The magnetic structure of neutron stars and their surface-to-core   temperature relation
  We study the relation between the mean effective surface temperature T_s and the internal temperature T_b 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 T_b(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. 
A. Y. Potekhin (1,2,3), V. Urpin (2,3), G. Chabrier (1) ((1) CRAL,   ENS-Lyon, (2) Ioffe Inst., St.Petersburg, (3) INI, St.P...