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5.3 Effect of magnetic fields on the EoS

Typical values of the surface magnetic field of radio pulsars are B ∼ 1012 g. For magnetars, surface magnetic fields can be as high as ∼ 1015 G. Effects of such fields on the EoS and structure of the crust are briefly reviewed in Section 6.4. A detailed study of the effect of BBB on neutron star envelopes can be found in Chapter 4 of [184Jump To The Next Citation Point].
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