Abstract
Gravitational self-force techniques will be shortly reviewed along the lines of the two lectures presented by D. Bini at the 2019 edition of the “Domoschool.” The most important application of gravitational self-force concerns metric and curvature perturbations in black hole spacetimes due to moving particles or evolving fields. However, from a practical point of view (and for teaching purposes) we have chosen to perform the whole discussion at the level of a (massless) scalar field. In fact, in this simple case one can look at the various steps implicit in any self-force computation without facing with the additional difficulties of implementing them in a more involved tensorial background.
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Notes
- 1.
Note that PN solutions “do not know” the horizon at r = 2M, but they are sensitive to the origin r = 0 only. The horizon, in fact, will be a regular singular point of the radial equation only when all PN terms will be summed. Practically, we may say that high-PN orders already start “seeing” the horizon, marked by the presence of successive l − n diverging coefficients at various PN n orders.
References
L. Barack, A. Pound, Self-force and radiation reaction in general relativity. Rept. Prog. Phys. 82(1), 016904 (2019). https://doi.org/10.1088/1361-6633/aae552, ar**v:1805.10385 [gr-qc]
D. Bini, T. Damour, Analytical determination of the two-body gravitational interaction potential at the fourth post-Newtonian approximation. Phys. Rev. D 87(12), 121501 (2013). https://doi.org/10.1103/PhysRevD.87.121501, ar**v:1305.4884 [gr-qc]
E. Poisson, The Motion of point particles in curved space-time. Living Rev. Rel. 7, 6 (2004). https://doi.org/10.12942/lrr-2004-6, gr-qc/0306052
M. Sasaki, H. Tagoshi, Analytic black hole perturbation approach to gravitational radiation. Living Rev. Rel. 6, 6 (2003). https://doi.org/10.12942/lrr-2003-6, gr-qc/0306120
L. Barack, Gravitational self force in extreme mass-ratio inspirals. Class. Quant. Grav. 26, 213001 (2009). https://doi.org/10.1088/0264-9381/26/21/213001, ar**v:0908.1664 [gr-qc]
S.L. Detweiler, B.F. Whiting, Self-force via a Green’s function decomposition. Phys. Rev. D 67, 024025 (2003). https://doi.org/10.1103/PhysRevD.67.024025, gr-qc/0202086
T. Regge, J.A. Wheeler, Stability of a Schwarzschild singularity. Phys. Rev. 108, 1063 (1957). https://doi.org/10.1103/PhysRev.108.1063
F.J. Zerilli, Gravitational field of a particle falling in a Schwarzschild geometry analyzed in tensor harmonics. Phys. Rev. D 2, 2141 (1970). https://doi.org/10.1103/PhysRevD.2.2141
S.A. Teukolsky, Perturbations of a rotating black hole. 1. Fundamental equations for gravitational electromagnetic and neutrino field perturbations. Astrophys. J. 185, 635 (1973). https://doi.org/10.1086/152444
W.H. Press, S.A. Teukolsky, Perturbations of a Rotating Black Hole. II. Dynamical Stability of the Kerr Metric. Astrophys. J. 185, 649 (1973). https://doi.org/10.1086/152445
S.A. Teukolsky, W.H. Press, Perturbations of a rotating black hole. III - Interaction of the hole with gravitational and electromagnetic radiation. Astrophys. J. 193, 443 (1974). https://doi.org/10.1086/153180
S. Mano, H. Suzuki, E. Takasugi, Analytic solutions of the Regge-Wheeler equation and the post-Minkowskian expansion. Prog. Theor. Phys. 96, 549 (1996). gr-qc/9605057
S. Mano, H. Suzuki, E. Takasugi, Analytic solutions of the Teukolsky equation and their low frequency expansions. Prog. Theor. Phys. 95, 1079 (1996). gr-qc/9603020
J.M. Cohen, L.S. Kegeles, Electromagnetic fields in curved spaces - a constructive procedure. Phys. Rev. D 10, 1070 (1974). https://doi.org/10.1103/PhysRevD.10.1070
