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Table 1

List of characteristic quantities for neutron stars with toroidal magnetic fields.

Model ρ c Uint/|W| Hmag/|W| Trot/|W| M 0 M b M0/Rcir

N22H5 2.2E-1 (1.24) 5.12E-1 5.01E-2 0 1.59E-1 (1.67) 1.73E-1 (1.81) 1.78E-1 37.4 (0.31)
N22H1 2.2E-1 (1.24) 5.32E-1 1.01E-2 0 1.60E-1 (1.68) 1.75E-1 (1.96) 1.87E-1 76.7 (0.63)
R22H2T8 2.2E-1 (1.24) 4.71E-1 1.50E-2 7.97E-2 1.84E-1 (1.93) 2.01E-1 (1.63) 1.55E-1 63.5 (0.63)
R22H08T8 2.2E-1 (1.24) 4.74E-1 7.86E-3 8.10E-2 1.85E-1 (1.94) 2.02E-1 (1.73) 1.65E-1 97.3 (0.93)

Notes. Central density (ρc), ratio of the internal energy to the gravitational potential energy W (Uint/|W|), ratio of the magnetic energy to W (Hmag/|W|), ratio of the rotational kinetic energy to W (Trot/|W|), ADM mass (M0), baryon rest mass (Mb), and compactness (M0/Rcir) with Rcir the equatorial circumferential radius. is an averaged Alfvén time in units of M0. The model name NXHY denotes nonrotating models with “X” and “Y” being the values of 100ρc and the values of 100Hmag/|W|, respectively. RXHYTZ denotes rotating models with “Z” for the values of 100Trot/|W|, where the meanings of “X” and “Y” are the same as the nonrotating models. The values shown in the brackets denote those in physical units, where the densities are normalized by 1015g/cm3, the masses by M, and the Alfvén time are given in units of millisecond. We set κ as 1.6 × 105 in CGS units.

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