Simulation of the spherically symmetric stellar core collapse, bounce, and postbounce evolution of a star of 13 solar masses with boltzmann neutrino transport, and its implications for the supernova mechanism

Physical Review Letters

Volumn 86, Issue 10, 2001, Pages 1935-1938

  Mezzacappa, Anthony ^a   Liebendörfer, Matthias ^a,b,c   Messer, O E Bronson ^a,b,d   Hix, W Raphael ^a,b,d   Thielemann, Friedrich Karl ^a,c   Bruenn, Stephen W ^e  

^a OAK RIDGE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF TENNESSEE   (United States)

^c UNIVERSITY OF BASEL   (Switzerland)

^d OAK RIDGE NATIONAL LABORATORY   (United States)

^e FLORIDA ATLANTIC UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ASTRONOMY; COMPUTER SIMULATION; ELEMENTARY PARTICLE; MICROCLIMATE; PHYSICS; PROCEDURES;

ASTRONOMY; COMPUTER SIMULATION; ELEMENTARY PARTICLES; EXTRATERRESTRIAL ENVIRONMENT; PHYSICS;

APPROXIMATION THEORY; BINDING ENERGY; COMPUTER SIMULATION; ELECTRON TRAPS; ELEMENTARY PARTICLES; EQUATIONS OF STATE; RELATIVITY; TRANSPORT PROPERTIES;

BOLTZMANN NEUTRINO TRANSPORT; SPHERICALLY SYMMETRIC STELLAR CORE COLLAPSE; SUPERNOVA;

ASTROPHYSICS;

EID: 0037918108     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.86.1935     Document Type: Article

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