All Tables

Table 1: Parameters of the torus evolution models. The 3D simulations were performed with three levels of nested Cartesian grids with the number of grid cells per level and spatial direction given in column "zone''. $\Delta t_{\rm cal}$ is the time interval over which the model was evolved. All models started with a black hole mass of $M_{\rm BH}^{\rm i} = 4.017 ~M_\odot$ . The initial torus masses are given by $M_{\rm d}^{\rm i}$ , $0 \le a \le 1$ is the initial value of the dimensionless BH spin parameter, "pro'' means that torus and BH were chosen to rotate in the same direction, "ret'' means opposite directions of rotation, and $\alpha$ denotes the dimensionless disk viscosity parameter.
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 $\langle\epsilon_{\nu_x}\rangle$ .
Table 3: Torus mass $M_{\rm d}$ , black hole mass accretion rate $\dot M_{\rm d}$ , estimated accretion time scale of the torus, $t_{\rm acc}\equiv M_{\rm d}/\dot M_{\rm d}$ , total neutrino luminosity $L_\nu$ , integral rate of energy deposition by neutrino-antineutrino annihilation around the accretion torus, $\dot{E}_{\nu\bar{\nu}}$ , and total energy deposition by $\nu\bar\nu$ annihilation in the time interval $t_{\rm fin}$ , $E_{\nu\bar{\nu}}$ , for all 64-resolution models. All quantities are given at time $t_{\rm fin}$ after the start of the simulation.