A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
摘要
相对论
场下的手徵强
模型研究了前中星内(
)K凝聚和超的生成。
A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
摘要相对论场下的手徵强模型研究了前中星内()K凝聚和超的生成。
It turns out that the weak interaction causes a kaon gradually to convert into its antiparticle, the antikaon, and then back again.
弱交互作会使k
逐渐变成反粒──反k，
后又变回来。
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