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- W2037617802 abstract "We study the properties of neutron stars using the complete relativistic equation of state based on the relativistic mean field theory. The complete relativistic equation of state covers a wide density range from 10(-7) to 1.2 fm(-3) for the use of describing both the interior region and the crusts of neutron stars. We include the Lambda, Sigma, and Xi hyperons which may appear as new degrees of freedom at high densities. We also examine the sensibility of the results to the choice of hyperon couplings." @default.
- W2037617802 created "2016-06-24" @default.
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- W2037617802 date "2003-04-24" @default.
- W2037617802 modified "2023-09-27" @default.
- W2037617802 title "Neutron Star Properties in the Relativistic Mean Field Theory" @default.
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- W2037617802 doi "https://doi.org/10.1088/0256-307x/20/5/317" @default.
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