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Comparing second-order gravitational self-force and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

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Detalles Bibliográficos
Autores principales:	Albertini, Angelica, Nagar, Alessandro, Mathews, Josh, Lukes-Gerakopoulos, Georgios
Formato:	Preprint
Publicado:	2024
Materias:	General Relativity and Quantum Cosmology
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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