Protoneutron star evolution and the neutrino-driven wind in general relativistic neutrino radiation hydrodynamics simulations

Astronomy and Astrophysics

Volumn 517, Issue 12, 2010, Pages

  Fischer, T ^a   Whitehouse, S C ^a   Mezzacappa, A ^b   Thielemann, F K ^a,c   Liebendorfer M ^a  

^a UNIVERSITY OF BASEL   (Switzerland)

^b OAK RIDGE NATIONAL LABORATORY   (United States)

^c GSI HELMHOLTZZENTRUM FÜR SCHWERIONENFORSCHUNG GMBH   (Germany)

Author keywords

Hydrodynamics; Neutrinos; Radiative transfer; Relativistic processes

Indexed keywords

CHEMICAL ELEMENTS; ENTROPY; EXPLOSIONS; HYDRODYNAMICS; KINETIC ENERGY; KINETICS; LUMINANCE; RADIATIVE TRANSFER; REACTION INTERMEDIATES; REACTION RATES; STARS;

NEUTRINO TRANSPORT; NEUTRINOS; PHYSICAL CONDITIONS; QUASI-STATIONARY STATE; R-PROCESS NUCLEOSYNTHESIS; RADIATION HYDRODYNAMICS; RADIATION HYDRODYNAMICS SIMULATION; SPHERICAL SYMMETRY;

NEUTRONS;

EID: 77955566072     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913106     Document Type: Article

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