Magnetic field amplification in proto-neutron stars: The role of the neutron-finger instability for dynamo excitation

Astronomy and Astrophysics

Volumn 479, Issue 1, 2008, Pages 167-176

  Naso, L ^a   Rezzolla, L ^b,c,d   Bonanno, A ^e   Paterno L ^f  

^a SISSA   (Italy)

^b ALBERT EINSTEIN INSTITUT   (Germany)

^c LOUISIANA STATE UNIVERSITY   (United States)

^d SEZIONE DI TRIESTE   (Italy)

^e INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^f UNIVERSITY OF CATANIA   (Italy)

Author keywords

Instabilities; Magnetohydrodynamics (MHD); Stars: magnetic fields; Stars: neutron; Stars: rotation; Turbulence

Indexed keywords

MAGNETIC FIELDS; STARS; TURBULENCE;

INSTABILITIES; NEUTRON-FINGER INSTABILITY; PROTONEUTRON STARS; RAYLEIGH-TYPE CONVECTION;

MAGNETOHYDRODYNAMICS;

EID: 38849098355     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078360     Document Type: Article

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