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Solid State Physics and Cooling of Neutron Stars

  • Sachiko Tsuruta
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 55)

Abstract

First we show the possible effect of the ‘magnetic’ condensation on cooling of neutron stars. Its observational significance (especially for younger pulsars such as the Crab pulsar) is emphasized. Other effects of solid state physics on cooling are also discussed.

Keywords

Neutron Star Stellar Surface Outer Envelope Observational Significance Magnetic Metal 
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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1976

Authors and Affiliations

  • Sachiko Tsuruta
    • 1
  1. 1.Astronomy CentreUniversity of SussexFalmerEngland

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