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David Blaschke (Uniwersytet Wroclawski
, Wroclaw
, Poland & Bogoliubovn Laboratory for Theoretical Physics
2008
Depending on the density reached in the cores of neutron stars, such objects may contain stable phases of novel matter found nowhere else in the Universe. This article gives a brief overview of these phases of matter and discusses astrophysical const
raints on the high-density equation of state associated with ultra-dense nuclear matter.