Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-10-25
Mon.Not.Roy.Astron.Soc. 358 (2005) 1361-1378
Astronomy and Astrophysics
Astrophysics
This version has been published in MNRAS
Scientific paper
10.1111/j.1365-2966.2005.08843.x
We consider the problem of tidal disruption of stars in the centre of a galaxy containing a supermassive binary black hole with unequal masses. We assume that over the separation distance between the black holes the gravitational potential is dominated by the more massive black hole. Also, we assume that the number density of stars is concentric with the primary black hole and has a power law cusp.We show that the bulk of stars with a small angular-momentum component normal to the black hole binary orbit can reach a small value of total angular momentum through secular evolution in the gravitational field of the binary, and hence they can be tidally disrupted. This effect is analogous to the so-called Kozai effect (Kozai, 1962, Lidov, 1961,1962) well known in celestial mechanics. We develop an analytical theory of secular evolution of the stellar orbits and calculate the rate of tidal disruption. We confront our analytical theory with a simple numerical model and find very good agreement. Our results show that for primary black-hole mass \sim 10^{6}-10^{7}M_{\odot}, the black- hole mass ratio q > 10^{-2}, cusp size \sim 1pc, the tidal disruption rate can be as large as \sim 10^{-2}-1M_{\odot}/yr. This is at least 10^{2}-10^{4} times larger than estimated for the case of a single supermassive black hole. The duration of the phase of enhanced tidal disruption is determined by the dynamical friction time scale, and it is rather short: \sim 10^{5}yr. The dependence of the tidal disruption rate on the mass ratio, as well as on the size of the cusp, is also discussed.
Ivanov Pavel B.
Polnarev Alexander G.
Saha Prasenjit
No associations
LandOfFree
The tidal disruption rate in dense galactic cusps containing a supermassive binary black hole does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The tidal disruption rate in dense galactic cusps containing a supermassive binary black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The tidal disruption rate in dense galactic cusps containing a supermassive binary black hole will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-477120