Monday, July 1, 2013

1003.2735 (Manuel Tessmer et al.)

Motion and gravitational wave forms of eccentric compact binaries with
orbital-angular-momentum-aligned spins under next-to-leading order in
spin-orbit and leading order in spin(1)-spin(2) and spin-squared couplings
   [PDF]

Manuel Tessmer, Johannes Hartung, Gerhard Schaefer
A quasi-Keplerian parameterisation for the solutions of second post-Newtonian (PN) accurate equations of motion for spinning compact binaries is obtained including leading order spin-spin and next-to-leading order spin-orbit interactions. Rotational deformation of the compact objects is incorporated. For arbitrary mass ratios the spin orientations are taken to be parallel or anti-parallel to the orbital angular momentum vector. The emitted gravitational wave forms are given in analytic form up to 2PN point particle, 1.5PN spin orbit and 1PN spin-spin contributions, where the spins are counted of 0PN order.
View original: http://arxiv.org/abs/1003.2735

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