The Role of Outflows in dynamic of Advection Dominated Accretion Flows: a Self-Similar Solution
Fahimeh Habibi

TL;DR
This paper presents a self-similar analytical model of advection-dominated accretion flows incorporating outflows, revealing how outflow parameters influence disc dynamics, temperature, and mass inflow rates.
Contribution
It introduces a self-similar solution framework for viscous accretion discs with outflows, linking outflow parameters to flow properties and the power-law index of mass inflow.
Findings
Outflow enhances the power index s of mass inflow rate.
Increased outflow parameter raises disc temperature and thickness.
Energy extraction by outflow decreases the power index s.
Abstract
The effects of outflow on the behavior of a viscous gaseous disc around a compact object in an advection-dominated state are examined in this paper. We suppose that the flow is steady, axisymmetric, and rotating. Also, we focus on the model in which the mass, the angular momentum, and the energy can be transported outward by outflow. Similar to the pioneering studies, we consider a power-law function for mass inflow rate as . We assume that the power index is proportional to the dimensionless thickness of disc. To analyze such a system, the hydrodynamic equations have extracted in cylindrical coordinates . Then, the flow equations were vertically integrated, and a set of self-similar solutions was got in the radial direction. Our solutions include three essential parameters: , and . The influence of the outflow on the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsFluid Dynamics and Turbulent Flows
