Abstract
We obtain a fourth-order accurate numerical algorithm to integrate the Zerilli and Regge–Wheeler wave equations, describing perturbations of non-rotating black holes, with source terms due to an orbiting particle. Those source terms contain Dirac's delta and its first derivative. We also re-derive the source of the Zerilli and Regge–Wheeler equations for more convenient definitions of the waveforms that allow direct metric reconstruction (in the Regge–Wheeler gauge).
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
