Table 2: Some results for the torus evolution models. The dynamical simulations were performed over a time interval of $\Delta t_{\rm cal}$ . All quantities refer to the conditions found at the end of the simulations. $M_{\rm d}$ is the mass of the gas of the disk, $T_{\rm max}$ is the maximum gas temperature in energy units, $L_{\nu _{\rm e}}$ denotes the electron neutrino luminosity near the end of the simulation, $L_{\bar{\nu}_{\rm e}}$ the corresponding electron antineutrino luminosity, and $L_{\nu _x}$ the luminosity of heavy-lepton neutrinos (summed for $\nu _{\mu }$ , $\bar\nu_{\mu}$ , $\nu _{\tau }$ or $\bar\nu_{\tau}$ , which are all treated equally). The sum of all neutrino luminosities is given by $L_\nu$ , and the mean energies of the different neutrino types by $\langle\epsilon_{\nu_{\rm e}}\rangle$ , $\langle\epsilon_{\bar{\nu}_{\rm e}}\rangle$ and $\langle\epsilon_{\nu_x}\rangle$ .
Model $\Delta t_{\rm cal}$ $M_{\rm d}$ $T_{\rm max}$ $L_{\nu _{\rm e}}$ $L_{\bar{\nu}_{\rm e}}$ $L_{\nu _x}$ $L_\nu$ $\langle\epsilon_{\nu_{\rm e}}\rangle$ $\langle\epsilon_{\bar{\nu}_{\rm e}}\rangle$ $\langle\epsilon_{\nu_x}\rangle$

ms $10^{-2}M_\odot$ MeV $10^{50}\frac{\rm erg}{\rm s}$ $10^{50}\frac{\rm erg}{\rm s}$ $10^{50}\frac{\rm erg}{\rm s}$ $10^{50}\frac{\rm erg}{\rm s}$ MeV MeV MeV

