Strong poloidal magnetic fields deform neutron stars and reduce central density, suppressing the direct Urca process and slowing thermal cooling.
1995 b , Astronomy and Astrophysics, 301, 757
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Axisymmetric Cooling of Neutron Stars with Strong Magnetic Fields
Strong poloidal magnetic fields deform neutron stars and reduce central density, suppressing the direct Urca process and slowing thermal cooling.