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The Composition of Baryon in the Proto Neutron Star PSR J0348+0432

机译:在原子中子星PSR J0348 + 0432中的Baryon的组成

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摘要

The effect of the mesons f(0)(975)(named as f ), phi(1020)(named as phi) and on the properties of the proto neutron star PSR J0348 + 0432 is studied in the framework of the relativistic mean field theory considering the baryon octet. We find the central particle number density will decrease considering the mesons but will increase as the mesons f, phi or mesons f, phi and all being considered. We also find that the mesons f, phi and have little effect on the field strengths of mesons sigma and but have a greater influence on those of mesons . For the chemical potential of neutrons, the influence of these mesons is relative small but for the chemical potential of electrons the meson effect is relatively large. It is also found that the relative particle number density of n will decrease while those of p and sigma(-) will increase considering the effect of the mesons , or f, phi, or f, phi and . The relative particle number density of , sigma(0), sigma(+), (-) and (0) will decrease considering the effect of the mesons but will increase as the mesons f, phi or the mesons f, phi and all being considered.
机译:在相对论平均场的框架中,研究了胶位F(0)(975)(命名为F),PHI(1020)(命名为PHI)和对原始中子星PSR J0348 + 0432的性质的影响考虑到Baryon Octet的理论。考虑到介子,我们发现中央粒子数密度将减少,但是将增加作为薄酯F,PHI或Mesons F,PHI和所有被认为。我们还发现偏斯蒙,辉,并对迈克斯西格玛的场地优点几乎没有影响,但对斯顿人有更大的影响。对于中子的化学潜力,这些介子的影响是相对较小的,但对于电子的化学电位,迈克森效应相对较大。还发现N的相对粒子数密度将减少,而P和Sigma( - )的效果会增加胶位,PHI或F,PHI和。考虑到介子的效果,而且将增加秒,但将随着偏蒙,猕猴或椎间子组,猕猴和所有存在的影响,σ(0),Σ(+),( - )和(0)的相对颗粒数密度降低,但将增加。经过考虑的。

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