Minimising the numerical viscosity in Smoothed Particle Hydrodynamics simulations of discs
Cheng Chen, C. J. Nixon

TL;DR
This paper investigates how to minimize numerical viscosity in SPH simulations of accretion discs by optimizing the viscosity coefficients, proposing a time-dependent quadratic term to reduce dissipation while capturing shocks effectively.
Contribution
It identifies optimal values for SPH viscosity coefficients to reduce numerical viscosity and suggests a time-dependent quadratic coefficient approach for better shock modeling.
Findings
Default SPH viscosity parameters can be too high for discs.
Higher quadratic coefficients are needed for strong shocks.
A time-dependent quadratic coefficient improves simulation accuracy.
Abstract
Simulations using the Smoothed Particle Hydrodynamics (SPH) technique typically include numerical viscosity to model shocks and maintain particle order on the kernel scale. This numerical viscosity is composed of linear and quadratic terms, with coefficients and respectively. Setting these coefficients too high results in excessive numerical dissipation, whereas setting them too low may lead to unwanted effects such as particle penetration, which also leads to excess dissipation. In this study, we simulate accretion discs using the SPH code {\sc phantom} to investigate the effective disc viscosity arising from numerical viscosity. We model steady-state coplanar and circular discs with different values of and , from which we determine the coefficients that lead to minimum levels of numerical viscosity by maximising…
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