P.L. Chrzanowski, Vector Potential and metric perturbations of a rotating black hole. Phys. Rev. D 11, 2042 (1975). https://doi.org/10.1103/PhysRevD.11.2042
L.S. Kegeles, J.M. Cohen, Constructive procedure for perturbations of space-times. Phys. Rev. D 19, 1641 (1979). https://doi.org/10.1103/PhysRevD.19.1641
T.S. Keidl, A.G. Shah, J.L. Friedman, D.H. Kim, L.R. Price, Gravitational self-force in a radiation gauge. Phys. Rev. D 82(12), 124012 (2010). Erratum: Phys. Rev. D 90(10), 109902 (2014). https://doi.org/10.1103/PhysRevD.82.124012, https://doi.org/10.1103/PhysRevD.90.109902, ar**v:1004.2276 [gr-qc]
A.G. Shah, T.S. Keidl, J.L. Friedman, D.H. Kim, L.R. Price, Conservative, gravitational self-force for a particle in circular orbit around a Schwarzschild black hole in a Radiation Gauge. Phys. Rev. D 83, 064018 (2011). https://doi.org/10.1103/PhysRevD.83.064018, ar**v:1009.4876 [gr-qc]
A.G. Shah, J.L. Friedman, T.S. Keidl, EMRI corrections to the angular velocity and redshift factor of a mass in circular orbit about a Kerr black hole. Phys. Rev. D 86, 084059 (2012). https://doi.org/10.1103/PhysRevD.86.084059, ar**v:1207.5595 [gr-qc]
M. van de Meent, A.G. Shah, Metric perturbations produced by eccentric equatorial orbits around a Kerr black hole. Phys. Rev. D 92(6), 064025 (2015). https://doi.org/10.1103/PhysRevD.92.064025, ar**v:1506.04755 [gr-qc]
D. Bini, A. Geralico, Gauge-fixing for the completion problem of reconstructed metric perturbations of a Kerr spacetime. ar**v:1908.03191 [gr-qc]
M. Abramowitz, I. Stegun, Handbook of Mathematical Functions (Dover Publications Inc., New York, 1970)
S.L. Detweiler, E. Messaritaki, B.F. Whiting, Self-force of a scalar field for circular orbits about a Schwarzschild black hole. Phys. Rev. D 67, 104016 (2003). https://doi.org/10.1103/PhysRevD.67.104016, gr-qc/0205079
N. Sago, H. Nakano, M. Sasaki, Gauge problem in the gravitational self-force. 1. Harmonic gauge approach in the Schwarzschild background. Phys. Rev. D 67, 104017 (2003). https://doi.org/10.1103/PhysRevD.67.104017, gr-qc/0208060
H. Nakano, N. Sago, M. Sasaki, Gauge problem in the gravitational self-force. 2. First post-Newtonian force under Regge-Wheeler gauge. Phys. Rev. D 68, 124003 (2003). https://doi.org/10.1103/PhysRevD.68.124003, gr-qc/0308027
W. Hikida, H. Nakano, M. Sasaki, Self-force regularization in the Schwarzschild spacetime. Class. Quant. Grav. 22(15), S753 (2005). https://doi.org/10.1088/0264-9381/22/15/009, gr-qc/0411150
D. Bini, G. Carvalho, A. Geralico, Scalar field self-force effects on a particle orbiting a Reissner-Nordström black hole. Phys. Rev. D 94(12), 124028 (2016). https://doi.org/10.1103/PhysRevD.94.124028, ar**v:1610.02235 [gr-qc]
T. Damour, B.R. Iyer, A. Nagar, Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries. Phys. Rev. D 79, 064004 (2009), ar**v:0811.2069 [gr-qc]
L.M. Diaz-Rivera, E. Messaritaki, B.F. Whiting, S.L. Detweiler, Scalar field self-force effects on orbits about a Schwarzschild black hole. Phys. Rev. D 70, 124018 (2004), gr-qc/0410011
S. Akcay, L. Barack, T. Damour, N. Sago, Gravitational self-force and the effective-one-body formalism between the innermost stable circular orbit and the light ring. Phys. Rev. D 86, 104041 (2012). ar**v:1209.0964 [gr-qc]
S.L. Detweiler, A Consequence of the gravitational self-force for circular orbits of the Schwarzschild geometry. Phys. Rev. D 77, 124026 (2008). https://doi.org/10.1103/PhysRevD.77.124026, ar**v:0804.3529 [gr-qc] s
