The DOI matches its Crossref record; 82 of the 82 references it cites were found in a registry or an index.
Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes
Open accessAbstract
In this paper we present imrphenomxas, a thorough overhaul of the imrphenomd [S. Husa et al., Phys. Rev. D 93, 044006 (2016); S. Khan et al., Phys. Rev. D 93, 044007 (2016)] waveform model, which describes the dominant $l=2$, $|m|=2$ spherical harmonic mode of nonprecessing coalescing black holes in terms of piecewise closed form expressions in the frequency domain. Improvements include in particular the accurate treatment of unequal spin effects, and the inclusion of extreme mass ratio waveforms. imrphenomd has previously been extended to approximately include spin precession [M. Hannam et al., Phys. Rev. Lett. 113, 151101 (2014)] and subdominant spherical harmonics [L. London et al., Phys. Rev. Lett. 120, 161102 (2018)], and with its extensions it has become a standard tool in gravitational wave parameter estimation. Improved extensions of imrphenomxas are discussed in companion papers [C. Garc\'{\i}a-Quir\'os et al., Phys. Rev. D 102, 064002 (2020); G. Pratten et al., arXiv:2004.06503].
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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
Self-citationAdvanced Virgo: a second-generation interferometric gravitational wave detector
Acernese, F., Agathos, M., Agatsuma, K., Aisa, D., Allemandou, N., Allocca, A., Amarni, J., Astone, P., Balestri, G., Ballardin, G., et al. (2015) · Classical and Quantum Gravity · doi:10.1088/0264-9381/32/2/024001 · Cited by 4,050
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) · Physical Review X · doi:10.1103/physrevx.9.031040 · Cited by 3,518
Self-citationThe LIGO Scientific Collaboration, Aasi, J., Abbott, B. P., Abbott, R., Abbott, T., Abernathy, M. R., Ackley, K., Adams, C., Adams, T., Addesso, P., et al. (2015) · Classical and Quantum Gravity · doi:10.1088/0264-9381/32/7/074001 · Cited by 3,356
Self-citationGravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
Blanchet, L. (2014) · Living Reviews in Relativity · doi:10.12942/lrr-2014-2 · Cited by 2,224
Quasinormal modes of black holes and black branes
Berti, E., Cardoso, V., & Starinets, A. O. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/16/163001 · Cited by 2,095
Quasi-Normal Modes of Stars and Black Holes
Kokkotas, K. D., & Schmidt, B. G. (1999) · Living Reviews in Relativity · doi:10.12942/lrr-1999-2 · Cited by 2,055
Cutler, C., & Flanagan, É. E. (1994) · Physical Review D · doi:10.1103/physrevd.49.2658 · Cited by 1,615
Accurate Evolutions of Orbiting Black-Hole Binaries without Excision
Campanelli, M., Lousto, C. O., Marronetti, P., & Zlochower, Y. (2006) · Physical Review Letters · doi:10.1103/physrevlett.96.111101 · Cited by 1,423
Effective one-body approach to general relativistic two-body dynamics
Buonanno, A., & Damour, T. (1999) · Physical Review D · doi:10.1103/physrevd.59.084006 · Cited by 1,311
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
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
Self-citationPratten, G., García-Quirós, C., Colleoni, M., Ramos-Buades, A., Estellés, H., Mateu-Lucena, M., Jaume, R., Haney, M., Keitel, D., Thompson, J. E., et al. (2021) · Physical Review D · doi:10.1103/physrevd.103.104056 · Cited by 555
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Metadata
- Authors
- Pratten, G., Husa, S., García-Quirós, C., Colleoni, M., Ramos-Buades, A., Estellés, H., & Jaume, R.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2020-09-02
- Volume
- 102
- Issue
- 6
- ISSN
- 2470-0010 (ISSN-L)
- 2470-0029
- OpenAlex
- W3003162054
- Cited by
- 285
- References
- 82
- FWCI
- 13.91
- Type
- journal article
- Language
- en
- Open access
- bronze
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