The Influences of Outflow on the Dynamics of Inflow

TL;DR

This paper investigates how outflows affect inflow dynamics in accretion flows, extending previous models by considering detailed interactions between outflow and inflow based on numerical simulations.

Contribution

It provides a more detailed analysis of outflow influence by including mass, momentum, and energy exchange in a 1.5D accretion flow model, beyond simple radius-dependent accretion rates.

Findings

Outflow significantly impacts inflow dynamics.

Radius-dependent accretion rate captures main outflow effects.

Model aligns with numerical simulation properties.

Abstract

Both numerical simulations and observations indicate that in an advection-dominated accretion flow most of the accretion material supplied at the outer boundary will not reach the inner boundary. Rather, they are lost via outflow. Previously, the influence of outflow on the dynamics of inflow is taken into account only by adopting a radius-dependent mass accretion rate $\dot{M}=\dot{M}_0 (r/r_{\rm out})^s$ with $s>0$. In this paper, based on a 1.5 dimensional description to the accretion flow, we investigate this problem in more detail by considering the interchange of mass, radial and azimuthal momentum, and the energy between the outflow and inflow. The physical quantities of the outflow is parameterized based on our current understandings to the properties of outflow mainly from numerical simulations of accretion flows. Our results indicate that under reasonable assumptions to the properties of outflow, the main influence of outflow has been properly included by adopting $\dot{M}=\dot{M}_0 (r/r_{\rm out})^s$.