Solving 1-D special relativistic hydrodynamics (SRH) equations using different numerical methods and results from different test problems

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dc.contributor.authorDonmez, Orhan
dc.date.accessioned2019-08-01T13:38:39Z
dc.date.available2019-08-01T13:38:39Z
dc.date.issued2006
dc.departmentNiğde ÖHÜ
dc.description.abstractIn this paper, we have solved I-D special relativistic hydrodynamical equations using different numerical methods in computational gas dynamics. Numerical solutions of these equations for smooth wave cases give better solution when we use Non-TVD (total variable diminishing) but solution of discontinuity wave produces some oscillation behind the shock. On the other hand, TVD type schemes give good approximation at discontinuity cases. Because TVD schemes completely remove the oscillations, they reduce locally the accuracy of the solution around the extrema. (c) 2006 Elsevier Inc. All rights reserved.
dc.identifier.doi10.1016/j.amc.2006.01.031
dc.identifier.endpage270
dc.identifier.issn0096-3003
dc.identifier.issue1
dc.identifier.scopus2-s2.0-33749534137
dc.identifier.scopusqualityQ1
dc.identifier.startpage256
dc.identifier.urihttps://dx.doi.org/10.1016/j.amc.2006.01.031
dc.identifier.urihttps://hdl.handle.net/11480/5475
dc.identifier.volume181
dc.identifier.wosWOS:000242276600025
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.institutionauthorDonmez, Orhan
dc.language.isoen
dc.publisherELSEVIER SCIENCE INC
dc.relation.ispartofAPPLIED MATHEMATICS AND COMPUTATION
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjecthydrodynamics
dc.subjectnumerical relativity
dc.subjectshock waves
dc.subjectnumerical method
dc.subjectfluid dynamics
dc.titleSolving 1-D special relativistic hydrodynamics (SRH) equations using different numerical methods and results from different test problems
dc.typeArticle

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