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dc.contributor.authorCook, Todd A.en
dc.contributor.authorKim, Hong-Ryulen
dc.contributor.authorLouca, Loucas S.en
dc.creatorCook, Todd A.en
dc.creatorKim, Hong-Ryulen
dc.creatorLouca, Loucas S.en
dc.date.accessioned2019-05-06T12:23:30Z
dc.date.available2019-05-06T12:23:30Z
dc.date.issued1995
dc.identifier.isbn0-8194-1971-0
dc.identifier.isbn978-0-8194-1971-2
dc.identifier.urihttp://gnosis.library.ucy.ac.cy/handle/7/48300
dc.description.abstractN-body methods are used to simulate the evolution and interaction of galaxies. These simulations are usually run on large-scale supercomputers or on very expensive full-custom hardare. This paper presents an alternative hardware method for acceleration of N-body simulations. The method yields a significant fraction of the performance of custom hardware and provides a great deal more flexibility. A protoype implementation is presented.en
dc.language.isoengen
dc.publisherAffiliation: Rutgers Univ., Piscataway, NJ, USA, United Statesen
dc.publisherCorrespondence Address: Cook, Todd A.en
dc.publisherRutgers Univ., Piscataway, NJ, USAUnited Statesen
dc.sourceProceedings of SPIE - The International Society for Optical Engineeringen
dc.subjectSimulationen
dc.subjectPerformanceen
dc.subjectComputer hardwareen
dc.subjectAstronomyen
dc.subjectGalactic dynamicsen
dc.subjectHardware accelerationen
dc.subjectSupercomputersen
dc.titleHardware acceleration of n-body simulations for galactic dynamicsen
dc.typeinfo:eu-repo/semantics/conferenceObject
dc.description.volume2607
dc.description.startingpage115
dc.description.endingpage126
dc.author.facultyΠολυτεχνική Σχολή / Faculty of Engineering
dc.author.departmentΤμήμα Μηχανικών Μηχανολογίας και Κατασκευαστικής / Department of Mechanical and Manufacturing Engineering
dc.type.uhtypeConference Objecten
dc.contributor.orcidLouca, Loucas S. [0000-0002-0850-2369]
dc.description.totalnumpages115-126
dc.gnosis.orcid0000-0002-0850-2369


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