5.3 Effect of magnetic fields on the EoS
Typical values of the surface magnetic field of radio pulsars are . 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 on neutron star envelopes can be
found in Chapter 4 of .