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Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers

Posted on December 21, 2017 by pau

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Curvature conditions for spatial isotropy
X-MRIs: Extremely Large Mass-Ratio Inspirals
Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries
Post-Newtonian Dynamics in Dense Star Clusters: Binary Black Holes in the LISA Band
Innermost stable circular orbit of spinning test particle in Kerr-AdS black hole background

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Go to Astro-GR Meetings

Astro-GR Meetings

Since 2005 I started organising meetings and workshops in astrophysics and GR. This site is simply a metapage where I collect the different links to the various meetings and workshops I have organised in the past and I will be organising in the next future.

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Institute of Multidisciplinary Mathematics

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Pau Amaro Seoane

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