Semi-global simulations of the magneto-rotational instability in core collapse supernovae

Astronomy and Astrophysics

Volumn 498, Issue 1, 2009, Pages 241-271

  Obergaulinger, M ^a   Cerda Duran P ^a   Muller E ^a   Aloy, M A ^b  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF VALENCIA   (Spain)

Author keywords

Instabilities; Magnetohydrodynamics (MHD); Stars: magnetic fields; stars: supernovae: general

Indexed keywords

ACCRETION DISCS; ACCRETION DISKS; COMPUTATIONAL BOX; COMPUTATIONAL GRIDS; CORE COLLAPSE SUPERNOVAE; DISPERSION RELATIONS; ENTROPY GRADIENTS; FINITE CONDUCTIVITY; HYDROSTATIC EQUILIBRIUM; IN-CORE; INSTABILITIES; INSTABILITY CRITERION; KEPLERIAN VELOCITY; MAGNETIC-FIELD GEOMETRY; MAGNETOHYDRODYNAMICS (MHD); MHD SIMULATION; MHD TURBULENCE; NUMERICAL CODE; NUMERICAL MODELS; ON TIME; PARAMETER SPACES; PHYSICAL EFFECTS; RADIAL ENTROPY; RAPID GROWTH; SATURATED STATE; SEMI-GLOBAL; SIMULATION BOXES; STARS: MAGNETIC FIELDS; STARS: SUPERNOVAE: GENERAL; VELOCITY GRADIENTS;

AMPLIFICATION; ASPECT RATIO; ENTROPY; FLOW SIMULATION; FLUID DYNAMICS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; MAGNETOS; NUMERICAL METHODS; ROTATION; STABILITY; STARS; TURBULENCE;

SIMULATORS;

EID: 66249121020     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811323     Document Type: Article

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