The lifetime of a hyperon bounded in a hypernucleus is affected by the nuclear environment.

束缚在超中的超的寿命会受到原境的影响。

When we study hadronization mechanism through hyperon polarization, we must firstly consider about this two factors.

因此,利用超极化研究强产生机制时,都必须首先将这两个因进来。

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的手徵强模型研究了前中星内(平均值)K凝聚和超的生成。