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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Results for an n=1 polytropic equation of state<br />
11<br />
1<br />
0.9<br />
-0.06<br />
-0.05<br />
0.8<br />
-0.04<br />
-0.03<br />
(Bp/5.34 × 10 17 G) 2<br />
0.7<br />
0.6<br />
0.5<br />
0.4<br />
0.3<br />
0.2<br />
-0.02<br />
-0.01<br />
0.01<br />
0<br />
0.02<br />
0.03<br />
0.04<br />
0.05<br />
0.06<br />
0.07<br />
0.08<br />
0.090.1<br />
Isocontours of distortion ɛ = −3/2×<br />
Q zz /I as a function of peak <strong>magnetic</strong><br />
<strong>field</strong> strength and rotation frequency<br />
for an M = 1.4 M ⊙ model<br />
<strong>with</strong> a circumferential radius of<br />
R = 12km in the non-magnetized<br />
case.<br />
0.1<br />
0.12 0.13<br />
0<br />
0.11<br />
0.14<br />
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1<br />
( f /828 Hz) 2<br />
Joachim Frieben Golm, June 18, 2007
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