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Quark matter in compact stars?

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arxiv astro-ph/0606524 v2 pith:F4QGNQ5E submitted 2006-06-21 astro-ph hep-phnucl-th

classification astro-phhep-phnucl-th
keywords compactmatterquarkstarsdataactuallyastro-phcenter
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Ozel, in a recent reanalysis of EXO 0748-676 observational data (astro-ph/0605106), concluded that quark matter probably does not exist in the center of compact stars. We show that the data is actually consistent with the presence of quark matter in compact stars.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?

    nucl-th 2024-12 conditional novelty 6.0 of 10

    Hybrid stars with color-superconducting quark matter can reproduce the mass and spin of pulsar J0952-0607, whereas the hadronic-only model cannot, and the revised Kepler-frequency relation tightens radius bounds.

  2. Hybrid Stars with Post-Merger Rotation Profiles

    gr-qc 2026-06 unverdicted novelty 5.0 of 10

    Differential rotation in hybrid stars with deconfinement phase transition allows quasi-toroidal configurations with quark matter rings and leads to degeneracies in rotational profiles at mass-radius curve intersections.

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