Journal
PHYSICAL REVIEW LETTERS
Volume 86, Issue 10, Pages 1935-1938Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.86.1935
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With exact three-flavor Boltzmann neutrino transport, we simulate the stellar core collapse, bounce, and postbounce evolution of a M-13(.) star in spherical symmetry, the Newtonian limit, without invoking convection. In the absence of convection, prior spherically symmetric models, which implemented approximations to Boltzmann transport, failed to produce explosions. We consider exact transport to determine if these failures were due to the transport approximations made and to answer remaining fundamental questions in supernova theory, The model presented here is the first in a sequence of models beginning with different progenitors. In this model, a supernova explosion is not obtained.
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