The tail effect in gravitational radiation-reaction: time non-locality and renormalization group evolution

J. S. Schwinger, “Brownian motion of a quantum oscillator,” J. Math. Phys

1961

Earlier work this paper cites.

L. V. Keldysh, “Diagram technique for nonequilibrium processes,” Zh. Eksp. Teor. Fiz

1965

Earlier work this paper cites.

K. S. Thorne, “Nonradial Pulsation of General-Relativistic Stellar Models.IV. The Weakfield Limit,” Astrophys. J

1969

Earlier work this paper cites.

W. L. Burke, “Gravitational Radiation Damping of Slowly Moving Systems Calculated Using Matched Asymptotic Expansions,” J. Math. Phys

1971

Earlier work this paper cites.

T. Appelquist, M. Dine, and I. J. Muzinich, “The Static Potential in Quantum Chromodynamics,” Phys. Lett

1977

Earlier work this paper cites.

L. Blanchet and T. Damour, “Tail Transported Temporal Correlations in the Dynamics of a Gravitating System,” Phys. Rev

1988

Earlier work this paper cites.

L. Blanchet and T. Damour, “Hereditary effects in gravitational radiation,” Phys. Rev

1992

Earlier work this paper cites.

L. Blanchet, “Time asymmetric structure of gravitational radiation,” Phys. Rev

1993

Earlier work this paper cites.

B. R. Iyer and C. M. Will, “PostNewtonian gravitational radiation reaction for two-body systems,” Phys. Rev. Lett

1993

Earlier work this paper cites.

L. Blanchet and G. Schaefer, “Gravitational wave tails and binary star systems,” Class. Quant. Grav

1993

Earlier work this paper cites.

B. R. Iyer and C. M. Will, “PostNewtonian gravitational radiation reaction for two-body systems: Nonspinning bodies,” Phys. Rev

1995

Earlier work this paper cites.

N. Brambilla, A. Pineda, J. Soto, and A. Vairo, “The Infrared behavior of the static potential in perturbative QCD,” Phys. Rev

1999

Earlier work this paper cites.

N. Brambilla, A. Pineda, J. Soto, and A. Vairo, “Potential NRQCD: An Effective theory for heavy quarkonium,” Nucl. Phys

2000

Earlier work this paper cites.

H. Tagoshi, A. Ohashi, and B. J. Owen, “Gravitational field and equations of motion of spinning compact binaries to 2.5 postNewtonian order,” Phys. Rev

2001

Earlier work this paper cites.

V. C. de Andrade, L. Blanchet, and G. Faye, “Third postNewtonian dynamics of compact binaries: Noetherian conserved quantities and equivalence between the harmonic coordinate and ADM Hamiltonian formalisms,” Class. Quant. Grav

2001

Earlier work this paper cites.

A. H. Hoang, A. V. Manohar, and I. W. Stewart, “The Running Coulomb potential and Lamb shift in QCD,” Phys. Rev

2001

Earlier work this paper cites.

T. Damour, P. Jaranowski, and G. Schaefer, “Equivalence between the ADM-Hamiltonian and the harmonic coordinates approaches to the third postNewtonian dynamics of compact binaries,” Phys. Rev

2002

Earlier work this paper cites.

Y. Itoh and T. Futamase, “New derivation of a third postNewtonian equation of motion for relativistic compact binaries without ambiguity,” Phys. Rev

2003

Earlier work this paper cites.

L. Blanchet, T. Damour, G. Esposito-Farese, and B. R. Iyer, “Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order,” Phys. Rev. Lett

2004

Earlier work this paper cites.

W. D. Goldberger and I. Z. Rothstein, “An Effective field theory of gravity for extended objects,” Phys.Rev

2006

Earlier work this paper cites.

R. A. Porto, “Post-Newtonian corrections to the motion of spinning bodies in NRGR,” Phys.Rev

2006

Earlier work this paper cites.

R. A. Porto and I. Z. Rothstein, “The Hyperfine Einstein-Infeld-Hoffmann potential,” Phys.Rev.Lett

2006

Earlier work this paper cites.

G. Faye, L. Blanchet, and A. Buonanno, “Higher-order spin effects in the dynamics of compact binaries. I. Equations of motion,” Phys.Rev

2006

Earlier work this paper cites.

A. V. Manohar and I. W. Stewart, “The Zero-Bin and Mode Factorization in Quantum Field Theory,” Phys. Rev

2007

Earlier work this paper cites.

J. B. Gilmore and A. Ross, “Effective field theory calculation of second post-Newtonian binary dynamics,” Phys. Rev

Original

2008

Cited alongside, same era.

R. A. Porto and I. Z. Rothstein, “Spin(1)Spin(2) Effects in the Motion of Inspiralling Compact Binaries at Third Order in the Post-Newtonian Expansion,” Phys.Rev

Original

2008

Cited alongside, same era.

R. A. Porto and I. Z. Rothstein, “Next to Leading Order Spin(1)Spin(1) Effects in the Motion of Inspiralling Compact Binaries,” Phys.Rev

Original

2008

Cited alongside, same era.

T. Damour, P. Jaranowski, and G. Schaefer, “Hamiltonian of two spinning compact bodies with next-to-leading order gravitational spin-orbit coupling,” Phys. Rev

Original

2008

Cited alongside, same era.

J. Steinhoff, S. Hergt, and G. Schaefer, “On the next-to-leading order gravitational spin(1)-spin(2) dynamics,” Phys.Rev

L. Blanchet, G. Faye, B. R. Iyer, and S. Sinha, “The Third post-Newtonian gravitational wave polarisations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits,” Class. Quant. Grav

Original

2012

Later among the works it cites.

A. Buonanno, G. Faye, and T. Hinderer, “Spin effects on gravitational waves from inspiraling compact binaries at second post-Newtonian order,” Phys. Rev

Original

2013

Later among the works it cites.

J. Hartung, J. Steinhoff, and G. Schaefer, “Next-to-next-to-leading order post-Newtonian linear-in-spin binary Hamiltonians,” Annalen Phys

Original

2013

Later among the works it cites.

S. Marsat, A. Bohe, G. Faye, and L. Blanchet, “Next-to-next-to-leading order spin-orbit effects in the equations of motion of compact binary systems,” Class. Quant. Grav

Original

2013

Later among the works it cites.