A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
摘要相对场下的手徵强子模型研究了前中子星内(值)K凝聚和超子的生成。
A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
摘要相对场下的手徵强子模型研究了前中子星内(值)K凝聚和超子的生成。
It turns out that the weak interaction causes a kaon gradually to convert into its antiparticle, the antikaon, and then back again.
弱交作会使k介子逐渐变成反粒子──反k介子,然后又变回来。
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