Dynamic migration of rotating neutron stars due to a phase transition instability

Monthly Notices of the Royal Astronomical Society

Volumn 396, Issue 4, 2009, Pages 2269-2288

  Dimmelmeier, Harald ^a   Bejger, Michal ^b   Haensel, Pawel ^b   Zdunik, J Leszek ^b  

^a ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

Author keywords

Hydrodynamics; Methods: numerical; Relativity; Stars: neutron; Stars: rotation

Indexed keywords

BLACK HOLES; DAMPING; EQUATIONS OF STATE; GALAXIES; GRAVITATIONAL EFFECTS; GRAVITY WAVES; HADRONS; NEUTRONS; NUMERICAL METHODS; RADIATION EFFECTS; RELATIVITY; ROTATION; STARS; VISCOSITY;

DENSE CORE; DENSITY JUMPS; DYNAMIC MIGRATION; EQUATION-OF-STATE; GRAVITATIONAL RADIATION; METHOD: NUMERICAL; NEUTRON STARS; RELATIVISTIC HYDRODYNAMICS; STARS: NEUTRONS; STARS: ROTATION;

HYDRODYNAMICS;

EID: 67649883433     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14891.x     Document Type: Article

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