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Estimating effective higher order terms in the post-Newtonian binding energy and gravitational-wave flux: Non-spinning compact binary inspiral
Shasvath J. Kapadia, Nathan K. Johnson-McDaniel, Parameswaran Ajith
In the adiabatic post-Newtonian (PN) approximation, the phase evolution of gravitational waves (GWs) from inspiralling compact binaries in quasicircular orbits is computed by equat…
Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions
Tim Dietrich, Niclas Moldenhauer, Nathan K. Johnson-McDaniel +4
Information about the last stages of a binary neutron star inspiral and the final merger can be extracted from quasi-equilibrium configurations and dynamical evolutions. In this ar…
Experimental mathematics meets gravitational self-force
Nathan K. Johnson-McDaniel, Abhay G. Shah, Bernard F. Whiting
It is now possible to compute linear in mass-ratio terms in the post-Newtonian (PN) expansion for compact binaries to very high orders using black hole perturbation theory applied…