PIRSA:20120019

Video URL

https://pirsa.org/20120019

Self-torque and frame nutation in binary black hole simulations

Bustamante, M.J. (2020). Self-torque and frame nutation in binary black hole simulations. Perimeter Institute for Theoretical Physics. https://pirsa.org/20120019

Bustamante, Maria José. Self-torque and frame nutation in binary black hole simulations. Perimeter Institute for Theoretical Physics, Dec. 10, 2020, https://pirsa.org/20120019 

          @misc{ scivideos_PIRSA:20120019,
            doi = {10.48660/20120019},
            url = {https://pirsa.org/20120019},
            author = {Bustamante, Maria Jos{\'e}},
            keywords = {Strong Gravity},
            language = {en},
            title = {Self-torque and frame nutation in binary black hole simulations},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2020},
            month = {dec},
            note = {PIRSA:20120019 see, \url{https://scivideos.org/index.php/pirsa/20120019}}
          }

Maria José Bustamante The University of Texas at Austin

Talk numberPIRSA:20120019
DOI10.48660/20120019
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

We investigate the precession of the spin of the smaller black hole in binary black hole simulations. By considering a sequence of binaries at higher mass ratios, we approach the limit of geodetic precession of a test spin. This precession is corrected by the ``self-torque'' due to the smaller black hole's own spacetime curvature. We find that the spins undergo spin nutations which are not described in conventional descriptions of spin precession, an effect that has been noticed previously in simulations. These nutations arise because the spins are not measured in a frame where the smaller hole is stationary. We develop a simple model for these frame nutations, extract the instantaneous spin precession rate, and compare our results to PN and extreme-mass-ratio approximations for the self-torque.