期刊
PHYSICAL REVIEW D
卷 92, 期 8, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.92.083002
关键词
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资金
- U.S. Department of Energy (DOE), Office of Science, Office of Nuclear Physics [DE-FG02-05ER41375]
- DOE Topical Collaboration Neutrinos and Nucleosynthesis in Hot and Dense Matter Grant [DE-SC0004955]
- NewCompStar, European Cooperation in Science and Technology (COST) Action [MP1304]
- U.S. Department of Energy (DOE) [DE-SC0004955] Funding Source: U.S. Department of Energy (DOE)
We discuss the constant speed of sound (CSS) parametrization of the equation of state of high-density matter and its application to the field correlator method (FCM) model of quark matter. We show how observational constraints on the maximum mass and typical radius of neutron stars are expressed as constraints on the CSS parameters. We find that the observation of a 2 M-circle dot star already severely constrains the CSS parameters, and is particularly difficult to accommodate if the squared speed of sound in the high-density phase is assumed to be around 1/3 or less. We show that the FCM equation of state can be accurately represented by the CSS parametrization, which assumes a sharp transition to a high-density phase with density-independent speed of sound. We display the mapping between the FCM and CSS parameters, and see that FCM only allows equations of state in a restricted subspace of the CSS parameters.
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