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银心和星系核的磁单极模型
彭秋和,王德焴,李宗云
1985
Source Publication科学通报
ISSN0023-074X
Issue9Pages:686-691
Abstract<正> 改进后的暴涨宇宙学认为,宇宙极早期的相变时期Higgs场的急剧振荡和热涨落将可能产生极微量的磁单极(m_m~10~(16)m_p,对于无色磁单极而言,磁荷g_m=3hc/2e)。按照Parker、Lazarides等人的分析,宇宙极早期遗留的磁单极数目与核子总数之比ζ_0(≡(N_m/N_B)_0)(?)10~(-20±1)。
Keyword星系核 磁单极 暴涨宇宙 热涨落 相变 核子 Higgs场 振荡 致密天体 黑洞
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7572
Collection期刊(老文献)
Recommended Citation
GB/T 7714
彭秋和,王德焴,李宗云. 银心和星系核的磁单极模型[J]. 科学通报,1985(9):686-691.
APA 彭秋和,王德焴,李宗云.(1985).银心和星系核的磁单极模型.科学通报(9),686-691.
MLA 彭秋和,王德焴,李宗云."银心和星系核的磁单极模型".科学通报 .9(1985):686-691.
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