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Reaction Rates and Transport in Neutron Stars

  • Andreas Schmitt
  • Peter Shternin
Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 457)

Abstract

Understanding signals from neutron stars requires knowledge about the transport inside the star. We review the transport properties and the underlying reaction rates of dense hadronic and quark matter in the crust and the core of neutron stars and point out open problems and future directions.

Notes

Acknowledgements

We thank M. Alford, A. Chugunov, A. Kaminker, A. Rebhan, S. Reddy, A. Sedrakian, I. Shovkovy, and D. Yakovlev for useful comments and discussions and acknowledge support from the NewCompStar network, COST Action MP1304. A.S. is supported by the Science & Technology Facilities Council (STFC) in the form of an Ernest Rutherford Fellowship. P.S. is supported by the Foundation for the Advancement of Theoretical Physics and Mathematics “BASIS” and the Russian Foundation for Basic Research grant # 16-32-00507-mol-a.

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© Springer Nature Switzerland AG 2018

Authors and Affiliations

  1. 1.Mathematical Sciences and STAG Research CentreUniversity of SouthamptonSouthamptonUK
  2. 2.Ioffe InstituteSt. PetersburgRussia

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