GR-I-RMHD: a versatile numerical algorithm for modeling dissipative flows in high energy astrophysics

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dc.contributor.authorAhmad Hujeirat
dc.date.accessioned2017-05-03T09:37:02Z
dc.date.available2017-05-03T09:37:02Z
dc.date.issued2010-08-02
dc.description.abstract<p>GR-I-RMHD (-General Relativistic Implicit Radiative Magneto Hydro Dynamical) is a parallel numerical solver for highly/weakly compressible Navier-Stokes equations.<br /> In this talk, I will introduce GR-I-RMHD and address its regime of application.</p>en
dc.description.abstract<p>GR-I-RMHD (-General Relativistic Implicit Radiative Magneto Hydro Dynamical) is a parallel numerical solver for highly/weakly compressible Navier-Stokes equations.<br /> In this talk, I will introduce GR-I-RMHD and address its regime of application.</p>ar
dc.identifier.urihttps://hdl.handle.net/20.500.11888/9575
dc.titleGR-I-RMHD: a versatile numerical algorithm for modeling dissipative flows in high energy astrophysicsen
dc.titleGR-I-RMHD: a versatile numerical algorithm for modeling dissipative flows in high energy astrophysicsar
dc.typeOther
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Palestinian Conference on Modern Trends in Mathematics and Physics II