On the dynamics of proto-neutron star winds and r-process nucleosynthesis

Astronomy and Astrophysics

Volumn 494, Issue 3, 2009, Pages 829-844

  Panov, I V ^a,b   Janka, H Th ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b INSTITUTE FOR THEORETICAL AND EXPERIMENTAL PHYSICS   (Russian Federation)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: neutron; Stars: supernovae: general; Stars: winds, outflows

Indexed keywords

CHEMICAL ELEMENTS; COOLING; DECAY (ORGANIC); DYNAMICS; NUCLEAR ENERGY; NUCLEAR PHYSICS; NUCLEAR REACTORS; PLATINUM; STARS; SUPERCONDUCTING TRANSITION TEMPERATURE; WIND; WIND EFFECTS;

CAPTURE RATES; COMPACT OBJECTS; CONSTANT DENSITIES; DECAY RATES; EXPANSION BEHAVIORS; LOW TEMPERATURES; NEUTRON DENSITIES; NEUTRON STARS; NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES; POWER-LAW DECAYS; QUASI EQUILIBRIUMS; R PROCESS; R-PROCESS NUCLEOSYNTHESIS; SECOND PHASE; SIMPLIFIED MODELS; STARS: NEUTRON; STARS: SUPERNOVAE: GENERAL; STARS: WINDS, OUTFLOWS; TEMPERATURE REGIMES; TERMINATION SHOCKS; TIME-SCALE; TRANSITION TEMPERATURES;

NEUTRONS;

EID: 60349109462     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810292     Document Type: Article

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