Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits

Details Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits

2001-10-23

arxiv.org/abs/gr-qc/0110100v2

Phys.Rev. D65 (2002) 084011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

40 pages, 10 figures, To appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.65.084011

The second post-Newtonian (2PN) contribution to the `plus' and `cross' gravitational wave polarizations associated with gravitational radiation from non-spinning, compact binaries moving in elliptic orbits is computed. The computation starts from our earlier results on 2PN generation, crucially employs the 2PN accurate generalized quasi-Keplerian parametrization of elliptic orbits by Damour, Sch\"afer and Wex and provides 2PN accurate expressions modulo the tail terms for gravitational wave polarizations incorporating effects of eccentricity and periastron precession.

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