Cite
Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries
MLA
Albertini, Angelica, et al. Comparing Second-Order Gravitational Self-Force, Numerical Relativity and Effective One Body Waveforms from Inspiralling, Quasi-Circular and Nonspinning Black Hole Binaries. 2022. EBSCOhost, https://doi.org/10.1103/PhysRevD.106.084061.
APA
Albertini, A., Nagar, A., Pound, A., Warburton, N., Wardell, B., Durkan, L., & Miller, J. (2022). Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries. https://doi.org/10.1103/PhysRevD.106.084061
Chicago
Albertini, Angelica, Alessandro Nagar, Adam Pound, Niels Warburton, Barry Wardell, Leanne Durkan, and Jeremy Miller. 2022. “Comparing Second-Order Gravitational Self-Force, Numerical Relativity and Effective One Body Waveforms from Inspiralling, Quasi-Circular and Nonspinning Black Hole Binaries.” doi:10.1103/PhysRevD.106.084061.