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Relativistic loss cone dynamics: Infall and inspiral rates and branching ratios

Published online by Cambridge University Press:  23 June 2017

Tal Alexander
Tal Alexander*
Affiliation:
Department of Particle Physics & Astrophysics, Weizmann Institute of Science, 234 Herzl St, Rehovot 76100, Israel email: tal.alexander@weizmann.ac.il
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Abstract

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I describe recent advances in the formulation and modeling of relativistic stellar dynamics around a massive black hole, and the implications for the rates of infall (e.g. tidal disruption) and inspiral (e.g. gradual decay by gravitational wave emission) processes, and their branching ratios.

Keywords

stellar dynamicsblack hole physicsGalaxy: centergalaxies: activegravitational waves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 99 - 106
Copyright
Copyright © International Astronomical Union 2017 

References

Alexander, T. 2010 in: Amaro-Seoane, P. & Porter, E. (eds.), GW and EM signatures of MBH binaries and EMRIs, online proc. http://www.aei.mpg.de/~pau/conf_vid4/Alexander.pdf Google Scholar
Alexander, T. 2017, ARAA in press.Google Scholar
Alexander, T. & Livio, M. 2001, ApJ (Letters) 560, L143 CrossRefGoogle Scholar
Alexander, T. & Morris, M. 2003, ApJ (Letters) 590, L25 CrossRefGoogle Scholar
Alexander, T. & Hopman, C. 2003, ApJ (Letters) 590, L29 Google Scholar
Amaro Seoane, P., et al. 2007, CQG, 24, 113 CrossRefGoogle Scholar
Arcavi, I., et al. 2014, ApJ, 793, 38 Google Scholar
Bar-Or, B. & Alexander, T. 2014, ApJ, 820, 129 Google Scholar
Bar-Or, B. & Alexander, T. 2016, CQG, 31, 244003 Google Scholar
Davies, M. & King, A. 2005, ApJ (Letters) 624, L25 Google Scholar
Frank, J. & Rees, M. J. 1976, MNRAS, 176, 633 Google Scholar
Gillessen, S., et al. 2009, ApJ, 692, 362 Google Scholar
Hills, J. G. 1988, Nature, 331, 687 Google Scholar
Hopman, C. & Alexander, T. 2006, ApJ, 645, 1152 CrossRefGoogle Scholar
Ivanov, P. B., Polnarev, A. G. & Saha, P. 2005 MNRAS, 358, 1361 Google Scholar
Komossa, S. & Merritt, D. 2008 ApJ (Letters) 683, L21 Google Scholar
Levin, Y. 2007 MNRAS, 374, 515 Google Scholar
Lightman, A. P. & Shapiro, S. L. 1977, ApJ, 211, 244 Google Scholar
Magorrian, J., et al. 1998 AJ, 115, 2285 CrossRefGoogle Scholar
Merritt, D., Alexander, T., Mikkola, S., & Will, C. 2011, PRD, 84, 044024 Google Scholar
Ostriker, J. P. 1983, ApJ, 273, 99 Google Scholar
Perets, H. B., et al. 2009, ApJ, 702, 884 Google Scholar
Rauch, K. P. & Tremaine, S. 1996, New Astron., 1, 149 CrossRefGoogle Scholar
Sabsovich, D., Alexander, T. & Bar-Or, B. 2017 in prep. Google Scholar
Stone, N. C. & Metzger, B. D. 2016 MNRAS, 455, 859 Google Scholar
Syer, D. & Ulmer, A. 1999, MNRAS, 306, 35 Google Scholar
Vasiliev, E. & Merritt, D. 2013, ApJ, 774, 87 Google Scholar
Will, C. M. 2008, ApJ (Letters) 674, L25 Google Scholar