Solution of the 1D Special Relativistic Hydrodynamics(SRH) Equations Using Different Numerical Method and Results from Different Test Problems

Simple item page
dc.creatorDonmez, Orhan
dc.date2005-12-19
dc.date.accessioned2026-07-07T06:53:57Z
dc.date.available2026-07-07T06:53:57Z
dc.descriptionIn this paper, we have solved 1D special relativistic hydrodynamical equations using different numerical method in computational gas dynamics. The 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.
dc.description8 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0512104
dc.identifierhttp://arxiv.org/abs/gr-qc/0512104
dc.identifierAppl.Math.Comput. 181 (2006) 256-270
dc.identifierdoi:10.1016/j.amc.2006.01.031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/105775
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectComputational Physics
dc.titleSolution of the 1D Special Relativistic Hydrodynamics(SRH) Equations Using Different Numerical Method and Results from Different Test Problems
dc.typetext

Files

Collections

arXiv