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    • Spin-driven changes in neutron star magnetic fields

      Malvin Ruderman

      Volume 16 Issue 2 June 1995 pp 207-216

    • Fulltext

       

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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/016/02/0207-0216

    • 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

    • Dates

       
      Published
      June 1995

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      Posted on January 27, 2016

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