The Kerr–de Sitter spacetime in Bondi coordinates

Article

The Kerr–de Sitter spacetime in Bondi coordinates

Hoque Sk J.; Virmani A.

Class. Quantum Grav. 38(22), 21 (2021)

Abstract

We use zero angular momentum null geodesics in the Kerr-de Sitter spacetime to transform the metric in a generalised Bondi coordinate system. We write the metric components explicitly. Next, we choose the radial coordinate to be the areal coordinate and write the asymptotic metric in the Bondi-Sachs gauge.

Institute authors

Hoque, Sk Jahanur

Supported by

GACR 19-01850S — Black-hole and radiative spacetimes: exact methods

BibTeX

@article{UTF934,
  author        = {Hoque Sk J. and Virmani A.},
  title         = {{The Kerr–de Sitter spacetime in Bondi coordinates}},
  journal       = {Class. Quantum Grav.},
  volume        = {38},
  number        = {22},
  pages         = {21},
  year          = {2021},
  doi           = {10.1088/1361-6382/ac2c1f},
}