Impetus: consistent SPH calculations of 3D spherical Bondi accretion on to a black hole. Issue 4 (6th April 2018)

• Record Type: Journal Article
• Authors: Ramírez-Velasquez, J M; Sigalotti, L Di G; Gabbasov, R; Cruz, F; Klapp, J
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 477:Issue 4(2018)
• Page Start: 4308
• Page End: 4329
• Publication Date: 2018-04-06
• Subjects: accretion, accretion discs -- hydrodynamics -- methods: numerical -- galaxies: active -- galaxies nuclei -- supermassive black hole; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty876
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: We present three-dimensional calculations of spherically symmetric Bondi accretion on to a stationary supermassive black hole of mass 10 8 M⊙ within a radial range of 0.02–10 pc, using a modified version of the smoothed particle hydrodynamics gadget-2 code, which ensures approximate first-order consistency (i.e. second-order accuracy) for the particle approximation. First-order consistency is restored by allowing the number of neighbours, n neigh, and the smoothing length, h, to vary with the total number of particles, N, such that the asymptotic limits n neigh → ∞ and h → 0 hold as N → ∞. The ability of the method to reproduce the isothermal (γ = 1) and adiabatic (γ = 5/3) Bondi accretion is investigated with increased spatial resolution. In particular, for the isothermal models, the numerical radial profiles closely match the Bondi solution, except near the accretor, where the density and radial velocity are slightly underestimated. However, as n neigh is increased and h is decreased, the calculations approach first-order consistency and the deviations from the Bondi solution decrease. The density and radial velocity profiles for the adiabatic models are qualitatively similar to those for the isothermal Bondi accretion. Steady-state Bondi accretion is reproduced by the highly resolved consistent models with a percent relative error of ≲ 1 per cent for γ = 1 and ∼9 per cent for γ = 5/3, with the adiabatic accretion taking longer than the isothermal case to reach steady flow. The performance of the method is assessed by comparing the results with those obtained using the standard gadget-2 and gizmo codes.