = {250},
  number        = {2},
  pages         = {235-243},
  year          = {1997},
  month         = {9},
  doi           = {10.1023/A:1000400815399},
  url           = {https://link.springer.com/article/10.1023\%2FA\%3A1000400815399},
}