The magnetic structure of neutron stars and their surface-to-core temperature relation
نویسنده
چکیده
We study the relation between the mean effective surface temperature T s and the internal temperature Tb for magnetic neutron stars, assuming that the magnetic field near the surface has a presumably small-scale structure. The heavy-element (iron) and light-element (accreted) heat-blanketing envelopes are considered, and the results are compared with the case of a dipole magnetic field. We argue that the difference in the Tb(T s)-relation for different magnetic configurations is always much smaller than a possible difference caused by variations of the chemical composition in the envelope.
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