High-resolution calculations of merging neutron stars - II. Neutrino emission

Monthly Notices of the Royal Astronomical Society

Volumn 342, Issue 3, 2003, Pages 673-689

  Rosswog, S ^a   Liebendorfer M ^b  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

^b UNIVERSITY OF TORONTO   (Canada)

Author keywords

Dense matter; Gamma rays: bursts; Hydrodynamics; Methods: numerical; Neutrinos; Stars: neutron

Indexed keywords

EQUATIONS OF STATE; GAMMA RAYS; LUMINANCE; MERGING; NEUTRONS; NUMERICAL METHODS; SUPERNOVAE;

DENSE MATTER; GAMMA RAYS BURSTS; HIGH RESOLUTION; HIGH RESOLUTION SIMULATIONS; METHOD: NUMERICAL; NEUTRINO EMISSION; NEUTRON STARS; NEWTONIANS; STARS: NEUTRONS; THREE-DIMENSIONAL SMOOTHED PARTICLE HYDRODYNAMICS;

HYDRODYNAMICS;

EID: 0142105401     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06579.x     Document Type: Article

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