• Spin-driven changes in neutron star magnetic fields

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    • Abstract


      Interactions among a neutron star’s superfluid neutrons, superconducting protons, and solid crust cause predictable spin-down and spin-up driven crustal motion and magnetic field changes. Applications and unsolved problems are discussed for millisecond pulsar evolution and properties, glitches and post-glitch responses, and transcient gamma-ray emission.

    • Author Affiliations


      Malvin Ruderman1

      1. Department of Physics, Columbia University, 538 West 120th Street, New York, NY - 10027, USA
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