A new gravitational model for dark energy

HUANG Chao-Guang; ZHANG Hai-Qing; GUO Han-Ying

doi:10.1088/1674-1137/32/9/002

Chinese Physics C> 2008, Vol. 32> Issue(9) : 687-691 DOI: 10.1088/1674-1137/32/9/002

A new gravitational model for dark energy

Abstract
HTML
Reference
Related

PDF

Abstract：
A new gravitational model for dark energy is presented based on the model of de Sitter gauge theory of gravity. In the model, in addition to the cosmological constant, the homogeneous and isotropic torsion and its coupling with curvature play an important role for dark energy. The model may supply the universe with a natural transit from decelerating expansion to accelerating expansion.

References

[1]

. Riess A G, Fillippenko A V, Challis P et al. Astron. J.,1998, 116: 1009; Perlmutter S, Aldering G, Goldhaber G et al. Astrophys. J., 1999, 517: 565; Riess A G, FillippenkoA V, Liu M C et al. Astrophys. J., 2000, 536: 62; Riess A G, Nugent P E, Gillilangd R L et al. Astrophys. J., 2001,560: 492. WU Y S, LI G D, GUO H Y. Kexue Tongbao (Chi. Sci.Bull.), 1974, 19: 509 (in Chinese); AN Y, CHEN S, ZOUZ L et al. Kexue Tongbao (Chi. Sci. Bull.), 1974 19: 379(in Chinese); GUO H Y. Kexue Tongbao (Chi. Sci. Bull.),1976, 21: 31 (in Chinese); ZOU Z L. Sci. Sinica, 1979,XXII: 628 (in Chinese); YAN M L, ZHAO B H, GUOH Y. Kexue Tongbao (Chi. Sci. Bull.), 1979, 24: 587 (in Chinese)3. GUO H Y, HUANG C G, TIAN Y et al. Class. Quant.Grav., 2007, 24: 4009; GUO H Y, HUANG C G, TIAN Y et al. Front. Phys. China, 2007, 2: 3584. Townsend P. Phys. Rev. D, 1977, 15: 2795; Tseytsin A A.Phys. Rev. D, 1982, 26: 33275. LOOK K H, TSOU C L, KUO H Y. Acta Phy. Sin., 1974,23: 225 (in Chinese); GUO H Y. Kexue Tongbao (Chinese Sci. Bull.), 1977, 22: 487 (in Chinese)6. GUO H Y. A Theory of Inertial Motion in Space-Time of Constant Curvature. In: Ruffini R ed. Proceddings of 2nd Marcel Grossmann Meeting on GR. Amsterdam: North-Holland Press, 1982. 801; GUO H Y. Nucl. Phys. B (Proc.Suppl.), 1989, 6: 381; HUANG C G, GUO H Y. Gravita-tion and Astrophysics - On the Occasion of the 90th Year of General Relativity. In: Nester J M, CHEN C M, HSUJ P ed. Proceddings of the VII Asia-Paci c International Conference, Singapore: World Scienti c Press, 2007. 2607. GUO H Y, HUANG C G, XU Z et al. Mod. Phys. Lett. A,2004, 19: 1701; Phys. Lett. A, 2004, 331: 1; Chin. Phys.Lett., 2005, 22: 2477; GUO H Y, HUANG C G, TIAN Y et al. Acta Phys. Sin., 2005, 54: 2494 (in Chinese); GUOH Y, HUANG C G, ZHOU B. Europhys. Lett., 2005, 72:1045; Guo H Y. Phys. Lett. B, 2007, 653: 88; Scien. in China A, 2008, 51: 5888. Kibble T W B. J. Math. Phys., 1961, 2: 212; Held F W,von der Heyde P, Kerlick G D et al. Rev. Mod. Phys., 1976,48: 393 and references therein9. WU Y S, ZOU Z L, CHEN S. Kexue Tongbao (Chin. Sci.Bull.), 1973, 18: 119 (in Chinese)10. Freidel L, Starodubtsev A. Quantum Gravity in Terms of Topological Observables. arXiv: hep-th/050119111. Armenta J, Nieto J A. J. Math. Phys., 2005, 46: 11250312. Wise D K. MacDowell-Mansouri, Gravity and Cartan Ge-ometry. arXiv: gr-qc/061115413. Mahato P. Mod. Phys. Lett. A, 2002, 17: 1991-1998; Phys.Rev. D, 2004, 70: 124024; Int. J. Theor. Phys., 2005, 44:79-93; Int. J. Mod. Phys. A, 2007, 22: 83514. Leclerc M. Ann. Phys. (NY), 2006, 321: 70815. Riess A G, Strolger L G, Tonry J et al. Astropys. J., 2004,607: 66516. John M V. Astrophys. J., 2004, 614: 117. Rapetti D, Steven W A, Mustafa A A et al. Mon. Not. R.Soc., 2007, 375: 151018. Bahcall N, Fan X. Astrophys. J., 1998, 504: 1; Kashlinsky A. Phys. Rep., 1998, 307: 67; Carlberg R G, Yee H K C,Morris S L et al. Astrophys. J., 1999, 516: 55219. Bennett C L, Halpern M, Hinshaw G et al. Astrophys. J.Suppl., 2003, 148: 1; D. N. Spergel, Verde L, Peiris H Vet al. Astrophys. J. Suppl., 2003, 148: 17; Astrophys. J.Suppl., 2007, 170: 37720. Tegmark M. Phys. Rev. D, 2004,69: 10350121. Reid I N. Astron. J., 1997, 114: 161; Chaboyer B, Demar-que P, Kernan P J et al. Astrophys. J., 1998, 494: 96

