2019
DOI: 10.1007/s00033-018-1061-3
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Robust numerical schemes for Two-Fluid Ten-Moment plasma flow equations

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Cited by 6 publications
(5 citation statements)
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“…Expression (25) clearly shows that if f is entropy stable then together with the compact (or periodic) boundary condition the scheme is globally entropy stable.…”
Section: Theorem 31 ([8]mentioning
confidence: 99%
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“…Expression (25) clearly shows that if f is entropy stable then together with the compact (or periodic) boundary condition the scheme is globally entropy stable.…”
Section: Theorem 31 ([8]mentioning
confidence: 99%
“…In several fluid and plasma flow applications assumptions of the local thermodynamic equilibrium do not hold (see [14,29,5,28,19,25]). Due to this, the simulations of such flows using the scalar description of the pressure (used most commonly in Euler equations of compressible fluid flows) is not accurate and instead a tonsorial pressure (and hence temperature) is needed.…”
Section: Introductionmentioning
confidence: 99%
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“…However, RMHD has limitations when modeling several astrophysical systems, like pulsar, gamma-ray burst, etc., see [12] for a detailed discussion. Following the development of non-relativistic two-fluid plasma flow equations [13], [14], [15], [16], [17], [18], [19], several authors have considered an analogous relativistic two-fluid plasma flow equations [20], [21], [22], [23], [24]. Two-fluid relativistic plasma flow equations describe each fluid (ion and electron) in plasma using the equations of special relativistic hydrodynamics (RHD).…”
Section: Introductionmentioning
confidence: 99%