A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
摘要用相对论平均场下手徵强研究了前中星(平均值)K凝聚和超成。
It turns out that the weak interaction causes a kaon gradually to convert into its antiparticle, the antikaon, and then back again.
弱交互作用会使k介逐渐变成反粒──反k介,然后又变回来。
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