Detecting coalescences of intermediate-mass black holes in globular clusters with the Einstein Telescope
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🌌 astro-ph.CO
astro-ph.HEgr-qc
keywords
blackclusterseinsteinglobularholesintermediate-masstelescopecapability
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We discuss the capability of a third-generation ground-based detector such as the Einstein Telescope to detect mergers of intermediate-mass black holes that may have formed through runaway stellar collisions in globular clusters. We find that detection rates of 500 events per year are plausible.
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