Corpus ID: 237290113

Predictions for LISA and PTA based on SHARK galaxy simulations

@inproceedings{Curylo2021PredictionsFL,
  title={Predictions for LISA and PTA based on SHARK galaxy simulations},
  author={M. Curylo and T. Bulik},
  year={2021}
}
We present our analysis of a set of populations of massive black hole binaries generated in the recent semi-analytic model of galaxy evolution (SHARK). We focus on studying gravitational wave emission produced by these inspiraling binaries in terms of their detectability with current and future detectors, i.e. PTA (Pulsar Timing Array) and LISA (Laser Interferometer Space Antenna). The key advantage of SHARK is that it provides a way to explore a number of distinct models of black hole and… Expand

Figures and Tables from this paper

References

SHOWING 1-5 OF 5 REFERENCES
Acknowledgements. TB was suported by the Foundation for Polish Science grant TEAM/2016-3/19. We are grateful to the SHARK team for helpful discussions
  • 2019
M.Curyło and T.Bulik: Predictions for LISA and PTA based on SHARK galaxy
  • J. 1982,
  • 2016
2016, in Astronomical Society of the Pacific
  • 2016
A&A proofs: manuscript no. mcurylo21
    Total masses of binaries detected by LISA during whole 4-year long mission (color) and all binaries merging in 50 years (grey) as a function of redshift. Color scale shows predicted SNR of detection