{"title":"Adaptive particle refinement for compressible smoothed particle hydrodynamics","authors":"Rebecca Nealon, Daniel Price","doi":"arxiv-2409.11470","DOIUrl":null,"url":null,"abstract":"We introduce adaptive particle refinement for compressible smoothed particle\nhydrodynamics (SPH). SPH calculations have the natural advantage that\nresolution follows mass, but this is not always optimal. Our implementation\nallows the user to specify local regions of the simulation that can be more\nhighly resolved. We test our implementation on practical applications including\na circumbinary disc, a planet embedded in a disc and a flyby. By comparing with\nequivalent globally high resolution calculations we show that our method is\naccurate and fast, with errors in the mass accreted onto sinks of less than 9\npercent and speed ups of 1.07-6.62 times for the examples shown. Our method is\nadaptable and easily extendable, for example with multiple refinement regions\nor derefinement.","PeriodicalId":501163,"journal":{"name":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","volume":"85 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11470","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We introduce adaptive particle refinement for compressible smoothed particle
hydrodynamics (SPH). SPH calculations have the natural advantage that
resolution follows mass, but this is not always optimal. Our implementation
allows the user to specify local regions of the simulation that can be more
highly resolved. We test our implementation on practical applications including
a circumbinary disc, a planet embedded in a disc and a flyby. By comparing with
equivalent globally high resolution calculations we show that our method is
accurate and fast, with errors in the mass accreted onto sinks of less than 9
percent and speed ups of 1.07-6.62 times for the examples shown. Our method is
adaptable and easily extendable, for example with multiple refinement regions
or derefinement.