Numerical-relativity validation of effective-one-body waveforms in the intermediate-mass-ratio regime

@inproceedings{Nagar2022NumericalrelativityVO,
  title={Numerical-relativity validation of effective-one-body waveforms in the intermediate-mass-ratio regime},
  author={Alessandro Nagar and James Healy and Carlos O. Lousto and Sebastiano Bernuzzi and Ange Albertini},
  year={2022}
}
Alessandro Nagar, James Healy, Carlos O. Lousto, Sebastiano Bernuzzi, and Angelica Albertini INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy Institut des Hautes Etudes Scientifiques, 91440 Bures-sur-Yvette, France Center for Computational Relativity and Gravitation, School of Mathematical Sciences, Rochester Institute of Technology, 85 Lomb Memorial Drive, Rochester, New York 14623, USA Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, 07743, Jena, Germany… 

Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Tousif Islam,1, 2, 3, 4, ∗ Scott E. Field,2, 3 Scott A. Hughes,5 Gaurav Khanna,6, 1, 3 Vijay Varma,7, † Matthew Giesler,8 Mark A. Scheel,9 Lawrence E. Kidder,8 and Harald P. Pfeiffer7 1Department of

Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

We present the first systematic comparison between gravitational waveforms emitted by inspiralling, quasi-circular and nonspinning black hole binaries computed with three different approaches:

Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

We compare recently computed waveforms from second-order gravitational self-force (GSF) theory to those generated by a new, GSF-informed, effective one body (EOB) waveform model for (spin-aligned,

Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Gravitational wave observations of large mass ratio compact binary mergers like GW190814 highlight the need for reliable, high-accuracy waveform templates for such systems. We present NRHybSur2dq15 ,

References

SHOWING 1-10 OF 61 REFERENCES

and a at

The xishacorene natural products are structurally unique apolar diterpenoids that feature a bicyclo[3.3.1] framework. These secondary metabolites likely arise from the well-studied, structurally

“A and B”:

Direct fabrication of large micropatterned single crystals. p1205 21 Feb 2003. (news): Academy plucks best biophysicists from a sea of mediocrity. p994 14 Feb 2003.

Phys

  • Rev. D 102, 024077
  • 2020

Phys

  • Rev. Lett. 125, 191102
  • 2020

Phys

  • Rev. D92, 102001
  • 2015

Phys

  • Rev. D62, 084011
  • 2000

Class

  • Quant. Grav. 22, R167
  • 2005

Phys

  • Rev. D88, 064014
  • 2013

Phys

  • Rev. D 104, 024067
  • 2021
...