Intermediate-mass ratio inspirals in merging elliptical galaxies
Vázquez-Aceves V. Seoane P.A. Kuvatova D. Makukov M. Omarov C. Yurin D.
1 January 2023Oxford University Press
Monthly Notices of the Royal Astronomical Society
2023#518Issue 22113 - 2118 pp.
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 harbour intermediate-mass black holes (IMBHs). Therefore, these systems are potentially the breeding grounds of sources of GWs 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 IMBHs with masses ranging from M ∈ (103, 105) M⊙ and results in the formation of intermediate-mass ratio inspirals (IMRIs). We consider a set of IMBHs and smaller black holes with masses m2 ∈ (10, 103) M⊙ to estimate the IMRI formation rate. We find rates ranging between 10−8 and 10−5 yr−1, and the IMRI formation rate per comoving volume in merging galaxies as a function of the redshift. The peak frequencies of the gravitational radiation emitted when these IMRIs are formed are within the detection band of space-borne detectors such as the Laser Interferometer Space Antenna (LISA) and TianQin; taking into account the observable volume of these detectors, the total amount of IMRI detections per year is significant.
galaxies: interactions , gravitational waves , methods: analytical , stars: black holes
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Institute of Applied Mathematics, Academy of Mathematics and Systems Science, CAS, Beijing, 100190, China
Institute for Multidisciplinary Mathematics, UPV, València, 46022, Spain
Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, School of Physical Science and Technology, Lanzhou University, Lanzhou, 730000, China
Institute of Theoretical Physics, Research Center of Gravitation, Lanzhou University, Lanzhou, 730000, China
Kavli Institute for Astronomy and Astrophysics, Beijing, 100871, China
Fesenkov Astrophysical Institute, Almaty, 050020, Kazakhstan
Institute of Applied Mathematics
Institute for Multidisciplinary Mathematics
Lanzhou Center for Theoretical Physics
Institute of Theoretical Physics
Kavli Institute for Astronomy and Astrophysics
Fesenkov Astrophysical Institute
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