Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: Comparable mass, nonspinning case. Islam, T., Varma, V., Lodman, J., Field, S. E., Khanna, G., Scheel, M. A., Pfeiffer, H. P., Gerosa, D., & Kidder, L. E. Physical Review D, 103(6):064022, March, 2021.
doi  bibtex   
@article{2021PhRvD.103f4022I,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2021PhRvD.103f4022I},
	archiveprefix = {arXiv},
	author = {{Islam}, Tousif and {Varma}, Vijay and {Lodman}, Jackie and {Field}, Scott E. and {Khanna}, Gaurav and {Scheel}, Mark A. and {Pfeiffer}, Harald P. and {Gerosa}, Davide and {Kidder}, Lawrence E.},
	doi = {10.1103/PhysRevD.103.064022},
	eid = {064022},
	eprint = {2101.11798},
	journal = {Physical Review D},
	keywords = {General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
	month = mar,
	number = {6},
	pages = {064022},
	primaryclass = {gr-qc},
	title = {{Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: Comparable mass, nonspinning case}},
	volume = {103},
	year = 2021,
	bdsk-url-1 = {https://doi.org/10.1103/PhysRevD.103.064022}}

Downloads: 0