A generalized precession parameter \ensuremathḩi$_{p}$ to interpret gravitational-wave data. Gerosa, D., Mould, M., Gangardt, D., Schmidt, P., Pratten, G., & Thomas, L. M. Physical Review D, 103(6):064067, March, 2021.
doi  bibtex   
@article{2021PhRvD.103f4067G,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2021PhRvD.103f4067G},
	archiveprefix = {arXiv},
	author = {{Gerosa}, Davide and {Mould}, Matthew and {Gangardt}, Daria and {Schmidt}, Patricia and {Pratten}, Geraint and {Thomas}, Lucy M.},
	doi = {10.1103/PhysRevD.103.064067},
	eid = {064067},
	eprint = {2011.11948},
	journal = {Physical Review D},
	keywords = {General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
	month = mar,
	number = {6},
	pages = {064067},
	primaryclass = {gr-qc},
	title = {{A generalized precession parameter {\ensuremath{\chi}}$_{p}$ to interpret gravitational-wave data}},
	volume = {103},
	year = 2021,
	Bdsk-Url-1 = {https://doi.org/10.1103/PhysRevD.103.064067}}

Downloads: 0