All Tables

Table 1: Main properties of the tori considered in the numerical calculations. From left to right the columns report: the name of the model, the specific angular momentum $\ell$ (normalized to M), the polytropic constant $\kappa$ , the inner and outer cusps of the torus, $r_{\rm ci}$ and $r_{\rm co}$ , the radial position of the pressure maximum $r_{\rm max}$ (all radii are in units of the gravitational radius $r_{\rm g}$ ), the potential gaps $\Delta W_{\rm {i}}\equiv W_{\rm {in}}-W_{\rm {ci}}$ and $\Delta W_{\rm {o}}\equiv W_{\rm {in}}-W_{\rm {co}}$ , where $W_{\rm {in}}$ is the potential at the inner edge of the disc. The last column reports the orbital period at the centre of the torus, $t_{\rm orb}$ , expressed in milliseconds. All of the models share the same value of the cosmological parameter y=10^-6, the same mass for the black hole, $M=10~M_{\odot}$ , the same adiabatic index $\gamma =4/3$ , and the same torus-to-hole mass ratio $M_{\rm t}/M=0.2$ .