Hydrodynamical transport of angular momentum in accretion disks in the presence of nonlinear perturbations due to noise
Subham Ghosh, Banibrata Mukhopadhyay

TL;DR
This paper investigates how stochastic forces, such as noise from thermal fluctuations or outflows, can induce turbulence in linearly stable Keplerian accretion disks by amplifying nonlinear perturbations.
Contribution
It demonstrates that external stochastic forcing can destabilize otherwise stable accretion disk flows, leading to turbulence through nonlinear perturbation growth, a novel insight into disk instability mechanisms.
Findings
Forcing causes linear stable modes to grow to large amplitudes.
Nonlinear perturbations diverge faster with external force, promoting rapid turbulence.
Emergence of nonlinearity depends only on force, not initial perturbation amplitude.
Abstract
The origin of hydrodynamical instability and turbulence in the Keplerian accretion disk is a long-standing puzzle. The flow therein is linearly stable. Here we explore the evolution of perturbation in this flow in the presence of an additional force. Such a force, which is expected to be stochastic in nature hence behaving as noise, could result from thermal fluctuations (however small be), grain-fluid interactions, feedback from outflows in astrophysical disks, etc. We essentially establish the evolution of nonlinear perturbation in the presence of Coriolis and external forces, which is the modified Landau equation. We obtain that even in the linear regime, under suitable forcing and Reynolds number, the otherwise least stable perturbation evolves to a very large saturated amplitude, leading to nonlinearity and plausible turbulence. Hence, forcing essentially leads a linear stable mode…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Phase Equilibria and Thermodynamics · Advanced Combustion Engine Technologies
