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dc.contributor.authorLorén-Aguilar, P
dc.contributor.authorBate, Matthew R.
dc.date.accessioned2016-02-01T11:00:23Z
dc.date.issued2015-10-28
dc.description.abstractWe present an improved version of the Lorén-Aguilar & Bate method to integrate the twofluid dust/gas equations that correctly captures the limiting velocity of small grains in the presence of net differences (excluding the drag force) between the accelerations of the dust and the gas. A series of accelerated DUSTYBOX tests and a simulation of dust-settling in a protoplanetary disc are performed comparing the performance of the new and old methods. The modified method can accurately capture the correct limiting velocity while preserving all the conservation properties of the original method.en_GB
dc.description.sponsorshipSTFCen_GB
dc.description.sponsorshipEuropean Research Council under the European Community’s Seventh Framework Programmeen_GB
dc.description.sponsorshipBIS National E-Infrastructure capital granten_GB
dc.description.sponsorshipSTFC DiRAC Operations granten_GB
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2015, Vol. 454, Issue 4, pp. 4114 - 4119en_GB
dc.identifier.doi10.1093/mnras/stv2262
dc.identifier.grantnumberST/J001627/1en_GB
dc.identifier.grantnumberFP7/2007-2013 grant agreement no. 339248en_GB
dc.identifier.grantnumberST/K000373/1en_GB
dc.identifier.grantnumberST/K0003259/1en_GB
dc.identifier.urihttp://hdl.handle.net/10871/19454
dc.language.isoenen_GB
dc.publisherOxford University Pressen_GB
dc.relation.urlhttp://hdl.handle.net/10871/18407en_GB
dc.rights© 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.en_GB
dc.titleTwo-fluid dust and gas mixtures in smoothed particle hydrodynamics II: An improved semi-implicit approach (article)en_GB
dc.typeArticleen_GB
dc.date.available2016-02-01T11:00:23Z
dc.identifier.issn0035-8711
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.en_GB
dc.descriptionThe dataset associated with this article is available in ORE at: http://hdl.handle.net/10871/18407en_GB
dc.identifier.journalMonthly Notices of the Royal Astronomical Societyen_GB


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