Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularization

A method for improving the accuracy of hydrodynamical codes that use a moving Voronoi mesh is described. Our scheme is based on a new regularization scheme that constrains the mesh to be centroidal to high precision while still allowing the cells to move approximately with the local fluid velocity,...

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Bibliographic Details
Main Authors: Mocz, Philip (Author), Vogelsberger, Mark (Contributor), Pakmor, Rüdiger (Author), Genel, Shy (Author), Springel, Volker (Author), Hernquist, Lars (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Oxford University Press, 2017-04-27T17:46:16Z.
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Online Access:Get fulltext
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100 1 0 |a Mocz, Philip  |e author 
100 1 0 |a Massachusetts Institute of Technology. Department of Physics  |e contributor 
100 1 0 |a Vogelsberger, Mark  |e contributor 
700 1 0 |a Vogelsberger, Mark  |e author 
700 1 0 |a Pakmor, Rüdiger  |e author 
700 1 0 |a Genel, Shy  |e author 
700 1 0 |a Springel, Volker  |e author 
700 1 0 |a Hernquist, Lars  |e author 
245 0 0 |a Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularization 
260 |b Oxford University Press,   |c 2017-04-27T17:46:16Z. 
856 |z Get fulltext  |u http://hdl.handle.net/1721.1/108458 
520 |a A method for improving the accuracy of hydrodynamical codes that use a moving Voronoi mesh is described. Our scheme is based on a new regularization scheme that constrains the mesh to be centroidal to high precision while still allowing the cells to move approximately with the local fluid velocity, thereby retaining the quasi-Lagrangian nature of the approach. Our regularization technique significantly reduces mesh noise that is attributed to changes in mesh topology and deviations from mesh regularity. We demonstrate the advantages of our method on various test problems, and note in particular improvements obtained in handling shear instabilities, mixing, and in angular momentum conservation. Calculations of adiabatic jets in which shear excites Kelvin-Helmholtz instability show reduction of mesh noise and entropy generation. In contrast, simulations of the collapse and formation of an isolated disc galaxy are nearly unaffected, showing that numerical errors due to the choice of regularization do not impact the outcome in this case. 
546 |a en_US 
655 7 |a Article 
773 |t Monthly Notices of the Royal Astronomical Society