Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures. Gerosa, D., O'Shaughnessy, R., Kesden, M., Berti, E., & Sperhake, U. Physical Review D, 89(12):124025, June, 2014. doi bibtex @article{2014PhRvD..89l4025G,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {https://ui.adsabs.harvard.edu/abs/2014PhRvD..89l4025G},
archiveprefix = {arXiv},
author = {{Gerosa}, Davide and {O'Shaughnessy}, Richard and {Kesden}, Michael and {Berti}, Emanuele and {Sperhake}, Ulrich},
doi = {10.1103/PhysRevD.89.124025},
eid = {124025},
eprint = {1403.7147},
journal = {Physical Review D},
keywords = {04.25.dg, 04.70.Bw, 04.30.-w, Numerical studies of black holes and black-hole binaries, Classical black holes, Gravitational waves: theory, General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
month = jun,
number = {12},
pages = {124025},
primaryclass = {gr-qc},
title = {{Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures}},
volume = {89},
year = 2014,
bdsk-url-1 = {https://doi.org/10.1103/PhysRevD.89.124025}}
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