tokens: We thank Kate Scholberg, André Rubbia, Masayuki Nakahata, and Lutz Köpke for useful conversations. We also thank Gabriel Martinez-Pinedo for providing us with tables for the 40 Ar cross sections. The authors acknowledge support provided by the NSF PetaApps program, under award OCI-0905046 via subaward no. 44592 from Louisiana State University to Princeton University, and by the Max-Planck/Princeton Center (MPPC) for Plasma Physics (NSF PHY-1144374). The authors employed computational resources provided by the TIGRESS high-performance computer center at Princeton University, which is jointly supported by the Princeton Institute for Computational Science and Engineering (PICSciE) and the Princeton University Office of Information Technology and by the National Energy Research Scientific Computing Center (NERSC), which is supported by the Office of Science of the US Department of Energy under contract DE-AC03-76SF00098. This work is part of the “Three Dimensional Modeling of Core-Collapse Supernovae” PRAC allocation support by the National Science Foundation (award number ACI-1440032). In addition, this research is part of the Blue Waters sustained-petascale computing project, which is supported by the National Science Foundation (awards OCI-0725070 and ACI-1238993) and the state of Illinois. Blue Waters is a joint effort of the University of Illinois at Urbana-Champaign and its National Center for Supercomputing Applications.
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