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Next to leading order spin(1)spin(1) effects in the motion of inspiralling compact binaries
Open accessAbstract
Using effective field theory techniques we compute the next to leading order Spin(1)Spin(1) terms in the potential of spinning compact objects at third post-Newtonian (PN) order, including subleading self-induced finite size effects. This result represents the last ingredient to complete the relevant spin potentials to 3PN order from which the equations of motion follow via a canonical formalism. As an example we include the precession equation.
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Citations
Cited by
Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
Blanchet, L. (2006) · Living Reviews in Relativity · doi:10.12942/lrr-2006-4 · Cited by 686
The effective field theorist’s approach to gravitational dynamics
Porto, R. A. (2016) · Physics Reports · doi:10.1016/j.physrep.2016.04.003 · Cited by 443
Self-citationArun, K. G., Buonanno, A., Faye, G., & Ochsner, E. (2009) · Physical Review D · doi:10.1103/physrevd.79.104023 · Cited by 347
Probing ultralight bosons with binary black holes
Baumann, D., Chia, H. S., & Porto, R. A. (2019) · Physical Review D · doi:10.1103/physrevd.99.044001 · Cited by 294
Self-citationPrototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
Taracchini, A., Pan, Y., Buonanno, A., Barausse, E., Boyle, M., Chu, T., Lovelace, G., Pfeiffer, H. P., & Scheel, M. A. (2012) · Physical Review D · doi:10.1103/physrevd.86.024011 · Cited by 255
Metadata
- Authors
- Porto, R. A., & Rothstein, I. Z.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2008-08-07
- Volume
- 78
- Issue
- 4
- ISSN
- 0556-2821 (ISSN-L)
- 1550-7998
- 1550-2368
- OpenAlex
- W4247306364
- Cited by
- 207
- References
- 0
- FWCI
- 6.48
- Type
- journal article
- Language
- en
- Open access
- green
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