D. Bini, T. Damour, High-order post-Newtonian contributions to the two-body gravitational interaction potential from analytical gravitational self-force calculations. Phys. Rev. D 89(6), 064063 (2014). https://doi.org/10.1103/PhysRevD.89.064063, ar**v:1312.2503 [gr-qc]
D. Bini, T. Damour, Analytic determination of the eight-and-a-half post-Newtonian self-force contributions to the two-body gravitational interaction potential. Phys. Rev. D 89(10), 104047 (2014). https://doi.org/10.1103/PhysRevD.89.104047, ar**v:1403.2366 [gr-qc]
D. Bini, T. Damour, Detweiler’s gauge-invariant redshift variable: Analytic determination of the nine and nine-and-a-half post-Newtonian self-force contributions. Phys. Rev. D 91, 064050 (2015). https://doi.org/10.1103/PhysRevD.91.064050, ar**v:1502.02450 [gr-qc]
C. Kavanagh, A.C. Ottewill, B. Wardell, Analytical high-order post-Newtonian expansions for extreme mass ratio binaries. Phys. Rev. D 92(8), 084025 (2015). https://doi.org/10.1103/PhysRevD.92.084025, ar**v:1503.02334 [gr-qc]
D. Bini, T. Damour, A. Geralico, Confirming and improving post-Newtonian and effective-one-body results from self-force computations along eccentric orbits around a Schwarzschild black hole. Phys. Rev. D 93(6), 064023 (2016). https://doi.org/10.1103/PhysRevD.93.064023, ar**v:1511.04533 [gr-qc]
D. Bini, T. Damour, A. Geralico, New gravitational self-force analytical results for eccentric orbits around a Schwarzschild black hole. Phys. Rev. D 93(10), 104017 (2016). https://doi.org/10.1103/PhysRevD.93.104017 ar**v:1601.02988 [gr-qc]
D. Bini, T. Damour, A. Geralico, Novel approach to binary dynamics: application to the fifth post-Newtonian level. Phys. Rev. Lett. 123(23), 231104 (2019). https://doi.org/10.1103/PhysRevLett.123.231104, ar**v:1909.02375 [gr-qc]
D. Bini, T. Damour, Two-body gravitational spin-orbit interaction at linear order in the mass ratio. Phys. Rev. D 90(2), 024039 (2014). https://doi.org/10.1103/PhysRevD.90.024039, ar**v:1404.2747 [gr-qc]
D. Bini, T. Damour, Analytic determination of high-order post-Newtonian self-force contributions to gravitational spin precession. Phys. Rev. D 91(6), 064064 (2015). https://doi.org/10.1103/PhysRevD.91.064064, ar**v:1503.01272 [gr-qc]
C. Kavanagh, D. Bini, T. Damour, S. Hopper, A.C. Ottewill, B. Wardell, Spin-orbit precession along eccentric orbits for extreme mass ratio black hole binaries and its effective-one-body transcription. Phys. Rev. D 96(6), 064012 (2017). https://doi.org/10.1103/PhysRevD.96.064012, ar**v:1706.00459 [gr-qc]
D. Bini, T. Damour, A. Geralico, Spin-orbit precession along eccentric orbits: improving the knowledge of self-force corrections and of their effective-one-body counterparts. Phys. Rev. D 97(10), 104046 (2018). https://doi.org/10.1103/PhysRevD.97.104046, ar**v:1801.03704 [gr-qc]
T. Damour, Gravitational self-force in a Schwarzschild background and the effective one body formalism. Phys. Rev. D 81, 024017 (2010). https://doi.org/10.1103/PhysRevD.81.024017, ar**v:0910.5533 [gr-qc]
D. Bini, T. Damour, Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism. Phys. Rev. D 90, 124037 (2014). https://doi.org/10.1103/PhysRevD.90.124037, ar**v:1409.6933 [gr-qc]
S.R. Dolan, P. Nolan, A.C. Ottewill, N. Warburton, B. Wardell, Tidal invariants for compact binaries on quasicircular orbits. Phys. Rev. D 91, 023009 (2015). https://doi.org/10.1103/PhysRevD.91.023009, ar**v:1406.4890 [gr-qc]
P. Nolan, C. Kavanagh, S.R. Dolan, A.C. Ottewill, N. Warburton, B. Wardell, Octupolar invariants for compact binaries on quasicircular orbits. Phys. Rev. D 92, 123008 (2015). https://doi.org/10.1103/PhysRevD.92.123008, ar**v:1505.04447 [gr-qc]
