Orateur
Dr
Sashwat Tanay
(LUTH, Paris Observatory)
Description
We present an analytical solution to the binary black hole system with arbitrary spins, eccentricity, and masses at the second post-Newtonian order. This solution owing to its analytical nature is expected to facilitate quick gravitational wave (GW) template generation and accelerate GW detection and parameter estimation.
Auteurs principaux
Dr
Laura Bernard
(LUTH, Paris Observatory)
M.
Manuel Alva Morales
(Trujillo Natl. U.)
Dr
Sashwat Tanay
(LUTH, Paris Observatory)
M.
Tom Colin
(LUTH, Paris Observatory)
