Effective Potentials and Morphological Transitions for Binary Black Hole Spin Precession. Kesden, M., Gerosa, D., O'Shaughnessy, R., Berti, E., & Sperhake, U. Physical Review Letters, 114(8):081103, February, 2015.
doi  bibtex   
@article{2015PhRvL.114h1103K,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2015PhRvL.114h1103K},
	archiveprefix = {arXiv},
	author = {{Kesden}, Michael and {Gerosa}, Davide and {O'Shaughnessy}, Richard and {Berti}, Emanuele and {Sperhake}, Ulrich},
	doi = {10.1103/PhysRevLett.114.081103},
	eid = {081103},
	eprint = {1411.0674},
	journal = {Physical Review Letters},
	keywords = {04.25.dg, 04.30.-w, 04.70.Bw, Numerical studies of black holes and black-hole binaries, Gravitational waves: theory, Classical black holes, General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
	month = feb,
	number = {8},
	pages = {081103},
	primaryclass = {gr-qc},
	title = {{Effective Potentials and Morphological Transitions for Binary Black Hole Spin Precession}},
	volume = {114},
	year = 2015,
	Bdsk-Url-1 = {https://doi.org/10.1103/PhysRevLett.114.081103}}

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