Understanding the fate of merging supermassive black holes

DOI10.1088/0264-9381/22/10/034zbMath1071.83538arXivastro-ph/0411744OpenAlexW3123076406WikidataQ56882230 ScholiaQ56882230MaRDI QIDQ4681508

Manuela Campanelli

Publication date: 23 June 2005

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0411744

Mathematics Subject Classification ID

Black holes (83C57) Gravitational waves (83C35)

Related Items (7)

Black-hole binaries, gravitational waves, and numerical relativity ⋮ SPIN EXPANSION FOR HEAD-ON COLLISION OF TWO BLACK HOLES ⋮ Gravitational radiation from post-Newtonian sources and inspiralling compact binaries ⋮ Colliding Black Holes and Gravitational Waves ⋮ Flux-balance equations for linear momentum and center-of-mass position of self-gravitating post-Newtonian systems ⋮ Black-hole puncture initial data with realistic gravitational wave content ⋮ Maximum Kick from Nonspinning Black-Hole Binary Inspiral

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