Speaker
Balázs Kacskovics
Description
CBWaves is a numerical code designed to model gravitational wave emission from compact spinning binaries on eccentric orbits, employing the post-Newtonian (PN) expansion. Originally developed by Péter Csizmadia et al., the code has been continuously maintained and extended by members of the Gravitational Physics Group at HUN-REN Wigner Research Centre for Physics. A recent development includes the incorporation of the 4.5 PN radiation-reaction term, enhancing the code's accuracy in capturing energy dissipation effects. This presentation provides an overview of the current theoretical framework and computational capabilities of CBWaves.