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Galaxy rotation and supermassive black hole binary evolution
Mirza, M. A.1; Tahir, A.1; Khan, F. M.1; Holley-Bockelmann, H.2,3; Baig, A. M.1; Berczik, P.4,5,6,7; Chishtie, F.8
2017-08-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume470Issue:1Pages:940-947
AbstractSupermassive black hole (SMBH) binaries residing at the core of merging galaxies are recently found to be strongly affected by the rotation of their host galaxies. The highly eccentric orbits that form when the host is counterrotating emit strong bursts of gravitational waves that propel rapid SMBH binary coalescence. Most prior work, however, focused on planar orbits and a uniform rotation profile, an unlikely interaction configuration. However, the coupling between rotation and SMBH binary evolution appears to be such a strong dynamical process that it warrants further investigation. This study uses direct N-body simulations to isolate the effect of galaxy rotation in more realistic interactions. In particular, we systematically vary the SMBH orbital plane with respect to the galaxy rotation axis, the radial extent of the rotating component, and the initial eccentricity of the SMBH binary orbit. We find that the initial orbital plane orientation and eccentricity alone can change the inspiral time by an order of magnitude. Because SMBH binary inspiral and merger is such a loud gravitational wave source, these studies are critical for the future gravitational wave detector, Laser Interferometer Space Antenna, an ESA/NASA mission currently set to launch by 2034.
SubtypeArticle
KeywordBlack Hole Physics Gravitational Waves Methods: Numerical Galaxies: Kinematics And Dynamics Galaxies: Nuclei
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationHigher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Higher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Volkswagen Foundation(90411) ; Volkswagen Foundation(90411) ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project ; Higher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Higher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Volkswagen Foundation(90411) ; Volkswagen Foundation(90411) ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project
DOI10.1093/mnras/stx1248
WOS KeywordACTIVE GALACTIC NUCLEI ; FINAL-PARSEC PROBLEM ; LONG-TERM EVOLUTION ; DYNAMICAL FRICTION ; STELLAR-SYSTEMS ; DISK GALAXIES ; N-BODY ; COALESCENCE ; MERGERS ; ECCENTRICITY
Indexed BySCI
Language英语
Funding OrganizationHigher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Higher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Volkswagen Foundation(90411) ; Volkswagen Foundation(90411) ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project ; Higher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Higher Education Commission of Pakistan through National Research Program for Universities (NRPU) project(4159) ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; Chinese Academy of Sciences through the Silk Road Project at National Astronomy Observatory of China, through the 'Qianren' special foreign experts program ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; President's International Fellowship for Visiting Scientists programme of Chinese Academy of Sciences ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Strategic Priority Research Programme (Pilot B) 'Multiwavelength gravitational wave universe' of the Chinese Academy of Sciences(XDB23040100) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Deutsche Forschungsgemeinschaft (DFG) through Collaborative Research Center at the Ruprecht-Karls-Universitat Heidelberg(SFB 881) ; Volkswagen Foundation(90411) ; Volkswagen Foundation(90411) ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project ; National Academy of Sciences of Ukraine under the Main Astronomical Observatory GRID/GPU computing cluster project
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000406842600057
Citation statistics
Cited Times:6[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20062
Collection星系宇宙学研究部
Affiliation1.Inst Space Technol, Dept Space Sci, Islamabad 44000, Pakistan
2.Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37240 USA
3.Fisk Univ, Dept Phys, Nashville, TN 37208 USA
4.Jilin Univ, Int Ctr Future Sci, 2699 Qianjin St, Changchun 130012, Jilin, Peoples R China
5.Chinese Acad Sci, Natl Astron Observ China, 20A Datun Rd, Beijing 100012, Peoples R China
6.Chinese Acad Sci, Key Lab Computat Astrophys, 20A Datun Rd, Beijing 100012, Peoples R China
7.Natl Acad Sci Ukraine, Main Astron Observ, 27 Akad Zabolotnoho St, UA-03680 Kiev, Ukraine
8.Pakistan Acad Sci, Theoret Res Inst, Islamabad 44000, Pakistan
Recommended Citation
GB/T 7714
Mirza, M. A.,Tahir, A.,Khan, F. M.,et al. Galaxy rotation and supermassive black hole binary evolution[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,470(1):940-947.
APA Mirza, M. A..,Tahir, A..,Khan, F. M..,Holley-Bockelmann, H..,Baig, A. M..,...&Chishtie, F..(2017).Galaxy rotation and supermassive black hole binary evolution.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,470(1),940-947.
MLA Mirza, M. A.,et al."Galaxy rotation and supermassive black hole binary evolution".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 470.1(2017):940-947.
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