All Tables

Table 1: Properties of non-rotating PNSs and rigidly rotating PNSs at the limiting frequency, for a fixed baryonic mass $M_{\rm B} = 1.6~M_{\hbox{$\odot$ }}$ . The models are labeled by the evolutionary time of non-rotating PNSs at which the thermodynamical profile was calculated. The entries in the table are: central baryon number density, $n_{\rm c}$ ; gravitational mass, $M_{\rm G}$ ; circumferential equatorial radius, $R_{\rm eq}$ ; Kepler frequency, $\Omega _{\rm K}$ ; angular momentum, J; axis ratio r (polar to equatorial) and the rotation parameter |T/W| (rotational energy on absolute value of gravitational energy). For 4 time steps at early times we give results using the LS EOS at low densities for comparison (first four rows, between parenthesis).
Table 2: Properties of non-rotating PNSs and rigidly rotating PNSs at the limiting frequency, for a fixed baryonic mass $M_{\rm B} = 1.2~M_{\hbox{$\odot$ }}$ . The entries in the table are the same as in Table 1.