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- W1967000493 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." @default.
- W1967000493 created "2016-06-24" @default.
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- W1967000493 date "2007-02-01" @default.
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- W1967000493 title "PHASE TRANSITION IN ROTATING NEUTRON STARS" @default.
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- W1967000493 doi "https://doi.org/10.1142/s0218271807010092" @default.
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