论文标题

在高密度下的触发生产机制和对称能量的见解

Insights on pion production mechanism and symmetry energy at high density

论文作者

Liu, Yangyang, Wang, Yongjia, Cui, Ying, Xia, Chen-Jun, Li, Zhuxia, Chen, Yongjing, Li, Qingfeng, Zhang, Yingxun

论文摘要

$nδ\ to nn $横截面,该部分考虑了m-matrix和动量$ p_ {nδ} $的$δ$ - 质量依赖性,用于在URQMD模型的框架内计算PION生产。我们的研究表明,与$δ$ - 质量相关的$nδ\ to nn $横截面相关的$δ$nδ\ cross截面的计算增强了倾斜度的多数,并降低了$π^ - /π^+$比率。通过分析在0.4A GEV的光束能量的Au+Au的脉冲产量的时间演变和重叠区域中的密度,我们发现Pion多重性探测了正常密度1-2倍的对称能量。跟踪反应中的pion产生过程,包括$ nn \ leftrightArrownδ$和$δ\ leftrightArrownπ$,我们的计算表明,在4-5 n- $δ$ - $π$ loops in Pion loops Path中,$π^ - /π^ - /π^+$对符号能量的敏感性被削弱$π^{ - }/π^{+} $在接近阈值的反应中的比率仍然是其对对称能量的敏感性。通过将计算与FOPI数据进行比较,我们获得了对称能量的模型依赖性结论,而在正常密度的两倍的对称能量为$ S(2ρ_0)$ = 38-73 MEV $1σ$不确定性。在中子星的潮汐变形性和最大质量的限制下,正常密度的对称能量降低至$ 48-58 $ MEV和对称能量的斜率$ l = 54-81 $ MEV,并且与Asy-Eos流数据的约束一致。

The $NΔ\to NN$ cross sections, which take into account the $Δ$-mass dependence of M-matrix and momentum $p_{NΔ}$, are applied on the calculation of pion production within the framework of the UrQMD model. Our study shows that UrQMD calculations with the $Δ$-mass dependent $NΔ\to NN$ cross sections enhance the pion multiplicities and decrease the $π^-/π^+$ ratios. By analyzing the time evolution of the pion production rate and the density in the overlapped region for Au+Au at the beam energy of 0.4A GeV, we find that the pion multiplicity probes the symmetry energy in the region of 1-2 times normal density. The process of pion production in the reaction is tracked including the loops of $NN\leftrightarrow NΔ$ and $Δ\leftrightarrow Nπ$, our calculations show that the sensitivity of $π^-/π^+$ to symmetry energy is weakened after 4-5 N-$Δ$-$π$ loops in the pion production path, while the $π^{-}/π^{+}$ ratio in reactions at near threshold energies remains its sensitivity to the symmetry energy. By comparing the calculations to the FOPI data, we obtain a model dependent conclusion on the symmetry energy and the symmetry energy at two times normal density is $S(2ρ_0)$=38-73 MeV within $1σ$ uncertainties. Under the constraints of tidal deformability and maximum mass of neutron star, the symmetry energy at two times normal density is reduced to $48-58$ MeV and slope of symmetry energy $L=54-81$ MeV, and it is consistent with the constraints from ASY-EOS flow data.

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