TL;DR
VADER is a versatile, open-source numerical code designed to simulate viscous thin accretion disks with high accuracy and efficiency, accommodating various physical and boundary conditions for astrophysical research.
Contribution
The paper introduces VADER, a flexible, general numerical framework for simulating viscous thin accretion disks with improved speed and adaptability over existing specialized tools.
Findings
Implemented a second-order accurate, implicit finite-volume scheme.
Achieved ~5x speedup using Anderson acceleration.
Demonstrated flexibility with arbitrary disk parameters.
Abstract
The evolution of thin axisymmetric viscous accretion disks is a classic problem in astrophysics. While models based on this simplified geometry provide only approximations to the true processes of instability-driven mass and angular momentum transport, their simplicity makes them invaluable tools for both semi-analytic modeling and simulations of long-term evolution where two- or three-dimensional calculations are too computationally costly. Despite the utility of these models, the only publicly-available frameworks for simulating them are rather specialized and non-general. Here we describe a highly flexible, general numerical method for simulating viscous thin disks with arbitrary rotation curves, viscosities, boundary conditions, grid spacings, equations of state, and rates of gain or loss of mass (e.g., through winds) and energy (e.g., through radiation). Our method is based on a…
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