Relativistic fluids and magneto-fluids

By A. M. Anile. 2005

357 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology, Oceanography

View Paper: https://www.semanticscholar.org/paper/cf81206b62fa5024aded89468b06c68f96fb34f9

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Citations in the corpus

The black hole accretion code (2016, neutral): “and we can write the total energy-momentum tensor in terms of the vectors u and b alone [86] as”
A Numerical Method for General Relativistic Magnetohydrodynamics (2002, methodology): “APPENDIX C MHD SHOCKS Relativistic MHD shocks have been discussed by Anile (1989) and K99.”
THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics (2012, methodology): “The analytic solution can be easily found in Lagrangian coordinates, up to the caustic point, using the method of characteristics (Anile 1990), while its calculation in Eulerian coordinates involves the solution of a transcendental equation.”
An efficient shock-capturing central-type scheme for multidimensional relativistic flows. II. Magnetohydrodynamics (2002, methodology): “Our derivation follows that of Anile (1989), also described in KO and BA.”
An HLLC Riemann solver for relativistic flows – II. Magnetohydrodynamics (2006, methodology): “The presence of magnetic fields further entangles the solution, since the number of decaying waves increases from three to seven (Anile & Pennisi 1987; Anile 1989). An exact analytical approach to the solution (which does not allow compound waves) has been recently presented in Giacomazzo & Rezzolla”
Three-Dimensional Simulations of Magnetized Thin Accretion Disks around Black Holes: Stress in the Plunging Region (2008, background): “The fluid 4-velocity and the magnetic field 4-vector (see, e.g., Anile 1989 for definitions) are given byuµ andbµ, and the rest-mass density, internal energy density, thermal pressure, and magnetic pressure as measured in the fluid comoving frame areρ, ug, p = (γ −1)ug with adiabatic indexγ = 4/3,…”
Beyond ideal MHD: towards a more realistic modelling of relativistic astrophysical plasmas (2008, background): “Theoretical work to derive a fully relativistic theory of nonideal hydrodynamics and non-ideal MHD has been carried out by several authors in the past (Israel 1976; Stewart 1977; Carter 1991; Lichnerowicz 1967; Anile 1989) and is particularly simple in the case of the resistive MHD description.”
Time‐dependent, force‐free, degenerate electrodynamics (2002, background): “Here we describe a simple one-dimensional scheme which is very similar to the one constructed by Komissarov ( 1999) for RMHD.”
HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics (2003, background): “The reader may also find it useful to consult Anile (1989).”
PLUTO: A Numerical Code for Computational Astrophysics (2007, background): “Thisapproachdatesbacktothepioneeringworkof Godunov (1959), and it has now become the leading line in developing high-resolution codes examples of which include FLASH (Fryxell et al. 2000 for reactive hydrodynamics), the special relativistic hydro code GENESIS (Aloy et al. 1999), the versatile advect”
An HLLC Riemann solver for relativistic flows ¿ I. Hydrodynamics (2005, background): “Since it can be shown (Taub 1948; Anile 1989; Mignone et al. 2005a) that the specific heat ratio cannot exceed 2, one always has c2s < 1.”
General relativistic magnetohydrodynamic simulations of the jet formation and large-scale propagation from black hole accretion systems (2006, background): “A more complete discussion of the relativistic MHD equations can be found in Anile (1989).”
A Measurement of the Electromagnetic Luminosity of a Kerr Black Hole (2004, background): “(20) A more complete account of the relativistic MHD equations can be found in Gammie et al. (2003a) or Anile (1989).”