Affiliation:
1. Observatoire de la Côte d'Azur, Nice, France
Abstract
We review the properties of a phase transition from hadronic matter to deconfined strange quark matter in the core of neutron stars. The neutron star equation of state is computed using a non-linear field theoretical model and the MIT bag model. Rapidly rotating neutron star configurations are studied and the consequences of the conversion and a subsequently micro-collapse, such as gravitational wave emission and pulsar spin-up, are analyzed.
Publisher
World Scientific Pub Co Pte Lt
Subject
Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics
Cited by
1 articles.
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