[1]	Rui-Yun Guo , Jing-Fei Zhang , Xin Zhang . Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter. Chinese Physics C, 2018, 42(9): 095103. doi: 10.1088/1674-1137/42/9/095103
[2]	Peyman Zakeri , Mohammad Moosavi , Mohammadreza Zakeri , Yaser Ayazi . A minimal model for two-component FIMP dark matter: A basic search. Chinese Physics C, 2018, 42(7): 073101. doi: 10.1088/1674-1137/42/7/073101
[3]	Andrea Addazi , Pietro Donà , Antonino Marcianò . Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions. Chinese Physics C, 2018, 42(7): 075102. doi: 10.1088/1674-1137/42/7/075102
[4]	Andrea Addazi , Antonino Marcianò . Gravitational waves from dark first order phase transitions and dark photons. Chinese Physics C, 2018, 42(2): 023107. doi: 10.1088/1674-1137/42/2/023107
[5]	ZHENG Na , XU Hai-Bo . Transmission calculation by empirical numerical model and Monte Carlo simulation in high energy proton radiography of thick objects. Chinese Physics C, 2015, 39(10): 108201. doi: 10.1088/1674-1137/39/10/108201
[6]	N. Salehi , H. Hassanabadi , A. A. Rajabi . A new model for calculating the binding energy of the lithium nucleus under the generalized Yukawa potential and Hellmann potential. Chinese Physics C, 2015, 39(6): 063106. doi: 10.1088/1674-1137/39/6/063106
[7]	GUO Zhan-Ying , YANG Guang , YANG Bing-Fang . Single vector-like top partner production in the left-right twin Higgs model at TeV energy eγ colliders. Chinese Physics C, 2013, 37(10): 103101. doi: 10.1088/1674-1137/37/10/103101
[8]	LI Cheng , TIAN Jun-Long , QIN Yu-Jiao , LI Jing-Jing , WANG Ning . Determination of the nucleon-nucleon interaction in the ImQMD model by nuclear reactions at the Fermi energy region. Chinese Physics C, 2013, 37(11): 114101. doi: 10.1088/1674-1137/37/11/114101
[9]	QIAO Qing-Peng , XU Bin . Dark-matter pair production at the ILC in the littlest Higgs model with T-parity. Chinese Physics C, 2013, 37(3): 033103. doi: 10.1088/1674-1137/37/3/033103
[10]	CHANG Xue , LIU Chun , MA Feng-Cai , YANG Shuo . Supersymmetric extension of the minimal dark matter model. Chinese Physics C, 2012, 36(9): 810-817. doi: 10.1088/1674-1137/36/9/003
[11]	Jeong Ryeol . An approach to dark energy problem through linear invariants. Chinese Physics C, 2011, 35(3): 233-242. doi: 10.1088/1674-1137/35/3/005
[12]	ZHANG Lun-Dong , GUO Jian-You , FANG Xiang-Zheng . With the alpha-cluster model to explain the change of separating energy. Chinese Physics C, 2009, 33(S1): 140-141. doi: 10.1088/1674-1137/33/S1/044
