A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.

摘要相对论平均场下手强子模型研究了前中子星内(平均值)K凝聚和超子生成。

It turns out that the weak interaction causes a kaon gradually to convert into its antiparticle, the antikaon, and then back again.

弱交互作会使k介子逐渐变成反粒子──反k介子，然后又变回来。