Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6571
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dc.contributor.authorallHérault, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallBilotta, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallDaltrymple, R. A.; Johns Hopkins University, Baltimoreen
dc.date.accessioned2011-01-12T12:59:53Zen
dc.date.available2011-01-12T12:59:53Zen
dc.date.issued2010en
dc.identifier.urihttp://hdl.handle.net/2122/6571en
dc.description.abstractA Smoothed Particle Hydrodynamics (SPH) method for free surface flows has been implemented on a graphical processing unit (GPU) using the Compute Unified Device Architecture (CUDA) developed by Nvidia, resulting in tremendous speed-ups. The entire SPH code, with its three main components: neighbor list construction, force computation, and integration of the equation of motion, is computed on the GPU, fully exploiting its computational power. The simulation speed achieved is one to two orders of magnitude faster than the equivalent CPU code. Example applications are shown for paddle-generated waves in a basin and a dam-break wave impact on a structure. GPU implementation of SPH permits high resolution SPH modeling in hours and days rather than weeks and months on inexpensive and readily available hardware.en
dc.language.isoEnglishen
dc.relation.ispartofJournal of Hydraulic Researchen
dc.relation.ispartofseries/48 (2010)en
dc.subjectCUDA, fluid simulation, GPGPU, GPU, particle methods, smoothed particle hydrodynamicsen
dc.titleSPH on GPU with CUDAen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber74-79en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.08. Volcanic risken
dc.identifier.doi10.3826/jhr.2010.0005en
dc.description.obiettivoSpecifico2.1. TTC - Laboratorio per le reti informatiche, GRID e calcolo avanzatoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorHérault, A.en
dc.contributor.authorBilotta, G.en
dc.contributor.authorDaltrymple, R. A.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentJohns Hopkins University, Baltimoreen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.orcid0000-0002-1406-4545-
crisitem.author.orcid0000-0002-7915-6256-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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