EMMI Rapid Reaction Task Force Meeting on 'Quark Matter in Compact Star'
arXiv:1402.6911 · doi:10.1088/0954-3899/41/12/123001
Abstract
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.
31 pages, summary of the EMMI Rapid Reaction Task Force on "Quark Matter in Compact Stars", October 7-10, 2013, FIAS, Goethe University, Frankfurt, Germany
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Cited by in corpus (49)
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- Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
- Compact stars with sequential QCD phase transitions
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- Relativistic parameterizations of neutron matter and implications for neutron stars
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- Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
- The Quarkyonic Star
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