Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state

Astronomy and Astrophysics

Volumn 467, Issue 2, 2007, Pages 395-409

  Oechslin, R ^a   Janka, H T ^a   Marek, A ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Equation of state; Gamma rays: bursts; Hydrodynamics; Methods: numerical; Stars: neutron

Indexed keywords

ANGULAR MOMENTUM; EQUATIONS OF STATE; HYDRODYNAMICS; NUMERICAL METHODS; STARS;

COLLISION INTERFACE; EINSTEIN EQUATIONS; GAMMA RAYS: BURSTS; METHODS: NUMERICAL; STARS: NEUTRON; SUPERNUCLEAR DENSITIES;

ASTROPHYSICS;

EID: 34249284198     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066682     Document Type: Article

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