摘要
据两类自由流阻尼标度理论算得的3代粒子质量及宇宙早期核子与现实核子质量的关系式,计算了宇宙暴胀时产生的3代粒子的超对称伴子质量,它们填充了175~^14 GeV的质标区.利用研究光子结构的类似方法,分析了轻子的夸克/胶子结构图象,其结果尚待实验证实.
Based on the mass of three generation particles, calculated from the damping scale theory of free currents of two classes, and on the formula of the relation between the mass of the early universe nucleon and that of the present one, the mass of the supersymmetry companions of three generation particles, which were born during the universe inflation, is calculated, and the mass fills up the mass scale region from 175 GeV to 1014 GeV. By the similar method used to study photon structure, the structure picture of quark-gluons of a lepton is analysed, the result of which is to be verified by experiments.
出处
《西南师范大学学报(自然科学版)》
CAS
CSCD
北大核心
2006年第1期61-65,共5页
Journal of Southwest China Normal University(Natural Science Edition)
基金
国家自然科学基金资助项目(10299040)
关键词
宇宙早期粒子
宇宙暴胀
超对称
轻子结构
early universe particle
universe inflation
supersymmetry
lepton structure