Publications

Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University

← Back to the list

Article

Analysis of gravitational radiation generated by type D black holes with positive cosmological constant

Fernandez-Alvarez, F.; Podolský, J.; Senovilla, J. M. M.

Phys. Rev. D 110(10), 20 (2024)

doi ↗ link ↗

Abstract

The criterion for existence of gravitational radiation at conformal infinity in the presence of a positive cosmological constant is applied to a general family of exact solutions representing generic (pairs of) black holes of algebraic type D. Our analysis shows that only accelerating black holes generate gravitational radiation measurable at infinity. This very satisfactory result confirms the goodness of the criterion. To that end, a new metric form of the family of exact type D black holes is constructed-including any cosmological constant and a (double-aligned) non-null electromagnetic field-whose expression is suitable for investigation of the asymptotic structure of this large family of spacetimes. The family depends on seven physical parameters, namely m , a , l , alpha , e , g , and A that characterize mass, specific angular momentum parameter, NUT parameter, acceleration, electric and magnetic charges, and the cosmological constant, respectively.

Institute authors

Supported by

  • GACR 23-05914S — Pokročilé techniky aplikované na přesné prostoročasy s černými dírami a gravitačními vlnami

BibTeX

@article{UTF999,
  author        = {Fernandez-Alvarez, F. and Podolský, J. and Senovilla, J. M. M.},
  title         = {{Analysis of gravitational radiation generated by type D black holes with positive cosmological constant}},
  journal       = {Phys. Rev. D},
  volume        = {110},
  number        = {10},
  pages         = {20},
  year          = {2024},
  month         = {11},
  doi           = {10.1103/PhysRevD.110.104029},
  url           = {https://doi.org/10.1103/PhysRevD.110.104029},
}