Dynamics of spinning compact binaries: synergies between post-Newtonian and self-force approaches
APA
Khalil, M. (2021). Dynamics of spinning compact binaries: synergies between post-Newtonian and self-force approaches. Perimeter Institute. https://pirsa.org/21110046
MLA
Khalil, Mohammed. Dynamics of spinning compact binaries: synergies between post-Newtonian and self-force approaches. Perimeter Institute, Nov. 25, 2021, https://pirsa.org/21110046
BibTex
@misc{ pirsa_PIRSA:21110046, doi = {10.48660/21110046}, url = {https://pirsa.org/21110046}, author = {Khalil, Mohammed}, keywords = {Strong Gravity}, language = {en}, title = {Dynamics of spinning compact binaries: synergies between post-Newtonian and self-force approaches}, publisher = {Perimeter Institute}, year = {2021}, month = {nov}, note = {PIRSA:21110046 see, \url{https://pirsa.org}} }
Accurate waveform models are crucial for gravitational-wave (GW) data analysis, and since numerical-relativity waveforms are computationally expensive, it is important to improve the analytical approximations for the binary dynamics. The post-Newtonian (PN) approximation is most suited for describing the inspiral of comparable-mass binaries, which are the main sources for ground-based GW detectors. In this talk, I discuss a method for deriving PN results valid for arbitrary mass ratios from first-order self-force results, by exploiting the simple mass dependence of the scattering angle in the post-Minkowskian expansion. I present results for the spin-orbit dynamics up to the fourth-subleading PN order (5.5PN) and the spin-spin dynamics up to the third-subleading PN order (5PN). I also discuss implications for the first law of binary mechanics.
Zoom Link: https://pitp.zoom.us/j/92861625861?pwd=cHpXUlM1d01pc09mNGhhQVZxRHBiQT09