Rotating neutron star models with a toroidal magnetic field - SFB/TR7
Rotating neutron star models with a toroidal magnetic field - SFB/TR7
Rotating neutron star models with a toroidal magnetic field - SFB/TR7
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12<br />
Results for an n=1 polytropic equation of state<br />
10 −2<br />
10 −3<br />
10 −4<br />
10 −5<br />
Bonazzola & Gourgoulhon (1996)<br />
Cutler (2002)<br />
Magnetic distortion ɛ B as a<br />
function of circumferential<br />
radius R at fixed average<br />
<strong>magnetic</strong> <strong>field</strong> strength for<br />
a non-rotating M = 1.4 M ⊙<br />
model computed according<br />
to Bonazzola & Gourgoulhon<br />
(1996) and Cutler<br />
(2002) respectively.<br />
−ǫ B<br />
10 1 10 2<br />
10 −6<br />
R [km]<br />
Joachim Frieben Golm, June 18, 2007