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： 中國物理C(英文版)  ISTIC 英文刊名： CHINESE PHYSICS　C  年，卷(期)： 2008 32(8)  分類號： O4  關(guān)鍵詞： quasi-stellar objects   Oklo nature nuclear reactor   Dirac large number hypothesis   de Sitter invariant special relativity  

【Variation of the fine-structure cons】相關(guān)文章：

Variation Law of Organic Contaminant in Lijiang River04-26

THE CHARACTERISTICS OF THUNDERSTORM FREQUENCY VARIATION AND THEIR POSSIBLE RELATION WITH THE ADJUSTMENT OF CROP DISTRIBU04-27

The secular variation of inner zone high energy proton environment in the SAA04-26

An analysis on spatial variation of urban human thermal comfort in Hangzhou,China04-26

An Index Measuring the Interannual Variation of the East Asian Summer Monsoon--The EAP Index04-26

Variation of precipitation for the last 300 years over the middle and lower reaches of the Yellow River04-26

Variation characteristics of soil respiration fluxes in four types of grassland communities under different precipitatio04-26

THE RELATIONSHIP BETWEEN GLOBAL WARMING AND THE VARIATION IN TROPICAL CYCLONE FREQUENCY OVER THE WESTERN NORTH PACIFIC04-27