Gravitational waves and intermediate-mass black hole retention in globular clusters
The recent discovery of gravitational waves (GWs) has opened new horizons for physics. Current and upcoming missions, such as LIGO, VIRGO, KAGRA, and LISA, promise to shed light on black holes of every size from stellar mass (SBH) sizes up to supermassive black holes. The intermediate-mass black hol...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
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IOP Publishing
2018
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| _version_ | 1797097065259466752 |
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| author | Fragione, G Ginsburg, I Kocsis, B |
| author_facet | Fragione, G Ginsburg, I Kocsis, B |
| author_sort | Fragione, G |
| collection | OXFORD |
| description | The recent discovery of gravitational waves (GWs) has opened new horizons for physics. Current and upcoming missions, such as LIGO, VIRGO, KAGRA, and LISA, promise to shed light on black holes of every size from stellar mass (SBH) sizes up to supermassive black holes. The intermediate-mass black hole (IMBH) family has not been detected beyond any reasonable doubt. Recent analyses suggest observational evidence for the presence of IMBHs in the centers of two Galactic globular clusters (GCs). In this paper, we investigate the possibility that GCs were born with a central IMBH, which undergoes repeated merger events with SBHs in the cluster core. By means of a semi-analytical method, we follow the evolution of the primordial cluster population in the galactic potential and the mergers of the binary IMBH-SBH systems. Our models predict ≈1000 IMBHs within 1 kpc from the galactic center and show that the IMBH-SBH merger rate density changes from ${ \mathcal R }\approx 1000$ Gpc−3 yr−1 beyond z ≈ 2 to ${ \mathcal R }\approx 1\mbox{--}10$ Gpc−3 yr−1 at z ≈ 0. The rates at low redshifts may be significantly higher if young massive star clusters host IMBHs. The merger rates are dominated by IMBHs with masses between 103 and 104 M⊙. Currently, there are no LIGO/VIRGO upper limits for GW sources in this mass range, but our results show that at design sensitivity, these instruments will detect IMBH-SBH mergers in the coming years. LISA and the Einstein Telescope will be best suited to detect these events. The inspirals of IMBH-SBH systems may also generate an unresolved GW background. |
| first_indexed | 2024-03-07T04:50:22Z |
| format | Journal article |
| id | oxford-uuid:d4bc0283-cd7e-457a-ae06-d3370c49ff2b |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T04:50:22Z |
| publishDate | 2018 |
| publisher | IOP Publishing |
| record_format | dspace |
| spelling | oxford-uuid:d4bc0283-cd7e-457a-ae06-d3370c49ff2b2022-03-27T08:20:52ZGravitational waves and intermediate-mass black hole retention in globular clustersJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:d4bc0283-cd7e-457a-ae06-d3370c49ff2bEnglishSymplectic ElementsIOP Publishing2018Fragione, GGinsburg, IKocsis, BThe recent discovery of gravitational waves (GWs) has opened new horizons for physics. Current and upcoming missions, such as LIGO, VIRGO, KAGRA, and LISA, promise to shed light on black holes of every size from stellar mass (SBH) sizes up to supermassive black holes. The intermediate-mass black hole (IMBH) family has not been detected beyond any reasonable doubt. Recent analyses suggest observational evidence for the presence of IMBHs in the centers of two Galactic globular clusters (GCs). In this paper, we investigate the possibility that GCs were born with a central IMBH, which undergoes repeated merger events with SBHs in the cluster core. By means of a semi-analytical method, we follow the evolution of the primordial cluster population in the galactic potential and the mergers of the binary IMBH-SBH systems. Our models predict ≈1000 IMBHs within 1 kpc from the galactic center and show that the IMBH-SBH merger rate density changes from ${ \mathcal R }\approx 1000$ Gpc−3 yr−1 beyond z ≈ 2 to ${ \mathcal R }\approx 1\mbox{--}10$ Gpc−3 yr−1 at z ≈ 0. The rates at low redshifts may be significantly higher if young massive star clusters host IMBHs. The merger rates are dominated by IMBHs with masses between 103 and 104 M⊙. Currently, there are no LIGO/VIRGO upper limits for GW sources in this mass range, but our results show that at design sensitivity, these instruments will detect IMBH-SBH mergers in the coming years. LISA and the Einstein Telescope will be best suited to detect these events. The inspirals of IMBH-SBH systems may also generate an unresolved GW background. |
| spellingShingle | Fragione, G Ginsburg, I Kocsis, B Gravitational waves and intermediate-mass black hole retention in globular clusters |
| title | Gravitational waves and intermediate-mass black hole retention in globular clusters |
| title_full | Gravitational waves and intermediate-mass black hole retention in globular clusters |
| title_fullStr | Gravitational waves and intermediate-mass black hole retention in globular clusters |
| title_full_unstemmed | Gravitational waves and intermediate-mass black hole retention in globular clusters |
| title_short | Gravitational waves and intermediate-mass black hole retention in globular clusters |
| title_sort | gravitational waves and intermediate mass black hole retention in globular clusters |
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