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tokens: The authors acknowledge Chuck Horowitz, Evan O’Connor, and Todd Thompson for productive conversations, concerning insight into and help with the microphysics, and Ernazar Abdikamalov, Sean M. Couch, Luke F. Roberts, and Christian D. Ott for fruitful discussions on the nature of core-collapse supernovae. Support was provided by the Max-Planck/Princeton Center (MPPC) for Plasma Physics (NSF PHY-1523261). D.R. gratefully acknowledges support from the Schmidt Fellowship. A.B. acknowledges support from the NSF under award number AST-1714267. J.D. acknowledges support from a Laboratory Directed Research and Development Early Career Research award at LANL. 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 (DOE) under contract DE-AC03-76SF00098. The authors express their gratitude to Ted Barnes of the DOE Office of Nuclear Physics for facilitating their use of NERSC. This paper has been assigned a LANL preprint # LA-UR-17-20973.