Ohmic decay of internal magnetic fields in neutron stars

Details Ohmic decay of internal magnetic fields in neutron stars Ohmic decay of internal magnetic fields in neutron stars

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...229..133h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 229, no. 1, March 1990, p. 133-137.

Astronomy and Astrophysics

Astrophysics

49

Neutron Stars, Stellar Magnetic Fields, Dense Plasmas, Electrical Resistivity, Stellar Interiors, Stellar Models, Stellar Temperature

Scientific paper

The electric resistivity of the interiors of neutron stars can significantly increase in the presence of a magnetic field which strongly influences the motion of the charge carriers. The internal magnetic field may decay, irrespectively of its initial value, to about 10 to the 12th G in about 10 to the 7th yr, producing the heat release which delays noticeably the cooling process.

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