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 |
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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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