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

Carl L Rodriguez1, Pau Amaro-Seoane2, Sourav Chatterjee3

  • 1Massachusetts Institute of Technology-Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, 37-664H, Cambridge, Massachusetts 02139, USA.

Physical Review Letters
|May 15, 2018
PubMed

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