r00-32 70.0 1.06 2.6 0.08 0.22 0.002 0.3 9.7 9.3 7.8

al1-32 70.0 1.14 3.3 0.2 0.6 0.01 0.8 12.5 12.0 10.0

al2-32 70.0 1.25 4.3 1.0 2.9 0.1 4.0 15.4 15.2 12.8

al3-32 70.0 1.43 5.0 1.4 3.9 0.2 5.5 17.5 17.2 14.7

al4-32 70.0 0.84 5.9 4.0 9.0 2.0 15.0 17.5 19.2 16.9

ro1-32 70.0 1.54 3.8 0.3 0.8 0.008 1.1 11.3 11.0 9.4

ro2-32 70.0 2.10 4.5 0.7 1.8 0.03 2.5 11.4 11.2 9.7

ro3-32 70.0 2.02 6.4 9.0 14.0 0.4 23.0 18.2 19.1 18.3

ro4-32 70.0 0.67 2.1 0.009 0.02 0.0006 0.03 8.5 8.3 6.9

ro5-32 70.0 0.56 1.8 <0.005 <0.01 <0.0002 <0.015 5.8 6.1 5.4

ir1-32 70.0 0.46 1.4 <0.0005 <0.0005 <0.0001 <0.001 5.1 5.6 4.7

ir2-32 70.0 0.57 1.9 <0.0025 <0.0025 <0.0005 <0.005 6.8 6.7 5.7

ir3-32 70.0 2.35 3.1 1.7 2.4 0.035 4.1 11.9 11.4 9.6

ir4-32 70.0 4.31 7.1 34.0 50.0 2.0 86.0 17.3 17.3 17.0

r00-64 40.0 2.22 4.2 0.6 1.2 0.01 1.8 12.0 11.6 10.2

al3-64 40.0 2.44 5.6 3.4 7.7 0.3 11.4 16.4 17.8 15.4

al4-64 40.0 1.76 8.7 18.0 55.0 7.0 80.0 21.3 22.8 20.1

ri4-64 40.0 12.22 7.0 26.0 43.0 1.0 70.0 14.5 16.5 17.9

ro2-64 40.0 3.10 4.6 1.6 1.8 0.02 3.4 12.9 11.7 11.7

ro5-64 40.0 1.13 3.9 0.3 0.7 0.01 1.0 12.2 11.8 9.8

ir1-64 40.0 0.71 2.4 0.07 0.03 0.001 0.1 9.4 8.4 7.0

ir4-64 40.0 7.87 6.2 7.2 15.0 0.2 22.4 13.8 12.8 14.9

ir5-64 40.0 8.77 10.4 150.0 350.0 110.0 610.0 20.7 20.9 26.7

ar1-64 40.0 2.34 6.6 25.0 70.0 15.0 110.0 21.5 22.7 20.3

ar2-64 40.0 10.44 9.5 120.0 240.0 80.0 440.0 19.4 19.7 25.2

**Table 2:** Some results for the torus evolution models. The dynamical simulations were performed over a time interval of $\Delta t_{\rm cal}$ . All quantities refer to the conditions found at the end of the simulations. $M_{\rm d}$ is the mass of the gas of the disk, $T_{\rm max}$ is the maximum gas temperature in energy units, $L_{\nu _{\rm e}}$ denotes the electron neutrino luminosity near the end of the simulation, $L_{\bar{\nu}_{\rm e}}$ the corresponding electron antineutrino luminosity, and $L_{\nu _x}$ the luminosity of heavy-lepton neutrinos (summed for $\nu _{\mu }$ , $\bar\nu_{\mu}$ , $\nu _{\tau }$ or $\bar\nu_{\tau}$ , which are all treated equally). The sum of all neutrino luminosities is given by $L_\nu$ , and the mean energies of the different neutrino types by $\langle\epsilon_{\nu_{\rm e}}\rangle$ , $\langle\epsilon_{\bar{\nu}_{\rm e}}\rangle$ and $\langle\epsilon_{\nu_x}\rangle$ .
Model	$\Delta t_{\rm cal}$	$M_{\rm d}$	$T_{\rm max}$	$L_{\nu _{\rm e}}$	$L_{\bar{\nu}_{\rm e}}$	$L_{\nu _x}$	$L_\nu$	$\langle\epsilon_{\nu_{\rm e}}\rangle$	$\langle\epsilon_{\bar{\nu}_{\rm e}}\rangle$	$\langle\epsilon_{\nu_x}\rangle$
	ms	$10^{-2}M_\odot$	MeV	$10^{50}\frac{\rm erg}{\rm s}$	$10^{50}\frac{\rm erg}{\rm s}$	$10^{50}\frac{\rm erg}{\rm s}$	$10^{50}\frac{\rm erg}{\rm s}$	MeV	MeV	MeV
r00-32	70.0	1.06	2.6	0.08	0.22	0.002	0.3	9.7	9.3	7.8
al1-32	70.0	1.14	3.3	0.2	0.6	0.01	0.8	12.5	12.0	10.0
al2-32	70.0	1.25	4.3	1.0	2.9	0.1	4.0	15.4	15.2	12.8
al3-32	70.0	1.43	5.0	1.4	3.9	0.2	5.5	17.5	17.2	14.7
al4-32	70.0	0.84	5.9	4.0	9.0	2.0	15.0	17.5	19.2	16.9
ro1-32	70.0	1.54	3.8	0.3	0.8	0.008	1.1	11.3	11.0	9.4
ro2-32	70.0	2.10	4.5	0.7	1.8	0.03	2.5	11.4	11.2	9.7
ro3-32	70.0	2.02	6.4	9.0	14.0	0.4	23.0	18.2	19.1	18.3
ro4-32	70.0	0.67	2.1	0.009	0.02	0.0006	0.03	8.5	8.3	6.9
ro5-32	70.0	0.56	1.8	<0.005	<0.01	<0.0002	<0.015	5.8	6.1	5.4
ir1-32	70.0	0.46	1.4	<0.0005	<0.0005	<0.0001	<0.001	5.1	5.6	4.7
ir2-32	70.0	0.57	1.9	<0.0025	<0.0025	<0.0005	<0.005	6.8	6.7	5.7
ir3-32	70.0	2.35	3.1	1.7	2.4	0.035	4.1	11.9	11.4	9.6
ir4-32	70.0	4.31	7.1	34.0	50.0	2.0	86.0	17.3	17.3	17.0
r00-64	40.0	2.22	4.2	0.6	1.2	0.01	1.8	12.0	11.6	10.2
al3-64	40.0	2.44	5.6	3.4	7.7	0.3	11.4	16.4	17.8	15.4
al4-64	40.0	1.76	8.7	18.0	55.0	7.0	80.0	21.3	22.8	20.1
ri4-64	40.0	12.22	7.0	26.0	43.0	1.0	70.0	14.5	16.5	17.9
ro2-64	40.0	3.10	4.6	1.6	1.8	0.02	3.4	12.9	11.7	11.7
ro5-64	40.0	1.13	3.9	0.3	0.7	0.01	1.0	12.2	11.8	9.8
ir1-64	40.0	0.71	2.4	0.07	0.03	0.001	0.1	9.4	8.4	7.0
ir4-64	40.0	7.87	6.2	7.2	15.0	0.2	22.4	13.8	12.8	14.9
ir5-64	40.0	8.77	10.4	150.0	350.0	110.0	610.0	20.7	20.9	26.7
ar1-64	40.0	2.34	6.6	25.0	70.0	15.0	110.0	21.5	22.7	20.3
ar2-64	40.0	10.44	9.5	120.0	240.0	80.0	440.0	19.4	19.7	25.2

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