论文标题

晶格QCD数据和中子星中黑德子的排斥特性

Repulsive properties of hadrons in lattice QCD data and neutron stars

论文作者

Motornenko, Anton, Pal, Somenath, Bhattacharyya, Abhijit, Steinheimer, Jan, Stoecker, Horst

论文摘要

二阶敏感性$χ^{11} _ {ij} $ of Baryon,Electric and Strangeness,$ b $,$ Q $和$ s $,费用,收费是在手学均值字段(CMF)模型中计算的,并与可用的lattice QCD数据进行了比较。敏感性对不同强子物种之间的短距离排斥相互作用敏感,尤其是对超子的硬核排斥。与非爆炸式重子的大小相比,减小超子大小的尺寸确实显着提高了CMF模型结果与晶格QCD数据的一致性。电荷依赖性的敏感性对介子的短距离排斥体积敏感。与晶格QCD数据的比较表明,奇怪的重子,非震动介子和奇怪的媒介物的排除体积明显小于非震撼人心。具有这些修饰的强子体积的CMF模型允许对QCD易感性的宽带描述显着高于手性伪临界温度。这种改进的基于晶格QCD数据的CMF模型已用于研究冷QCD物质和中子星物质的特性。在两种情况下,相结构基本上都没有变化,即手性的一阶相变发生在低温下($ t _ {\ rm cp} \大约17 $ meV),而超音长则与非抗震动Hadron相比,将其脱发至更高的密度。中子恒星最大质量保持接近2.1 $ m_ \ odot $,并且由于超子的出现,质量 - 拉迪乌斯图仅稍微修改,并且与天体物理观测一致。

Second-order susceptibilities $χ^{11}_{ij}$ of baryon, electric, and strangeness, $B$, $Q$, and $S$, charges, are calculated in the Chiral Mean Field (CMF) model and compared to available lattice QCD data. The susceptibilities are sensitive to the short range repulsive interactions between different hadron species, especially to the hardcore repulsion of hyperons. Decreasing the hyperons size, as compared to the size of the non-strange baryons, does improve significantly the agreement of the CMF model results with the Lattice QCD data. The electric charge-dependent susceptibilities are sensitive to the short range repulsive volume of mesons. The comparison with lattice QCD data suggests that strange baryons, non-strange mesons and strange mesons have significantly smaller excluded volumes than non-strange baryons. The CMF model with these modified hadron volumes allows for a mainly hadronic description of the QCD susceptibilities significantly above the chiral pseudo-critical temperature. This improved CMF model which is based on the lattice QCD data, has been used to study the properties of both cold QCD matter and neutron star matter. The phase structure in both cases is essentially unchanged, i.e. a chiral first-order phase transition occurs at low temperatures ($T_{\rm CP}\approx 17$ MeV), and hyperons survive deconfinement to higher densities than non-strange hadrons. The neutron star maximal mass remains close to 2.1$M_\odot$ and the mass-radius diagram is only modified slightly due to the appearance of hyperons and is in agreement with astrophysical observations.

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