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.

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. Murphy M T, Webb J K, Flambaum V V. astro-ph/06124072. Murphy M T, Flambaum V V, Webb J K, Dzuba V V,Prochaska J X, Wolfe A M. Lec. Notes in Phys., 2004, 648:1313. Murphy M T, Webb J K, Flambaum V V. Mon. Not. Roy.Astron. Soc., 2003, 345: 6094. Murphy M T, Webb J K, Flambaum V V, Prochaska J X,Wolfe A M. Month. Not. R. Astron. Soc., 2001, 327: 12375. Murphy M T, Webb J K, Flambaum V V, Churchill C W,Prochaska J X. Month. Not. R. Astron. Soc., 2001, 327:12086. Webb J K, Murphy M T, Flambaum V V, Dzuba V A,Barrow J D, Churchill C W, Pochaska J X, Wolfe A M.Phys. Rev. Lett., 2001, 87: 0913017. Webb J K, Flambaum V V, Churchill C W, Drinkwater M J, Barrow J D. Phys. Rev. Lett., 1999, 82: 8848. Lee S. astro-ph/07020639. Flambaum V V, Shuryak E V. physics/070122010. Khatri R, Wandelt B D. astro-ph/070175211. Dirac P A M. Nature, 1937, 139: 32312. Dirac P A M. Proc. Roy. Soc. London A, 1938, 165: 19813. Dirac P A M. Proc. Roy. Soc. London A, 1974, 338: 43914. Dirac P A M. Proc. Roy. Soc. London A, 1979, 365: 1915. Uzan J P. Rev. Mod. Phys., 2003, 75: 40316. PENG H W. Commu. Theor. Phys., 2004, 42: 703; 2005,43: 8117. Hagiwara K et al. Phys. Rev. D, 2002, 66: 01000118. Shlyakhter A I. Nature, 1976, 264: 34019. Irvine J M. Phil. Trans. R. Soc. A, 1983, 310: 23920. Damour T, Dyson F J. Nuc. Phys. B, 1996, 480: 3721. Fujii Y, Iwamoto A, Fukahori T, Ohnuki T, Nakagawa M,Hidaka H, Oura Y, Moller P. Nuc. Phys. B, 2000, 573: 37722. Olive K, Pospelov M, QIAN Y Z, Coc A, Cassé M,Vangioni-Flam E. Phys. Rev. D, 2002, 66: 04502223. Petrov Y V, Nazarov A I, Onegin M S, Petrov V Y,Sakhnovsky E G. Phys. Rev. C, 2006, 74: 06461024. Riess A G et al. Astron. J., 1998, 116: 100925. Perlmutter S et al. Astrophys. J., 1999, 517: 56526. de Bernardis P et al. Nature, 2000, 404: 95527. GUO H Y, ZHOU B, TIAN Y, XU Z. Phys. Rev. D, 2007,75: 02600628. GUO H Y, HUANG C G, XU Z, ZHOU B. Mod. Phys.Lett. A, 2004, 19: 170129. GUO H Y, HUANG C G, XU Z, ZHOU B. Phys. Lett. A,2004, 331: 130. LU Q K, ZOU Z L, GUO H Y. Acta Phys. Sin., 1974, 23:225. (in Chinese)31. YAN M L, XIAO N C, HUANG W, LI S. hep-th/0512319,Commu. Theor. Phys., 2007, 48: 2732. HUANG C G. Private communication

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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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