[13]	GU Pei-Hong , BI Xiao-Jun , FENG Bo , YOUNG Bing-Lin , ZHANG Xin-Min . Detecting dark energy in long baseline neutrino oscillations. Chinese Physics C, 2008, 32(7): 530-535. doi: 10.1088/1674-1137/32/7/004
[14]	Huo Anxiang , Kuang Haohuai . A Model for the Enhancement of Very High Energy Particles During Large Solar Flares. Chinese Physics C, 1997, 21(S1): 411-416.
[15]	Shuanquan Luo , Cheng-Shing Wang . Thomas-Fermi Statistical Model Theory for the Surface Energy of Hot Nuclei. Chinese Physics C, 1995, 19(S2): 199-205.
[16]	Wang Qun , Liu Ximing , Xie Qubing . Behaviors of Inelasticity and Cluster Number at High Energy in Interacting Parton Model. Chinese Physics C, 1995, 19(S3): 281-288.
[17]	Cao Zhen , Ding Linkai . Generator of QCD Parton Model for the Cosmic Ray Ultrahigh Energy Interaction. Chinese Physics C, 1994, 18(S4): 321-332.
[18]	Liu Bo , Zhao Weiqin . Analysis of the New Data of Transverse Energy Distributions in High Energy p-A Collisions Based on Geometrical Model. Chinese Physics C, 1994, 18(S4): 385-390.
[19]	Zhang Zhaoxi , Li Xueqian , Yang Maozhi , Wang Jianxiong . Study on the Production of tc at LEPII Energy in the Extended Standard Model with Two Higgs-Doublets. Chinese Physics C, 1993, 17(S4): 335-345.
[20]	Qiu Zhongping , Cai Xu . Cylindrical Bag Model of Particle Production in High Energy e⁺e^- Annihilation. Chinese Physics C, 1988, 12(S4): 359-364.

Access

Get Citation

HUANG Chao-Guang, ZHANG Hai-Qing and GUO Han-Ying. A new gravitational model for dark energy[J]. Chinese Physics C, 2008, 32(9): 687-691. doi: 10.1088/1674-1137/32/9/002

HUANG Chao-Guang, ZHANG Hai-Qing and GUO Han-Ying. A new gravitational model for dark energy[J]. Chinese Physics C, 2008, 32(9): 687-691. doi: 10.1088/1674-1137/32/9/002 shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2008-04-23
Revised: 2008-04-25

Article Metric

Article Views(3904)
PDF Downloads(737)
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

A new gravitational model for dark energy

Corresponding author: ZHANG Hai-Qing,

Received Date: 2008-04-23

Accepted Date: 2008-04-25

Available Online: 2008-09-05

Abstract:

A new gravitational model for dark energy is presented based on the model of de Sitter gauge theory of gravity. In the model, in addition to the cosmological constant, the homogeneous and isotropic torsion and its coupling with curvature play an important role for dark energy. The model may supply the universe with a natural transit from decelerating expansion to accelerating expansion.

HTML

Reference (1)

A new gravitational model for dark energy

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article