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 realistic equations of state<br />
13<br />
Isocontours of the <strong>magnetic</strong> <strong>field</strong><br />
strength for a non-rotating M = 1.4 M ⊙<br />
model based on the SLy4 EOS. The peak<br />
value is B p = 2.47 × 10 17 G which is the<br />
maximum possible.<br />
Joachim Frieben Golm, June 18, 2007