Analytic solution to the dynamical friction acting on circularly moving perturbers
arXiv:2111.07366 · doi:10.3847/1538-4357/ac5519
Abstract
We present an analytic approach to the dynamical friction (DF) acting on a circularly moving point mass perturber in a gaseous medium. We demonstrate that, when the perturber is turned on at , steady-state (infinite time perturbation) is achieved after exactly one sound-crossing time. At low Mach number , the circular-motion steady-state DF converges to the linear-motion, finite time perturbation expression. The analytic results describe both the radial and tangential forces on the perturbers caused by the backreaction of the wake propagating in the medium. The radial force is directed inward, toward the motion centre, and is dominant at large Mach numbers. For subsonic motion, this component is negligible. For moderate and low Mach numbers, the tangential force is stronger and opposes the motion of the perturber. The analytic solution to the circular-orbit DF suffers from a logarithmic divergence in the supersonic regime. This divergence appears at short distances from the perturber solely (unlike the linear motion result which is also divergent at large distances) and can be encoded in a maximum multipole. This is helpful to assess the resolution dependence of numerical simulations implementing DF at the level of Liénard-Wiechert potentials. We also show how our approach can be generalised to calculate the DF acting on a compact circular binary.
(v1) 6 pages, 4 figures, comments welcome (v2) extended version with revised discussion of the divergence, accepted for publication in ApJ. Code computing the circular DF available at https://github.com/nyalothep/dynfricGas
References in corpus (7)
- Ultralight scalars as cosmological dark matter
- Dynamical Friction of a Circular-Orbit Perturber in a Gaseous Medium
- The response of ultralight dark matter to supermassive black holes and binaries
- Relativistic dynamical friction in a collisional fluid
- Dynamical Friction of Double Perturbers in a Gaseous Medium
- A Self-Consistent, Time-Dependent Treatment of Dynamical Friction: New Insights regarding Core Stalling and Dynamical Buoyancy
- Resonant and non-resonant relaxation of globular clusters