Viscosity and Rotation in Core-Collapse Supernovae

Details Viscosity and Rotation in Core-Collapse Supernovae Viscosity and Rotation in Core-Collapse Supernovae

2004-03-09

arxiv.org/abs/astro-ph/0403224v2

Astrophys.J. 620 (2005) 861-877

Astronomy and Astrophysics

Astrophysics

accepted to ApJ, references added, discussion tightened, 26 pages, 11 figures, emulateapj

Scientific paper

10.1086/427177

We construct models of core-collapse supernovae in one spatial dimension, including rotation, angular momentum transport, and viscous dissipation employing an alpha-prescription. We compare the evolution of a fiducial 11 M_sun non-rotating progenitor with its evolution including a wide range of imposed initial rotation profiles (1.25

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