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The need for more and more accurate gravitational wave templates requires taking into account all possible contributions to the emission of gravitational radiation from a binary system.
1907
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1909
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T. Damour and N. Deruelle, “ General relativistic celestial mechanics of binary systems. I. The post-newtonian motion,” Annales de l’Institut Henri Poincaré., section A, 43
1985
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L. Blanchet and T. Damour, “Radiative gravitational fields in general relativity I. general structure of the field outside the source,” Phil. Trans. Roy. Soc. Lond. A 320
1986
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L. Blanchet and T. Damour, “Tail Transported Temporal Correlations in the Dynamics of a Gravitating System,” Phys. Rev. D 37
1988
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L. Blanchet and T. Damour, “Post-Newtonian Generation of Gravitational Waves,” Ann. Inst. H. Poincaré Phys. Théor. 50
1989
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T. Damour and B. R. Iyer, “Post-Newtonian generation of gravitational waves. 2. The Spin moments,” Ann. Inst. H. Poincaré Phys. Théor. 54
1991
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L. Blanchet and T. Damour, “Hereditary effects in gravitational radiation,” Phys. Rev. D 46
1992
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L. Blanchet and G. Schaefer, “Gravitational wave tails and binary star systems,” Class. Quant. Grav. 10
1993
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L. Blanchet and B. S. Sathyaprakash, “Detecting the tail effect in gravitational wave experiments,” Phys. Rev. Lett. 74
1995
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R. Rieth and G. Schaefer, “Spin and tail effects in the gravitational-wave emission of compact binaries,” Class. Quant. Grav. 14
1997
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L. Blanchet, “On the multipole expansion of the gravitational field,” Class. Quant. Grav. 15
1998
Cited alongside, same era.
O. Poujade and L. Blanchet, “Post-Newtonian approximation for isolated systems calculated by matched asymptotic expansions,” Phys. Rev. D 65
2002
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2003
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2004
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L. Blanchet, “Gravitational wave tails of tails,” Class. Quant. Grav. 15
2005
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2014
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2014
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2015
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2007
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2008
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2009
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2011
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2012
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2013
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2016
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2016
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2017
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2017
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2018
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