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Updated: Aug 23, 2026

Hyperpolarized Xenon for NMR and MRI Applications
Published on: September 6, 2012
Phase transition to hyperon matter in neutron stars
Jürgen Schaffner-Bielich1, Matthias Hanauske, Horst Stöcker
1Department of Physics, Columbia University, 538 West 120th Street, New York, New York 10027, USA.
Abstract:
Recent progress in the understanding of the high density phase of neutron stars advances the view that a substantial fraction of the matter consists of hyperons. The possible impacts of a highly attractive interaction between hyperons on the properties of compact stars are investigated. We find that a hadronic equation of state with hyperons allows for a first order phase transition to hyperonic matter. The corresponding hyperon stars can have rather small radii of R approximately equal 8 km.
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