Variation of the fine-structure constant from the de Sitter invariant special relativity

We discuss the variation of the fine-structure constant,α.There are obvious discrepancies among the results of α-variation from recent Quasi-stellar observation experiments and from the Oklo uranium mine analysis.We use dS Sitter invariant Special Relativity (SRc,R) and Dirac large number hypothesis to discuss this puzzle,and present a possible solution to the disagreement.By means of the observational data and the discussions presented in this paper,we estimate the radius of the Universe in SRc,R which is about ～2(√5)×1011l.y.

作 者： CHEN Shao-Xia XIAO Neng-Chao YAN Mu-Lin   作者單位： Interdisciplinary Center for Theoretical Study, University of Science sad Technology of China,Hefei 230026,China  刊 名： 中國(guó)物理C(英文版)  ISTIC 英文刊名： CHINESE PHYSICS　C  年，卷(期)： 2008 32(8)  分類號(hào)： O4  關(guān)鍵詞： quasi-stellar objects   Oklo nature nuclear reactor   Dirac large number hypothesis   de Sitter invariant special relativity  

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