Magnetic field evolution in neutron stars: One-dimensional multi-fluid model

Astronomy and Astrophysics

Volumn 487, Issue 3, 2008, Pages 789-803

  Hoyos, J ^a   Reisenegger, A ^a   Valdivia, J A ^b  

^a PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^b UNIVERSITY OF CHILE   (Chile)

Author keywords

Magnetohydrodynamics (MHD); Methods: numerical; Stars: interiors; Stars: magnetic fields; Stars: neutron

Indexed keywords

ATOMS; COMPUTER SIMULATION; DIFFERENCE EQUATIONS; DIFFERENTIAL EQUATIONS; DIFFERENTIATION (CALCULUS); ELECTRIC FIELDS; ELECTROMAGNETIC FIELD THEORY; ELECTROMAGNETIC FIELDS; ELECTROMAGNETISM; EQUATIONS OF MOTION; INTEGRATION; MAGNETIC DOMAINS; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC MATERIALS; NEUTRONS; NONLINEAR EQUATIONS; NUMERICAL ANALYSIS; PARTIAL DIFFERENTIAL EQUATIONS; PLASMAS; POLYNOMIAL APPROXIMATION; PROTONS; SEMICONDUCTOR DOPING; STARS;

AMBIPOLAR DIFFUSION; BINARY COLLISIONS; CARTESIAN; CHEMICAL-; CONSERVATION LAWS; FINITE DIFFERENCING; HIGHLY NONLINEAR; INTER-PARTICLE COLLISIONS; IONIZED PLASMAS; LONG-TERM EVOLUTION; MAGNETOHYDRODYNAMICS (MHD); METHODS: NUMERICAL; MULTI FLUIDS; NEUTRON STARS; NORMAL-MODE ANALYSIS; NUMERICAL INTEGRATIONS; NUMERICAL SIMULATIONS; ONE-DIMENSIONAL; ONE-DIMENSIONAL GEOMETRY; ORTHOGONAL DIRECTIONS; PARAMETER VALUES; PARTICLE SPECIES; QUASI-EQUILIBRIUM; QUASI-EQUILIBRIUM STATES; SECOND ORDERS; STARS: INTERIORS; STARS: MAGNETIC FIELDS; STARS: NEUTRON; TIME-SCALES; WEAK INTERACTIONS;

MAGNETISM;

EID: 49749151006     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809466     Document Type: Article

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