Relativistic gas accretion onto supermassive black hole binaries from inspiral through merger
Year: 2025
Type: article
DOI: 10.1103/yc25-v1q4
Authors: Lorenzo Ennoggi, Manuela Campanelli, Yosef Zlochower, Scott C. Noble, Julian Krolik, Federico Cattorini, Jay V. Kalinani, Vassilios Mewes, Michail Chabanov, Liwei Ji, Maria Chiara de Simone
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: closed
Awards: G1011805105, G203625172, Collaborative Research: Deploying Curvilinear Coordinate and Multipatch Methods on Neutron Star Mergers, WoU-MMA: Collaborative Research: Supermassive Binary Black Holes: Accretion Dynamics and Electromagnetic Output, WoU-MMA: Collaborative Research: Supermassive Binary Black Hole Mergers: Accretion Dynamics and Electromagnetic Output, G3886122786, MRI: Acquisition of an Advanced Computer Cluster for Computational Relativity and Gravitation, G4524147383, MRI: Acquisition of an Advanced Computing Cluster for General Relativistic Astrophysics, Collaborative Research: Deploying Curvilinear Coordinate and Multipatch Methods on Neutron Star Mergers, MRI: Acquisition of a Computing Cluster for Gravitational-Wave and Multimessenger Astrophysics in the Era of LIGO Detections, Collaborative research: Frameworks: The Einstein Toolkit ecosystem: Enabling fundamental research in the era of multi-messenger astrophysics, Leveraging Curvilinear Coordinates for Long-term and Accurate Simulations of Compact Binary Inspirals and Mergers, MRI: Acquisition of a Computing System for Large Simulation Data Sets in Multimessenger Astrophysics
OpenAlex ID: W4413061917