Intermediate-mass ratio inspirals in merging elliptical galaxies
Ver\'onica V\'azquez-Aceves, Pau Amaro Seoane, Dana Kuvatova, Maxim, Makukov, Chingis Omarov, Denis Yurin

TL;DR
This paper investigates the formation of intermediate mass-ratio inspirals (IMRIs) in merging elliptical galaxies with intermediate-mass black holes, estimating their formation rates and detectability by space-based gravitational wave detectors.
Contribution
It demonstrates that merging elliptical galaxies can efficiently produce IMRIs with detectable gravitational wave signals, providing new estimates of formation rates and detection prospects.
Findings
IMRI formation rates range from 10^{-8} to 10^{-5} per year.
Peak GW frequencies are within LISA and TianQin detection bands.
Significant number of IMRI detections expected annually.
Abstract
Close encounters between two initially unbound objects can result in a binary system if enough energy is released as gravitational waves (GWs). We address the scenario in which such encounters occur in merging elliptical galaxies. There is evidence that elliptical galaxies can harbor intermediate-mass black holes. Therefore, these systems are potentially the breeding grounds of sources of gravitational waves corresponding to inspiraling compact objects onto a massive black hole due to the dynamics, the large densities, and the number of compact remnants they contain. We show that this process is efficient for intermediate-mass black holes (IMBHs) with masses ranging from M M and results in the formation of intermediate mass-ratio inspirals (IMRIs). We consider a set of IMBHs and smaller black holes with masses M to estimate the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
