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
手徵强
模型研究了前中星内(平均值)K凝聚和超
。
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徵强模型研究了前中星内(平均值)K凝聚和超。
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介逐
反粒──反k介，然后又回来。
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