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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