A new general relativistic magnetohydrodynamics code for dynamical spacetimes

Astronomy and Astrophysics

Volumn 492, Issue 3, 2008, Pages 937-953

  Cerda Duran P ^a   Font, J A ^b   Anton L ^b   Muller E ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF VALENCIA   (Spain)

Author keywords

Gravitation; Hydrodynamics; Magnetohydrodynamics (MHD); Methods: numerical; Relativity; Stars: supernovae: general

Indexed keywords

ASTROPHYSICS; EQUATIONS OF STATE; FLUID DYNAMICS; GRAVITATION; GRAVITATIONAL EFFECTS; HYDRODYNAMICS; MAGNETIC FIELD EFFECTS; MAGNETIC FIELDS; MAGNETIC MATERIALS; MAGNETOHYDRODYNAMICS; MAGNETOS; NEUTRONS; NUMERICAL METHODS; POLYNOMIAL APPROXIMATION; RELATIVITY; SHOCK WAVES;

ANALYTICAL EXPRESSIONS; ASTROPHYSICAL APPLICATIONS; COLLAPSE SIMULATIONS; DYNAMICAL SPACETIME; EINSTEIN EQUATIONS; EQUILIBRIUM CONFIGURATIONS; FIELD APPROXIMATIONS; FIRST ORDERS; GRAVITATIONAL FIELDS; HIGH MAGNETIC FIELDS; HIGH RESOLUTIONS; HYPERBOLIC FORMS; ISOLATED NEUTRON STARS; MAGNETIZED NEUTRON STARS; METHODS: NUMERICAL; NEUTRON STARS; NUMERICAL CODES; RELATIVISTIC MAGNETOHYDRODYNAMICS; SPACE TIMES; SPHERICAL SYMMETRIES; STARS: SUPERNOVAE: GENERAL; STELLAR CORES; STRINGENT TESTS; TRANSPORT METHODS;

STARS;

EID: 57649245565     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810086     Document Type: Article

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