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

CHEN Shao-Xia; XIAO Neng-Chao; YAN Mu-Lin

doi:10.1088/1674-1137/32/8/004

Chinese Physics C> 2008, Vol. 32> Issue(8) : 612-616 DOI: 10.1088/1674-1137/32/8/004

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

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Abstract：
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 (SR_c,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 SR_c,R which is about ~2√5×10¹¹l.y.

References

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CHEN Shao-Xia, XIAO Neng-Chao and YAN Mu-Lin. Variation of the fine-structure constant from the de Sitter invariant special relativity[J]. Chinese Physics C, 2008, 32(8): 612-616. doi: 10.1088/1674-1137/32/8/004

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Received: 2007-10-09
Revised: 2007-11-04

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沈阳化工大学材料科学与工程学院沈阳 110142

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

Corresponding author: YAN Mu-Lin,

Received Date: 2007-10-09

Accepted Date: 2007-11-04

Available Online: 2008-08-05

Abstract:

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 (SR_c,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 SR_c,R which is about ~2√5×10¹¹l.y.

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

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