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- W2036768823 abstract "The state of cold quark matter at supra-nuclear density, depending on the non-perturbative nature of quantum chromo-dynamics (QCD), is essential for modelling pulsars. It is conventionally thought that the state equation of dense matter softens and thus cannot result in high maximum mass if pulsars are quark stars. However, this standard point of view would be revisited and updated if the strong coupling between quarks at realistic baryon densities of compact stars could render quarks grouped in quark-clusters, because the state equation of clustering quark matter stiffs to support compact stars with maximum mass M max > 2M ⊙ . Although the hypothetical quark-clusters has not been confirmed due to the lack of both theoretical and experimental evidence, the astrophysical observations of pulsars (e.g. pulsar-mass) could help us to explore the properties of cold quark matter." @default.
- W2036768823 created "2016-06-24" @default.
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- W2036768823 date "2011-12-01" @default.
- W2036768823 modified "2023-09-23" @default.
- W2036768823 title "A 2M⊙ PULSAR: IMPLICATIONS FOR QUARK MATTER" @default.
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- W2036768823 doi "https://doi.org/10.1142/s0218301311040682" @default.
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