A.G. Shah, A. Pound, Linear-in-mass-ratio contribution to spin precession and tidal invariants in Schwarzschild spacetime at very high post-Newtonian order. Phys. Rev. D 91(12), 124022 (2015). https://doi.org/10.1103/PhysRevD.91.124022, ar**v:1503.02414 [gr-qc]
D. Bini, A. Geralico, Gravitational self-force corrections to tidal invariants for particles on eccentric orbits in a Schwarzschild spacetime. Phys. Rev. D 98(6), 064026 (2018). https://doi.org/10.1103/PhysRevD.98.064026, ar**v:1806.06635 [gr-qc]
A.G. Shah, Talk delivered at the XIV Marcel Grossmann meeting, Rome (2015)
D. Bini, T. Damour, A. Geralico, Spin-dependent two-body interactions from gravitational self-force computations. Phys. Rev. D 92(12), 124058 (2015). Erratum: Phys. Rev. D 93(10), 109902 (2016). https://doi.org/10.1103/PhysRevD.93.109902, https://doi.org/10.1103/PhysRevD.92.124058, ar**v:1510.06230 [gr-qc]
C. Kavanagh, A.C. Ottewill, B. Wardell, Analytical high-order post-Newtonian expansions for spinning extreme mass ratio binaries. Phys. Rev. D 93(12), 124038 (2016). https://doi.org/10.1103/PhysRevD.93.124038, ar**v:1601.03394 [gr-qc]
D. Bini, T. Damour, A. Geralico, High post-Newtonian order gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole. Phys. Rev. D 93(12), 124058 (2016). https://doi.org/10.1103/PhysRevD.93.124058, ar**v:1602.08282 [gr-qc]
D. Bini, A. Geralico, New gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole: redshift invariant. Phys. Rev. D 100(10), 104002 (2019). https://doi.org/10.1103/PhysRevD.100.104002, ar**v:1907.11080 [gr-qc]
D. Bini, T. Damour, A. Geralico, C. Kavanagh, M. van de Meent, Gravitational self-force corrections to gyroscope precession along circular orbits in the Kerr spacetime. Phys. Rev. D 98(10), 104062 (2018). https://doi.org/10.1103/PhysRevD.98.104062, ar**v:1809.02516 [gr-qc]
D. Bini, A. Geralico, New gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole: gyroscope precession. Phys. Rev. D 100(10), 104003 (2019). https://doi.org/10.1103/PhysRevD.100.104003, ar**v:1907.11082 [gr-qc]
M. van de Meent, Self-force corrections to the periapsis advance around a spinning black hole. Phys. Rev. Lett. 118(1), 011101 (2017). https://doi.org/10.1103/PhysRevLett.118.011101, ar**v:1610.03497 [gr-qc]
D. Bini, A. Geralico, Analytical determination of the periastron advance in spinning binaries from self-force computations. Phys. Rev. D 100(12), 121502 (2019). https://doi.org/10.1103/PhysRevD.100.121502, ar**v:1907.11083 [gr-qc]
D. Bini, A. Geralico, Gravitational self-force corrections to tidal invariants for particles on circular orbits in a Kerr spacetime. Phys. Rev. D 98(6), 064040 (2018). https://doi.org/10.1103/PhysRevD.98.064040, ar**v:1806.08765 [gr-qc]
A. Buonanno, T. Damour, Effective one-body approach to general relativistic two-body dynamics. Phys. Rev. D 59, 084006 (1999). https://doi.org/10.1103/PhysRevD.59.084006, gr-qc/9811091
A. Buonanno, T. Damour, Transition from inspiral to plunge in binary black hole coalescences. Phys. Rev. D 62, 064015 (2000). https://doi.org/10.1103/PhysRevD.62.064015, gr-qc/0001013
Acknowledgements
We thank Thibault Damour for helpful discussions on analytical self-force computations.
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Bini, D., Geralico, A. (2022). Gravitational Self-force in the Schwarzschild Spacetime. In: Cacciatori, S.L., Kamenshchik, A. (eds) Einstein Equations: Local Energy, Self-Force, and Fields in General Relativity. Tutorials, Schools, and Workshops in the Mathematical Sciences . Birkhäuser, Cham. https://doi.org/10.1007/978-3-031-21845-3_2
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