Next to leading order gravitational wave emission and dynamical evolution of compact binary systems with spin

Abstract

Compact binary systems with spinning components are considered. Finite size effects due to rotational deformation are taken into account. The dynamical evolution and next to leading order gravitational wave forms are calculated, taking into account the orbital motion up to the first post-Newtonian approximation.

typos corrected; version submitted to Class. Quant. Grav

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