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Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian Order

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Blanchet, Luc, Damour, Thibault, Iyer, Bala R., Will, Clifford M., Wiseman, Alan G.·1995·Physical Review Letters

Abstract

The rate of gravitational-wave energy loss from inspiralling binary systems of compact objects of arbitrary mass is derived through second post-Newtonian (2PN) order $O(({Gm/rc}^{2}{)}^{2})$ beyond the quadrupole approximation. The result has been derived by two independent calculations of the (source) multipole moments. The 2PN terms, and, in particular, the finite mass contribution therein (which cannot be obtained in perturbation calculations of black hole spacetimes), are shown to make a significant contribution to the accumulated phase of theoretical templates to be used in matched filtering of the data from future gravitational-wave detectors.

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Metadata

Authors
Blanchet, L., Damour, T., Iyer, B. R., Will, C. M., & Wiseman, A. G.
Venue
Physical Review Letters
Published
1995-05-01
Volume
74
Issue
18
Pages
3515-3518
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W1995114597
Cited by
533
References
0
FWCI
21.22
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian Order. https://app.cochat.ai/papers/10.1103/physrevlett.74.3515
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Blanchet, L., Damour, T., Iyer, B. R., Will, C. M., & Wiseman, A. G. (1995). Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian Order. Physical Review Letters. https://doi.org/10.1103/physrevlett.74.3515

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