GRHydro: a new open-source general-relativistic magnetohydrodynamics code for the Einstein toolkit

被引:100
|
作者
Moesta, Philipp [1 ]
Mundim, Bruno C. [2 ,3 ,4 ]
Faber, Joshua A. [3 ,4 ]
Haas, Roland [1 ,5 ]
Noble, Scott C. [3 ,4 ]
Bode, Tanja [5 ,6 ]
Loeffler, Frank [7 ]
Ott, Christian D. [1 ,7 ]
Reisswig, Christian [1 ]
Schnetter, Erik [7 ,8 ,9 ]
机构
[1] CALTECH, TAPIR, Pasadena, CA 91125 USA
[2] Max Planck Inst Gravitat Phys, D-14476 Golm, Germany
[3] Rochester Inst Technol, Ctr Computat Relat & Gravitat, Rochester, NY 14623 USA
[4] Rochester Inst Technol, Sch Math Sci, Rochester, NY 14623 USA
[5] Georgia Inst Technol, Sch Phys, Ctr Relativist Astrophys, Atlanta, GA 30332 USA
[6] Univ Tubingen, Inst Astron & Astrophys, D-72076 Tubingen, Germany
[7] Louisiana State Univ, Ctr Computat & Technol, Baton Rouge, LA 70803 USA
[8] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
[9] Univ Guelph, Dept Phys, Guelph, ON N1G 2W1, Canada
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会;
关键词
general-relativistic MHD; Einstein toolkit; VARIATION DIMINISHING SCHEME; FLUX-CORRECTED TRANSPORT; NUMERICAL SCHEME; MAGNETIC-FIELDS; BLACK-HOLE; HYDRODYNAMICS; SIMULATIONS; EQUATIONS; MHD; INSTABILITY;
D O I
10.1088/0264-9381/31/1/015005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the new general-relativistic magnetohydrodynamics (GRMHD) capabilities of the Einstein toolkit, an open-source community-driven numerical relativity and computational relativistic astrophysics code. The GRMHD extension of the toolkit builds upon previous releases and implements the evolution of relativistic magnetized fluids in the ideal MHD limit in fully dynamical spacetimes using the same shock-capturing techniques previously applied to hydrodynamical evolution. In order to maintain the divergence-free character of the magnetic field, the code implements both constrained transport and hyperbolic divergence cleaning schemes. We present test results for a number of MHD tests in Minkowski and curved spacetimes. Minkowski tests include aligned and oblique planar shocks, cylindrical explosions, magnetic rotors, Alfven waves and advected loops, as well as a set of tests designed to study the response of the divergence cleaning scheme to numerically generated monopoles. We study the code's performance in curved spacetimes with spherical accretion onto a black hole on a fixed background spacetime and in fully dynamical spacetimes by evolutions of a magnetized polytropic neutron star and of the collapse of a magnetized stellar core. Our results agree well with exact solutions where these are available and we demonstrate convergence. All code and input files used to generate the results are available on http://einsteintoolkit.org. This makes our work fully reproducible and provides new users with an introduction to applications of the code.
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页数:50
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