Large Number,Dark Matter,Dark Energy,and Superstructures in the Universe  

作　　者：HUANG Wu-Liang HUANG Xiao-Dong 

机构地区：[1]Institute of High Energy Physics, Chinese Academy of Sciences, P.O. Box 918（3）, Beijing 100049, China [2]Department of Mathematics, University of California, Los Angeles, Los Angeles, CA 90095, U.S.A.

出　　处：《Communications in Theoretical Physics》2009年第3期575-576,共2页理论物理通讯（英文版）

摘　　要：Since there may exist dark matter particles ν and δ with mass - 10^-1 e V in the universe, the superstructures with a scale of 10^19 solar masses （large number A - 10^19） appeared during the era near and before the hydrogen recombination. Since there are superstructures in the universe, there may be no necessity for the existence of dark energy. For checking the superstructure in the universe by CMB anisotropy, we need to measure CMB angular power spectrum especially around ten degrees across the sky- in more details, While neutrino u is related to electroweak unification, the fourth stable elementary particle 6 may be related to strong-gravity unification, which suggests p ＋ p^- → n ＋ δ^- and that some new baryons appeared in the TeV region.

关 键 词：large number dark matter dark energy stable elementary particle SUPERSTRUCTURE 

分 类 号：O572.31[理学—粒子物理与原子核物理] P145.9[理学—物理]