The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse

Astronomy and Astrophysics

Volumn 514, Issue 7, 2010, Pages

  Scheidegger, S ^a   Kappeli R ^a   Whitehouse, S C ^a   Fischer, T ^a   Liebendorfer M ^a  

^a UNIVERSITY OF BASEL   (Switzerland)

Author keywords

Gravitational waves; Hydrodynamics; Neutrinos; Stars: neutron; Stars: rotation; Supernovae: general

Indexed keywords

COMPUTER SIMULATION; EQUATIONS OF STATE; FLUID DYNAMICS; GRAVITATIONAL EFFECTS; GRAVITY WAVES; HYDRODYNAMICS; MAGNETIC FIELDS; NEUTRONS; PLASMAS; RELATIVITY; STARS; WAVES;

AXISYMMETRIC; AXISYMMETRIC SIMULATION; COLLAPSE SIMULATION; COMBINED ACTIONS; DENSE MATTER; DYNAMICAL EVOLUTION; DYNAMICAL INSTABILITIES; EMISSION PROCESS; EQUATION OF STATE; FAST ROTATION; FIELD WINDING; FLUID INSTABILITY; GRAVITATIONAL ENERGY; GRAVITATIONAL WAVES; GRAVITATIONAL-WAVE SIGNALS; IN-LINE; ISOTROPIC DIFFUSION; JET FORMATION; LATTIMER; MAGNETIC FIELD PRESSURE; MODEL PARAMETERS; NARROW BANDS; NEUTRINO EMISSION; NEUTRINO PHYSICS; NEUTRON STARS; NUCLEAR EQUATIONS; PARAMETRISATION; PARTIAL IMPLEMENTATION; POLOIDAL MAGNETIC FIELD; QUANTITATIVE PREDICTION; ROTATION RATE; SIGNAL STEMMING; STARS:NEUTRON STARS; STELLAR CORE; STELLAR EVOLUTIONS; SUPERNOVA EXPLOSION; SUPERNOVAE: GENERAL; TOROIDAL MAGNETIC FIELDS; TWO-POINT; WAVE SIGNATURES; WEAK MAGNETIC FIELDS;

ROTATION;

EID: 77952468727     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913220     Document Type: Article

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