Volume 464, Number 2, March III 2007
|Page(s)||447 - 450|
|Published online||19 December 2006|
Adaptive smoothing lengths in SPH
School of Physics & Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, Wales, UK e-mail: [Rhianne.Attwood; Anthony.Whitworth]@astro.cf.ac.uk
2 Department of Physics & Astronomy, University of Sheffield, Hicks Building, Housfield Road, Sheffield S3 7RH, UK e-mail: S.Goodwin@Sheffield.ac.uk
Accepted: 18 December 2006
Context.There is a need to improve the fidelity of SPH simulations of self-gravitating gas dynamics.
Aims.We remind users of SPH that, if smoothing lengths are adjusted so as to keep the number of neighbours, , in the range , the tolerance, , should be set to zero, as first noted by Nelson & Papaloizou. We point out that this is a very straightforward and computationally inexpensive constraint to implement.
Methods.We demonstrate this by simulating acoustic oscillations of a self-gravitating isentropic monatomic gas-sphere (cf. Lucy), using particles and .
Results.We show that there is a marked reduction in the rates of numerical dissipation and diffusion as is reduced from 10 to zero. Moreover this reduction incurs a very small computational overhead.
Conclusions.We propose that this should become a standard test for codes used in simulating star formation. It is a highly relevant test, because pressure waves generated by the switch from approximate isothermality to approximate adiabaticity play a critical role in the fragmentation of collapsing prestellar cores. Since many SPH simulations in the literature use and , their results must be viewed with caution.
Key words: hydrodynamics / methods: numerical / stars: oscillations
© ESO, 2007
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