A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
摘要相对论平
手徵强子模型研究了前中子星内(平
值)K凝聚和超子
生成。
A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
摘要相对论平
手徵强子模型研究了前中子星内(平
值)K凝聚和超子
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介子逐渐变成反粒子──反k介子,然后又变回来。
声明:以上例句、词性分互联网资源自动生成,部分未经过人工审核,其表达内容亦不代表本软件
观点;若发现问题,欢迎向我们指正。
A chiral hadronic model is extended to investigate antikaon condensation and hyperons production of protoneutron stars.
要
相对论平均场下的手徵强子模型研究了前中子星内(平均值)K凝聚和超子的
。
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介子逐渐变
反粒子──反k介子,然后又变回来。
声明:以上例、词性分类均由互联网资源自动
,
分未经过人工审核,其表达内容亦不代表本软件的观点;若发现问题,欢迎向我们指正。
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的手徵强子模型研究了前中子星
(平均值)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.
弱交互作会使k介子逐渐变成反粒子──反k介子,然后又变回来。
声明:以上例句、词性分类均由互联网资源自动生成,部分未经过人工审核,其表亦不代表本软件的观点;若发现问题,欢迎向我们指正。
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
手徵强子模型研究了前中子星内(平均值)K凝聚和超子
。
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介子
反粒子──反k介子,然后又
回来。
声明:以上例句、词性分类均由互联网资源自动,部分未经过人工审核,其表达内容亦不代表本软件
观点;若发现问题,欢迎向我们指正。
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
强子模型研究了前中子星内(平均值)K凝聚和超子
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介子逐渐变成反粒子──反k介子,然后又变回来。
声明:以上例句、词均由互联网资源自动生成,部
未经过人工审核,其表达内容亦不代表本软件
观点;若发现问题,欢迎向我们指正。
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的手徵强子模型研究了前中子星内(平均值)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.
弱交互作会使k介子逐渐变成反粒子──反k介子,然后又变回来。
声明:以上例句、词性分类均由互联网资源自动生成,部分未经过人工审,
达内容亦不代
本软件的观点;若发现问题,欢迎向我们指正。
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的手徵强子模型研究了前中子星内(平均值)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.
弱交互作会使k
子逐渐变成
粒子──
k
子,然后又变回来。
声明:以上例句、词性分类均由互联网资源自动生成,部分未经过核,其表达内容亦不代表本软件的观点;若发现问题,欢迎向我们指正。
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的手徵强子模型研究了前中子星内(平均值)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.
弱交互作会使k介子逐渐变成反粒子──反k介子,然后又变回来。
声明:以上例句、词性分类均由互联网资源自动生成,部分未经过人工,
表达内容亦不代表本软件的观点;若发现问题,欢迎向我们指正。
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的手徵强子模型研
中子星内(平均值)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.
弱交互作会使k介子逐渐变成反粒子──反k介子,然后又变回
。
:以上例句、词性分类均由互联网资源自动生成,部分未经过人工审核,其表达内容亦不代表本软件的观点;若发现问题,欢迎向我们指正。