The complete non-spinning effective-one-body metric at linear order in the mass ratio
Thursday, November 24th, 2011by Barausse, Enrico and Buonanno, Alessandra and Tiec, Alexandre Le
11 pages, 2 figures
Editors: Pau Amaro-Seoane & Bernard Schutz
The
last GW Note is by Jonathan Thornburg
Archive for the ‘post-Newtonian theory’ Category
The First Law of Binary Black Hole Mechanics in General Relativity and Post-Newtonian Theory
Thursday, November 24th, 2011by Tiec, Alexandre Le and Blanchet, Luc and Whiting, Bernard F.
43 pages, 3 figures
Analytical meets numerical relativity – status of complete gravitational waveform models
Thursday, November 17th, 2011Importance of including small body spin effects in the modelling of intermediate mass-ratio inspirals. II Accurate parameter extraction of strong sources using higher-order spin effects
Tuesday, November 15th, 2011by Huerta, E. A. and Gair, Jonathan R. and Brown, Duncan A.
22 pages, 3 figures. Submitted to Phys. Rev. D. arXiv admin note: substantial text overlap with arXiv:1105.3567
Energy versus Angular Momentum in Black Hole Binaries
Friday, October 14th, 2011by Damour, Thibault and Nagar, Alessandro and Pollney, Denis and Reisswig, Christian
4 pages, 2 figures
Elimination of the spin supplementary condition in the effective field theory approach to the post-Newtonian approximation
Wednesday, October 12th, 2011by Hergt, Steven and Steinhoff, Jan and Schaefer, Gerhard
37 pages, submitted
Accurate gravitational waveforms for binary-black-hole mergers with nearly extremal spins
Wednesday, October 12th, 2011by Lovelace, Geoffrey and Boyle, Michael and Scheel, Mark A. and Szilagyi, Bela
17 pages, 7 figures, submitted to Classical and Quantum Gravity
The butterfly effect in the extreme-mass ratio inspiral problem
Monday, August 29th, 2011by Amaro-Seoane, Pau and Brem, Patrick and Cuadra, Jorge and Armitage, Philip J.
Submitted
Stability and chaos of hierarchical three black hole configurations
Wednesday, August 24th, 2011The gravitational-wave memory from eccentric binaries
Thursday, August 18th, 2011Binary dynamics from spin1-spin2 coupling at fourth post-Newtonian order
Friday, July 22nd, 2011Next-to-next-to-leading order post-Newtonian spin(1)-spin(2) Hamiltonian for self-gravitating binaries
Friday, July 22nd, 2011Effective one body Hamiltonian of two spinning black-holes with next-to-next-to-leading order spin-orbit coupling
Thursday, June 23rd, 2011Periastron Advance in Black Hole Binaries
Sunday, June 19th, 2011by Tiec, Alexandre Le and Mroué, Abdul H. and Barack, Leor and Buonanno, Alessandra and Pfeiffer, Harald P. and Sago, Norichika and Taracchini, Andrea
5 pages, 3 figures
Tail-induced spin-orbit effect in the gravitational radiation of compact binaries
Monday, May 2nd, 2011by Blanchet, Luc and Buonanno, Alessandra and Faye, Guillaume
Submitted to Physical Review D
Gravitational radiation for extreme mass ratio inspirals to the 14th post-Newtonian order
Monday, May 2nd, 2011Accuracy of the post-Newtonian approximation. II. Optimal asymptotic expansion of the energy flux for quasicircular, extreme mass-ratio inspirals into a Kerr black hole
Saturday, April 2nd, 2011by Zhang, Zhongyang and Yunes, Nicolas and Berti, Emanuele
9 pages, 8 figures
On the unreasonable effectiveness of the post-Newtonian approximation in gravitational physics
Monday, February 28th, 2011by Will, Clifford M.
9 pages, 2 figures, submitted to Proceedings of the National Academy of Sciences (US)
Black-hole binaries go to eleven orbits
Monday, January 10th, 2011by Sperhake, Ulrich and Bruegmann, Bernd and Mueller, Doreen and Sopuerta, Carlos F.
Submitted to CQG, Special Edition for NRDA/CAPRA 2010, 13 pages, 7 figures
Conservative corrections to the innermost stable circular orbit (ISCO) of a Kerr black hole: a new gauge-invariant post-Newtonian ISCO condition, and the ISCO shift due to test-particle spin and the gravitational self-force
Thursday, October 14th, 2010Accuracy and effectualness of closed-form, frequency-domain waveforms for non-spinning black hole binaries
Friday, October 1st, 2010Conservative self-force correction to the innermost stable circular orbit: comparison with multiple post-Newtonian-based methods
Monday, August 30th, 2010Length requirements for numerical-relativity waveforms
Thursday, August 19th, 2010by Hannam, Mark and Husa, Sascha and Ohme, Frank and Ajith, P.
13 pages, 11 figures, 2 tables
Precession effect of the gravitational self-force in a Schwarzschild spacetime and the effective one-body formalism
Monday, August 9th, 2010by Barack, Leor and Damour, Thibault and Sago, Norichika
25 pages, 5 eps figures
High-Accuracy Comparison between the Post-Newtonian and Self-Force Dynamics of Black-Hole Binaries
Friday, July 16th, 2010by Blanchet, Luc and Detweiler, Steven and Tiec, Alexandre Le and Whiting, Bernard F.
29 pages, 3 figures; to appear in the book “Mass and Motion in General Relativity”, proceedings of the C.N.R.S. School in Orleans, France, eds. L. Blanchet, A. Spallicci and B. F. Whiting
A hybrid method for understanding black-hole mergers: head-on case
Thursday, July 15th, 2010by Nichols, David A. and Chen, Yanbei
13 pages, 6 figures, 1 table, revtex4 format
Full-analytic frequency-domain 1pN-accurate gravitational wave forms from eccentric compact binaries
Tuesday, June 22nd, 2010Statistical constraints on binary black hole inspiral dynamics
Tuesday, June 15th, 2010by Galley, Chad R. and Herrmann, Frank and Silberholz, John and Tiglio, Manuel and Guerberoff, Gustavo
Supermassive black hole spin-flip during the inspiral
Monday, May 17th, 2010by Gergely, László Á. and Biermann, Peter L. and Caramete, Laurenţiu I.
11 pages, 2 figures
Spin effects in the phasing of gravitational waves from binaries on eccentric orbits
Monday, May 17th, 2010by Klein, Antoine and Jetzer, Philippe
7 pages, 1 figure; Accepted for publication in Phys. Rev. D