Laying the foundation of the effective-one-body waveform models SEOBNRv5: Improved accuracy and efficiency for spinning nonprecessing binary black holes
Lorenzo Pompili(Max Planck Institute for Gravitational Physics), Jennifer Sánchez(Northwestern University), Maarten van de Meent(Max Planck Institute for Gravitational Physics), Michael Boyle(California Institute of Technology), Sierra Thomas(California State University, Fullerton), Sizheng Ma(California Institute of Technology), Mohammed Khalil(Perimeter Institute), A. K. Mehta(Tata Institute of Fundamental Research), Keefe Mitman(California Institute of Technology), Deyan P. Mihaylov(Max Planck Institute for Gravitational Physics), Harald Pfeiffer(Max Planck Institute for Gravitational Physics), Nils L. Vu(California Institute of Technology), Reetika Dudi(Max Planck Institute for Gravitational Physics), D. A. Melchor(California State University, Fullerton), Mark Scheel(California Institute of Technology), R. Cotesta(Max Planck Institute for Gravitational Physics), A. Ramos-Buades(Pennsylvania State University), H. Estellés(Universitat de les Illes Balears), Hannes R. Rüter(University of Coimbra), M. Pürrer(Cardiff University), Serguei Ossokine(Max Planck Institute for Gravitational Physics), S. Marsat(Centre National de la Recherche Scientifique), Larry Kidder(Cornell University), Alessandra Buonanno(Centre National de la Recherche Scientifique)
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