Erratum: Damping of vibrations and of the secular instability in quark stars

@article{Sawyer1989ErratumDO,
  title={Erratum: Damping of vibrations and of the secular instability in quark stars},
  author={R. Sawyer},
  journal={Physics Letters B},
  year={1989}
}
  • R. Sawyer
  • Published 1989
  • Physics
  • Physics Letters B
We calculate the bulk viscosity of hot quark matter, or “strange” matter, which could be present in neutron stars. In the temperature range characteristic of young neutron stars, the bulk viscosity arising from non-leptonic strangeness-changing quark-quark interactions is orders of magnitude larger than that which has been calculated for ordinary nuclear matter. The gravitational wave secular instability should be completely suppressed for quark stars, and the damping times for pulsations will… Expand
Bulk viscosity of Mixed nucleon-hyperon-quark Matter in Neutron stars
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