SHOULD ONE USE THE RAY-BY-RAY APPROXIMATION IN CORE-COLLAPSE SUPERNOVA SIMULATIONS?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/831/i=1/a=81/pdf
Reference54 articles.
1. BEYOND MIXING-LENGTH THEORY: A STEP TOWARD 321D
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3. Stability of Standing Accretion Shocks, with an Eye toward Core‐Collapse Supernovae
4. RESULTS FROM CORE-COLLAPSE SIMULATIONS WITH MULTI-DIMENSIONAL, MULTI-ANGLE NEUTRINO TRANSPORT
5. THE DEVELOPMENT OF EXPLOSIONS IN AXISYMMETRICAB INITIOCORE-COLLAPSE SUPERNOVA SIMULATIONS OF 12–25 ${M}_{\odot }$ STARS
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