Black hole binaries in Einstein-scalar-Gauss-Bonnet gravity and their effective-one-body description
APA
Julié, F. (2024). Black hole binaries in Einstein-scalar-Gauss-Bonnet gravity and their effective-one-body description. Perimeter Institute. https://pirsa.org/24070037
MLA
Julié, Félix-Louis. Black hole binaries in Einstein-scalar-Gauss-Bonnet gravity and their effective-one-body description. Perimeter Institute, Jul. 16, 2024, https://pirsa.org/24070037
BibTex
@misc{ pirsa_PIRSA:24070037, doi = {10.48660/24070037}, url = {https://pirsa.org/24070037}, author = {Juli{\'e}, F{\'e}lix-Louis}, keywords = {Cosmology, Strong Gravity, Mathematical physics}, language = {en}, title = {Black hole binaries in Einstein-scalar-Gauss-Bonnet gravity and their effective-one-body description}, publisher = {Perimeter Institute}, year = {2024}, month = {jul}, note = {PIRSA:24070037 see, \url{https://pirsa.org}} }
Max Planck Institute for Gravitational Physics
Talk Type
Abstract
I will show how to derive libraries of semi-analytic gravitational waveforms for coalescing “hairy” black hole binaries, focusing on the example of Einstein-scalar-Gauss-Bonnet gravity (ESGB). To do so, I will start from the state-of-the-art, effective-one-body waveform model “SEOBNRv5PHM” in general relativity, and deform it with ESGB corrections to infer inspiral-merger-ringdown waveform estimates.