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

Abstract
HTML
Reference
Related

PDF

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

[1]

. 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

[1]	Yubo Ma , Songtao Zheng , Jing Li . Universal thermodynamic relations with constant corrections for five-dimensional de Sitter spacetime. Chinese Physics C, 2025, 49(4): 1-9.
[2]	Wenxi Zhai , Xiangdong Zhang . Gauss-Bonnet solution with a cloud of strings in de Sitter and anti-de Sitter space. Chinese Physics C, 2024, 48(1): 015101. doi: 10.1088/1674-1137/ad010d
[3]	Ata Sojasi , Ebrahim Yusofi , Majid Mohsenzadeh . Asymptotic-de sitter inflation in the light of the planck data. Chinese Physics C, 2018, 42(11): 115102. doi: 10.1088/1674-1137/42/11/115102
[4]	Hong Ma , Jin Li . Gravitational quasinormal modes of static Einstein-Gauss-Bonnet anti-de Sitter black holes. Chinese Physics C, 2018, 42(4): 045101. doi: 10.1088/1674-1137/42/4/045101
[5]	S. Parsamehr . Gaupta-Bleuler triplet for massless spin-3/2 field in de Sitter space. Chinese Physics C, 2017, 41(9): 093106. doi: 10.1088/1674-1137/41/9/093106
[6]	M. Mohsenzadeh , E. Yusofi . Higher order corrections to asymptotic-de Sitter inflation. Chinese Physics C, 2017, 41(8): 085101. doi: 10.1088/1674-1137/41/8/085101
[7]	S. Parsamehr , M. Mohsenzadeh . Gauge theory of massless spin-(3/2) field in de Sitter space-time. Chinese Physics C, 2016, 40(11): 113102. doi: 10.1088/1674-1137/40/11/113102
[8]	ZHAO Dong , LI Ming-Hua , WANG Ping , CHANG Zhe . Inflation in de Sitter spacetime and CMB large scale anomaly. Chinese Physics C, 2015, 39(9): 095101. doi: 10.1088/1674-1137/39/9/095101
[9]	LIU Wei-Wei , LUO Zhi-Quan , YANG Juan , BIAN Gang . Quantum tunnelling of higher-dimensional Kerr-anti-de Sitter black holes beyond semi-classical approximation. Chinese Physics C, 2011, 35(1): 22-25. doi: 10.1088/1674-1137/35/1/005
[10]	YAN Mu-Lin . Evidence for special relativity with de Sitter space-time symmetry. Chinese Physics C, 2011, 35(3): 228-232. doi: 10.1088/1674-1137/35/3/004
[11]	CAO Xue-Xiang , LI Wei-Dong , Roy A , LIU Chun-Lei , MAO Ze-Pu , CHEN Shen-Jian , DENG Zi-Yan , HE Kang-Lin , HUANG Xing-Tao , HUANG Bin , HUANG Yan-Ping , JIA Lu-Kui , JI Xiao-Bin , LI Xiu-Rong , LIU Chun-Yan , LIU Huai-Min , MA Qiu-Mei , MA Xiang , QIU Jin-Fa , WANG Da-Yong , WU Ling-Hui , WU Zhi , YUAN Ye , ZHANG Xue-Yao , ZHAO Chuan , ZHANG Yao , ZOU Jia-Heng . Studies of dE/dx measurements with the BESⅢ. Chinese Physics C, 2010, 34(12): 1852-1859.
[12]	QIN Hu , DONG Liao-Yuan , SHEN Xiao-Yan , JIN Shan , LUO Cheng-Lin . Weight of dE/dx and TOF in Particle Identification. Chinese Physics C, 2004, 28(7): 738-743.
[13]	Rong Gang , Ma Jimao , Mao Huishun , Bai JingZhi , Xie Peipei , Yan Jie , Wang Yunyong , Mao Zepu , Liu Rongguang , Sun Shijun , Li Weiguo , Song Xiaofei , Wu Zhendong . Study of Particle Identification Using dE/dx in the BES Large Cylindrical Drift Chamber. Chinese Physics C, 1996, 20(7): 577-587.
[14]	RONG Gang , CA Ji-Mao , MAO Hu-Shun , WANG Tai-Jie , BAI Jing-Zhi , LI Wei-Guo . Application of dE/dx Method for e/π Identification to the Measurement of the Mass of τ Heavy Lepton by BES. Chinese Physics C, 1993, 17(10): 865-872.
[15]	WANG En-Ke , LI Jia-Rong , LIU Lian-Shou . CHANGE OF VACUUM STRUCTURE AND DECONFINEMENT TRANSITION IN THE SOLITON BAG MODEL. Chinese Physics C, 1990, 14(5): 407-415.
[16]	MAO Hui-Shun . ESTIMATION OF ENERGY LOSS dE/dX AT MAIN DRIFT CHAMBEROF BEIJING SPECTROMETER. Chinese Physics C, 1986, 10(6): 752-756.
[17]	LIU HAN-ZHAO . FINESTRUCTURES OF INCLUSIVE SPECTRA (Ⅱ)——CALCULATED PRELIMINARILY USING MODELS,AND TO BE DETERMINED USING EXISTING DATA. Chinese Physics C, 1979, 3(2): 131-140.
[18]	LIU HAN-ZHAO . FINE STRUCTURES OF INCLUSIVE SPECTRA(Ⅰ)——SUM RULES AND THE GENERALIZATION OF FEYNMAN-YANG SCALING. Chinese Physics C, 1979, 3(1): 19-26.
[19]	YU YOU-WEN , TZU HSI-CHUEN , WU WEI-FANG . FINE STRUCTURE OF THE GIANT DIPOLE RESONACE IN ¹⁶O. Chinese Physics C, 1978, 2(3): 280-284.
[20]	FU TE-CHI , FANG PAO . THE FINE STRUCTURE OF ²⁰⁸Pb 1⁺ STATES. Chinese Physics C, 1978, 2(3): 263-266.

Access

Get Citation

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(1640)
PDF Downloads(870)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
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.

HTML

Reference (1)

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

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article