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The Properties of the Neutron Star PSR B2303+46

机译:中子星PSR B2303 + 46的性质

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The properties of the neutron star PSR B2303+46 are investigated within the framework of relativistic mean field theory for the baryon octet system through adjusting the hyperon coupling constants. Models for the neutron star B2303+46 are obtained by choosing suitable hyperon coupling constants x_(σh) and x_(ωh), with x_(ρh) being determined by the constituent quark model SU(6) symmetry and the nucleon coupling constants being chosen as the set CZ11. Our results show that the field strengths of the mesons σ, ω, and ρ, the chemical potentials of the neutron and electron, the relative particle number density of the electron, muon, neutron, proton, Λ, Σ, and Ξ, and the pressure and energy density of the neutron star PSR B2303+46 all have an uncertain value region, respectively.
机译:通过调整超子耦合常数,在相对论平均场理论的基础上研究了重子八位位组系统的中子星PSR B2303 + 46的性质。通过选择合适的超子耦合常数x_(σh)和x_(ωh)获得中子星B2303 + 46的模型,其中x_(ρh)由构成夸克模型SU(6)对称性确定并选择核子耦合常数。作为套装CZ11。我们的结果表明介子σ,ω和ρ的场强,中子和电子的化学势,电子,μ子,中子,中子,质子,Λ,Σ和relative的相对粒子数密度以及PSR B2303 + 46的中子星压力和能量密度分别具有不确定的值区域。

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