How empty is an empty loss cone?
arXiv:1705.02603 · doi:10.1093/mnras/stx485
Abstract
We consider two body relaxation in a spherical system with a loss cone. Considering two-dimensional angular momentum space, we focus on "empty loss cone" systems, where the typical scattering during a dynamical time is smaller than the size of the loss cone . As a result, the occupation number within the loss cone is significantly smaller than outside. Classical diffusive treatment of this regime predict exponentially small occupation number deep in the loss cone. We revisit this classical derivation of occupancy distribution of objects in the empty loss cone regime. We emphasize the role of the rare large scatterings and show that the occupancy does not decay exponentially within the loss cone, but it is rather flat, with a typical value compared to the occupation in circular angular momentum (where is the smallest possible scattering). Implication are that although the loss cone for tidal break of Giants or binaries is typically empty, tidal events which occurs significantly inside the loss cone (), are almost as common as those with where is the ratio between the tidal radius and the periastron. The probability for event with penetration factor decreases only as rather than exponentially. This effect has no influence on events characterized by full loss cone, such as tidal disruption event of main sequence star.
arXiv comment12 pages, 3 figures
References in corpus (6)
- The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
- Observational constraints on growth of massive black holes
- Rates of tidal disruption of stars by massive central black holes
- Ejection of hypervelocity stars by the (binary) black hole(s) in the Galactic center
- Long Term Evolution of Massive Black Hole Binaries
- Stellar Energy Relaxation around A Massive Black Hole
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- Tidal Disruptions of Main Sequence Stars -- I. Observable Quantities and their Dependence on Stellar and Black Hole Mass
- Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS): Library of Fallback Rates
- Steeper stellar cusps in galactic centers from binary disruption
- Radio Emission from the unbound Debris of Tidal Disruption Events
- Scalar Resonant Relaxation of Stars Around a Massive Black Hole
- Tidal disruptions of main sequence stars -- IV. Relativistic effects and dependence on black hole mass
- Vector Resonant Relaxation of Stars around a Massive Black Hole
- Tidal Disruptions of Main Sequence Stars -- V. The Varieties of Disruptions
- Black Hole Mergers Induced by Tidal Encounters with a Galactic Centre Black Hole
- Shock Breakouts from Tidal Disruption Events
- Demographics of Tidal Disruption Events with L-Galaxies: I. Volumetric TDE rates and the abundance of Nuclear Star Clusters
- The Effect of Impact Parameter on Tidal Disruption Events
- The former companion of the hyper-velocity star S5-HVS1