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In this Comment we compute the contributions of the radiation reaction force in the 2.5 post-Newtonian (PN) gravitational wave polarizations for compact binaries in circular orbits.
- (i) We point out and correct an inconsistency in the derivation of Arun, Blanchet, Iyer, and Qusailah.
- (ii) We prove that all contributions from radiation reaction in the 2.5PN waveform are actually negligible since they can be absorbed into a modification of the orbital phase at the 5PN order.
Built on
Tagoshi H and Sasaki M 1994 Prog. Theor. Phys
1994
Earlier work this paper cites.
Similar
Arun K G, Blanchet L, Iyer B R, and Qusailah M S S 2004 Class. Quantum Grav
2005
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2005
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