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EMMI Rapid Reaction Task Force Meeting on 'Quark Matter in Compact Star'

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arxiv 1402.6911 v1 pith:N4S6LI24 submitted 2014-02-27 astro-ph.HE hep-phnucl-th

EMMI Rapid Reaction Task Force Meeting on 'Quark Matter in Compact Star'

classification astro-ph.HE hep-phnucl-th
keywords starsmattermeetingquarkdataforcerecenttask
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The recent measurement of two solar mass pulsars has initiated an intense discussion on its impact on our understanding of the high-density matter in the cores of neutron stars. A task force meeting was held from October 7-10, 2013 at the Frankfurt Institute for Advanced Studies to address the presence of quark matter in these massive stars. During this meeting, the recent oservational astrophysical data and heavy-ion data was reviewed. The possibility of pure quark stars, hybrid stars and the nature of the QCD phase transition were discussed and their observational signals delineated.

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Cited by 1 Pith paper

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  1. Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO

    astro-ph.HE 2026-07 accept novelty 3.5

    SKAO's sensitivity, surveys and sub-arraying will deliver tighter NS mass, MoI, spin, glitch and precession constraints that, with X-ray and GW data, probe cold ultra-dense matter.