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- W3108577772 endingPage "3642" @default.
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- W3108577772 abstract "With projects such as Laser Interferometer Space Antenna (LISA) and Pulsar Timing Arrays expected to detect gravitational waves from supermassive black hole mergers in the near future, it is key that we understand what we expect those detections to be, and maximize what we can learn from them. To address this, we study the mergers of supermassive black holes in the Illustris simulation, the overall rate of mergers, and the correlation between merging black holes and their host galaxies. We find that these mergers occur in typical galaxies along the $M_{rm{BH}}-M_*$ relation, and that between LISA and PTAs we expect to probe the full range of galaxy masses. As galaxy mergers can trigger increased star formation, we find that galaxies hosting low-mass black hole mergers tend to show a slight increase in star formation rates compared to a mass-matched sample. However, high-mass merger hosts have typical star formation rates, due to a combination of low gas fractions and powerful AGN feedback. Although minor black hole mergers do not correlate with disturbed morphologies, major mergers (especially at high-masses) tend to show morphological evidence of recent galaxy mergers which survives for ~500 Myr. This is on the same scale as the infall/hardening time of the merging black holes, suggesting that electromagnetic followups to gravitational wave signals may not be able to observe this correlation. We further find that incorporating a realistic timescale delay for the black hole mergers could shift the distribution of merger masses toward higher-masses, decreasing the rate of LISA detections while increasing the rate of PTA detections." @default.
- W3108577772 created "2020-12-07" @default.
- W3108577772 creator A5004531924 @default.
- W3108577772 creator A5006709063 @default.
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- W3108577772 creator A5023087030 @default.
- W3108577772 creator A5035375830 @default.
- W3108577772 creator A5066582692 @default.
- W3108577772 date "2021-03-22" @default.
- W3108577772 modified "2023-10-14" @default.
- W3108577772 title "Morphological evolution of supermassive black hole merger hosts and multimessenger signatures" @default.
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- W3108577772 doi "https://doi.org/10.1093/mnras/stab721" @default.
- W3108577772 hasPublicationYear "2021" @default.