TY - JOUR
T1 - Post-Newtonian Dynamics in Dense Star Clusters
T2 - Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers
AU - Rodriguez, Carl L.
AU - Amaro-Seoane, Pau
AU - Chatterjee, Sourav
AU - Rasio, Frederic A.
N1 - Publisher Copyright:
© 2018 American Physical Society.
Copyright:
Copyright 2018 Elsevier B.V., All rights reserved.
PY - 2018/4/10
Y1 - 2018/4/10
N2 - We present models of realistic globular clusters with post-Newtonian dynamics for black holes. By modeling the relativistic accelerations and gravitational-wave emission in isolated binaries and during three- and four-body encounters, we find that nearly half of all binary black hole mergers occur inside the cluster, with about 10% of those mergers entering the LIGO/Virgo band with eccentricities greater than 0.1. In-cluster mergers lead to the birth of a second generation of black holes with larger masses and high spins, which, depending on the black hole natal spins, can sometimes be retained in the cluster and merge again. As a result, globular clusters can produce merging binaries with detectable spins regardless of the birth spins of black holes formed from massive stars. These second-generation black holes would also populate any upper mass gap created by pair-instability supernovae.
AB - We present models of realistic globular clusters with post-Newtonian dynamics for black holes. By modeling the relativistic accelerations and gravitational-wave emission in isolated binaries and during three- and four-body encounters, we find that nearly half of all binary black hole mergers occur inside the cluster, with about 10% of those mergers entering the LIGO/Virgo band with eccentricities greater than 0.1. In-cluster mergers lead to the birth of a second generation of black holes with larger masses and high spins, which, depending on the black hole natal spins, can sometimes be retained in the cluster and merge again. As a result, globular clusters can produce merging binaries with detectable spins regardless of the birth spins of black holes formed from massive stars. These second-generation black holes would also populate any upper mass gap created by pair-instability supernovae.
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U2 - 10.1103/PhysRevLett.120.151101
DO - 10.1103/PhysRevLett.120.151101
M3 - Article
C2 - 29756855
AN - SCOPUS:85045306241
VL - 120
JO - Physical Review Letters
JF - Physical Review Letters
SN - 0031-9007
IS - 15
M1 - 151101
ER -