How post-Newtonian dynamics shape the distribution of stationary binary black hole LISA sources in nearby globular clusters
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DOI: 10.1103/physrevd.99.063006
Abstract: We derive the observable gravitational wave (GW) peak frequency ($f$) distribution of binary black holes (BBHs) that currently reside inside their globular clusters (GCs), with and without 2.5 Post-Newtonian (2.5PN) effects included in the dynamical… read more here.
Keywords: lisa; distribution; lisa sources; globular clusters ... See more keywords