The DOI matches its Crossref record; 43 of the 43 references it cites were found in a registry or an index.
Binary Black Hole Mergers from Field Triples: Properties, Rates, and the Impact of Stellar Evolution
Open accessAbstract
We consider the formation of binary black hole (BH) mergers through the evolution of field massive triple stars. In this scenario, favorable conditions for the inspiral of a BH binary are initiated by its gravitational interaction with a distant companion, rather than by a common-envelope phase invoked in standard binary evolution models. We use a code that follows self-consistently the evolution of massive triple stars, combining the secular triple dynamics (Lidov–Kozai cycles) with stellar evolution. After a BH triple is formed, its dynamical evolution is computed using either the orbit-averaged equations of motion, or a high-precision direct integrator for triples with weaker hierarchies for which the secular perturbation theory breaks down. Most BH mergers in our models are produced in the latter non-secular dynamical regime. We derive the properties of the merging binaries and compute a BH merger rate in the range (0.3–1.3) Gpc−3 yr−1, or up to ≈2.5 Gpc−3 yr−1 if the BH orbital planes have initially random orientation. Finally, we show that BH mergers from the triple channel have significantly higher eccentricities than those formed through the evolution of massive binaries or in dense star clusters. Measured eccentricities could therefore be used to uniquely identify binary mergers formed through the evolution of triple stars. While our results suggest up to ≈10 detections per year with Advanced-LIGO, the high eccentricities could render the merging binaries harder to detect with planned space based interferometers such as LISA.
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Cites
Observation of Gravitational Waves from a Binary Black Hole Merger
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.061102 · Cited by 14,151
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.241103 · Cited by 3,435
Secular perturbations of asteroids with high inclination and eccentricity
Kozai, Y. (1962) · The Astronomical Journal · doi:10.1086/108790 · Cited by 2,588
Gravitational Radiation and the Motion of Two Point Masses
Peters, P. C. (1964) · Physical Review · doi:10.1103/physrev.136.b1224 · Cited by 2,394
Binary Interaction Dominates the Evolution of Massive Stars
Sana, H., de Mink, S. E., de Koter, A., Langer, N., Evans, C. J., Gieles, M., Gosset, E., Izzard, R. G., Le Bouquin, J.-B., & Schneider, F. R. N. (2012) · Science · doi:10.1126/science.1223344 · Cited by 2,118
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Kroupa, P. (2002) · Science · doi:10.1126/science.1067524 · Cited by 1,793
Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
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Cited by
Abbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., et al. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab3800 · Cited by 895
Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences
Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, A., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., et al. (2021) · Institutional Repository of Leibniz Universität Hannover (Leibniz Universität Hannover) · doi:10.15488/11385 · Cited by 609
Astrophysics with the Laser Interferometer Space Antenna
Amaro-Seoane, P., Andrews, J., Arca Sedda, M., Askar, A., Baghi, Q., Balasov, R., Bartos, I., Bavera, S. S., Bellovary, J., Berry, C. P. L., et al. (2023) · Living Reviews in Relativity · doi:10.1007/s41114-022-00041-y · Cited by 609
Self-citation
Metadata
- Authors
- Antonini, F., Toonen, S., & Hamers, A. S.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2017-05-25
- Volume
- 841
- Issue
- 2
- Pages
- 77
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2611817759
- Cited by
- 328
- References
- 43
- FWCI
- 18.31
- Type
- journal article
- Language
- en
- Open access
- bronze
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