Ringing of Rapidly Rotating Black Holes in Higher-derivative Gravity
Simon Maenaut University of Copenhagen
Simon Maenaut University of Copenhagen
Chong Wang Perimeter Institute for Theoretical Physics
Kevin Costello Perimeter Institute for Theoretical Physics
Aldo Riello Perimeter Institute for Theoretical Physics
Simon Maenaut University of Copenhagen
Within the Effective Field Theory approach to gravity, deviations from General Relativity can be systematically described by higher-curvature operators. However, computing the resulting corrections to black hole quasinormal mode spectra remains challenging in the rapidly rotating regime, where perturbative expansions in the spin break down. Making use of recently constructed numerical rotating black hole solutions, we computed scalar quasinormal mode frequency shifts at leading order for scalar Gauss-Bonnet, dynamical Chern-Simons and Cubic Riemann corrections. We employed a pseudo-spectral collocation method to solve the perturbation equations on these backgrounds, enabling accurate computation across a broad parameter range. We observed that corrections to certain modes grow significantly as the spin approaches the near-extremal regime.
Chong Wang Perimeter Institute for Theoretical Physics
Kevin Costello Perimeter Institute for Theoretical Physics
Aldo Riello Perimeter Institute for Theoretical Physics