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Table 1:

Summary of initial conditionsa.

$\Omega _{c,i}$ $\left[ {\rm rad~s}^{-1}\right]$ $\beta_{i}$ $\beta _{b}$ EoS $\rho_{b}\left[\frac{g}{{\rm cm}^3}\right]$ $B_{{\rm tor},i}$[G] $B_{{\rm pol},i}$[G] Em/|W|b Em/|W|f

0 0 0 E1 $4.39\times10^{14}$ $5\times10^9$ $1\times10^6$ $1.8\times10^{-9}$ $3.8\times10^{-8}$
R0E3CA 0 0 0 E3 $4.17\times10^{14}$ $5\times10^9$ $1\times10^6$ $1.8\times10^{-9}$ $3.1\times10^{-8}$
R0STCA 0 0 0 ST $3.38\times10^{14}$ $5\times10^9$ $1\times10^6$ $1.7\times10^{-9}$ $3.3\times10^{-8}$
R1E1CA 0.3 $0.59\times10^{-5}$ $1.7 \times10^{-4}$ E1 $4.53\times10^{14}$ $5\times10^9$ $1\times10^6$ $1.7\times10^{-9}$ $3.4\times10^{-8}$
R1E3CA 0.3 $0.59\times10^{-5}$ $1.7 \times10^{-4}$ E3 $4.17\times10^{14}$ $5\times10^9$ $1\times10^6$ $1.7\times10^{-9}$ $3.6\times10^{-8}$
R1E1DB 0.3 $0.59\times10^{-5}$ $1.7 \times10^{-4}$ E1 $4.53\times10^{14}$ $5\times10^{10}$ $1\times10^7$ $1.7\times10^{-7}$ $3.0\times10^{-6}$
R1STCA 0.3 $0.59\times10^{-5}$ $1.7 \times10^{-4}$ ST $3.38\times10^{14}$ $5\times10^9$ $1\times10^6$ $1.7\times10^{-9}$ $3.2\times10^{-8}$
R1E1CAL 0.3 $0.59\times10^{-5}$ $1.8 \times10^{-4}$ E1 $4.38\times10^{14}$ $5\times10^9$ $1\times10^6$ $6.1\times10^{-9}$ $1.2\times10^{-7}$
R2E1AC $\pi$ $ 0.64\times10^{-3}$ $1.6\times10^{-2}$ E1 $4.27\times10^{14}$ $1\times10^6$ $1\times10^9$ $6.5\times10^{-9}$ $1.27\times10^{-5}$
R2E3AC $\pi$ $ 0.64\times10^{-3}$ $1.6\times10^{-2}$ E3 $4.00\times10^{14}$ $1\times10^6$ $5\times10^9$ $6.4\times10^{-9}$ $5.1\times10^{-6}$
R2STAC $\pi$ $ 0.64\times10^{-3}$ $1.6\times10^{-2}$ ST $3.30\times10^{14}$ $1\times10^6$ $5\times10^9$ $6.4\times10^{-9}$ $3.6\times10^{-6}$
R3E1AC $2\pi $ $0.26\times10^{-2}$ $5.2\times10^{-2}$ E1 $3.80\times10^{14}$ $1\times10^6$ $5\times10^9$ $8.0\times10^{-9}$ $6.7\times10^{-6}$
R3E2AC $2\pi $ $0.26\times10^{-2}$ $5.1\times10^{-2}$ E2 $3.65\times10^{14}$ $1\times10^6$ $5\times10^9$ $8.9\times10^{-9}$ $7.2\times10^{-6}$
R3E3AC $2\pi $ $0.26\times10^{-2}$ $5.1\times10^{-2}$ E3 $3.64\times10^{14}$ $1\times10^6$ $5\times10^9$ $9.0\times10^{-9}$ $5.8\times10^{-6}$
R3STAC $2\pi $ $0.26\times10^{-2}$ $5.1\times10^{-2}$ ST $3.01\times10^{14}$ $1\times10^6$ $5\times10^9$ $8.9\times10^{-9}$ $4.7\times10^{-6}$
R3E1CA $2\pi $ $0.26\times10^{-2}$ $5.2\times10^{-2}$ E1 $3.82\times10^{14}$ $5\times10^9$ $1\times10^6$ $3.1\times10^{-9}$ $1.4\times10^{-8}$
R3E1DB $2\pi $ $0.26\times10^{-2}$ $5.2\times10^{-2}$ E1 $3.81\times10^{14}$ $5\times10^{10}$ $1\times10^7$ $3.1\times10^{-7}$ $1.6\times10^{-6}$
R3E1ACL 2$\pi$ $0.26\times10^{-2}$ $5.1\times10^{-2}$ E1 $3.65\times10^{14}$ $1\times10^6$ $5\times10^9$ $8.7\times10^{-9}$ $8.6\times10^{-5}$
R4E1AC $3\pi $ $0.57\times10^{-2}$ $8.6\times10^{-2}$ E1 $3.22\times10^{14}$ $1\times10^6$ $5\times10^9$ $1.2\times10^{-8}$ $1.3\times10^{-5}$
R4STAC $3\pi $ $0.57\times10^{-2}$ $9.0\times10^{-2}$ ST $2.69\times10^{14}$ $1\times10^6$ $5\times10^9$ $1.5\times10^{-8}$ $1.4\times10^{-5}$
R4E1EC $3\pi $ $0.57\times10^{-2}$ $8.6\times10^{-2}$ E1 $3.22\times10^{14}$ $1\times10^{11}$ $5\times10^9$ $2.4\times10^{-8}$ $1.3\times10^{-5}$
R4E1FC $3\pi $ $0.57\times10^{-2}$ $8.6\times10^{-2}$ E1 $3.19\times10^{14}$ $1\times10^{12}$ $5\times10^9$ $1.3\times10^{-4}$ $1.3\times10^{-4}$
R4E1FCL $3\pi $ $0.57\times10^{-2}$ $8.7\times10^{-2}$ E1 $3.14\times10^{14}$ $1\times10^{12}$ $5\times10^9$ $1.3\times10^{-4}$ $2.0\times10^{-4}$
R4E1CF $3\pi $ $0.57\times10^{-2}$ $8.2\times10^{-2}$ E1 $3.22\times10^{14}$ $5\times10^9$ $1\times10^{12}$ $5.8\times10^{-4}$ $5.9\times10^{-3}$
R5E1AC $4\pi $ $ 1.02\times10^{-2}$ $10.2\times10^{-2}$ E1 $2.47\times10^{14}$ $1\times10^6$ $5\times10^9$ $1.3\times10^{-8}$ $1.2\times10^{-5}$

Notes. (a) The subscript i stands for initial, b for bounce, while f stands for final. $\rho_{b}$ is the maximum central density at the time of core bounce. $B_{{\rm pol},i}$ and $B_{{\rm tor},i}$ abbreviate the initially imposed toroidal and poloidal magnetic fields, whereas Em/|W| stands for the ratio of magnetic to gravitational energy. The subscript L denotes models which were carried out with the leakage scheme.

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