A new code for the Hall-driven magnetic evolution of neutron stars

Computer Physics Communications

Volumn 183, Issue 10, 2012, Pages 2042-2053

  Vigano D ^a   Pons, J A ^a   Miralles, J A ^a  

^a UNIVERSITY OF ALICANTE   (Spain)

Author keywords

EMHD; Hall MHD; Magnetohydrodynamics; Neutron stars; Numerical methods

Indexed keywords

CRUSTAL MAGNETIC FIELDS; CURRENT SHEETS; EMHD; FIELD EVOLUTION; FINITE DIFFERENCE; HALL MHD; INDUCTION EQUATIONS; LOCAL CONDITIONS; LONG TERM SIMULATION; MAGNETIC DIFFUSIVITY; MAGNETIC FIELD STRENGTHS; MAGNETIC REYNOLDS NUMBER; NEUTRON STARS; NUMERICAL MODELING; NUMERICAL PROBLEMS; OHMIC DISSIPATION; RELATIVE CONTRIBUTION; REPRESENTATIVE CASE; SPECTRAL METHODS;

MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; NEUTRONS; NUMERICAL METHODS; REYNOLDS NUMBER;

STARS;

EID: 84863100823     PISSN: 00104655     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.cpc.2012.04.029     Document Type: Article

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