On Theoretical Models of Dark Energy

CAI Rong-Gen

Chinese Physics C> 2007, Vol. 31> Issue(9) : 827-834

On Theoretical Models of Dark Energy

CAI Rong-Gen ^,

Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080, China

Abstract
HTML
Reference
Related

PDF

Abstract：
In this talk I divide dark energy models (precisely speaking, models to explain origin of current cosmic acceleration) existing in literatures in to three classes. The first one is to ascribe the cosmic acceleration to modifications of general relativity at cosmological scales. The second one is due to the backreaction of perturbations, or say, the effect of inhomogeneity of the universe. The third one is some exotic component in the universe, which appears in the right hand side of Einstein's equations. For each class I demonstrate some examples.

References

[1]

. Peebles P J E, Ratra B. Rev. Mod. Phys., 2003, 75: 559[arXiv:astro-ph/0207347]; Padmanabhan T. Phys. Rept.,2003, 380: 235 [arXiv:hep-th/0212290]; Carroll S M. eConf2003, C0307282: TTH09 [AIP Conf. Proc. 2005, 743: 16][arXiv:astro-ph/0310342]; Sahni V, Starobinsky A A. Int.J. Mod. Phys., 2000, D9: 373 [arXiv:astro-ph/9904398];Carroll S M. Living Rev. Rel., 2001, 4: 1 [arXiv:astro-ph/0004075]; Padmanabhan T. Curr. Sci., 2005, 88: 1057[arXiv:astro-ph/0411044]; Weinberg S. Rev. Mod. Phys.,1989, 61: 1; Nobbenhuis S. Found. Phys., 2006, 36:613. [arXiv:gr-qc/0411093]; Copeland E J, Sami M, Tsu-jikawa S. Int. J. Mod. Phys., 2006, D15: 1753 [arXiv:hep-th/0603057]2. Riess A G et al. (Supernova Search Team Collaboration).Astron. J., 1998, 116: 1009 [arXiv:astro-ph/9805201];Perlmutter S et al. (Supernova Cosmology Project Col-laboration). Astrophys. J., 1999, 517: 565 [arXiv:astro-ph/9812133]3. Knop R A et al. (Supernova Cosmology Project Col-laboration). Astrophys. J., 2003, 598: 102 [arXiv:astro-ph/0309368]; Tonry J L et al. (Supernova Search TeamCollaboration). Astrophys. J., 2003, 594: 1 [arXiv:astro-ph/0305008]; Riess A G et al. (Supernova Search TeamCollaboration). Astrophys. J., 2004, 607: 665 [arXiv:astro-ph/0402512]4. Bennett C L et al. (WMAP Collaboration). Astrophys.J., 2003, 148(Suppl.): 1 [arXiv:astro-ph/0302207]; SpergelD N et al. (WMAP Collaboration). Astrophys. J., 2003,148(Suppl.): 175 [arXiv:astro-ph/0302209]5. Spergel D N et al. (WMAP Collaboration). arXiv:astro-ph/06034496. Tegmark M et al. (SDSS Collaboration). Phys. Rev., 2004,D69: 103501 [arXiv:astro-ph/0310723]; Tegmark M etal. (SDSS Collaboration). Astrophys. J., 2004, 606: 702[arXiv:astro-ph/0310725]7. Seljak U et al. (SDSS Collaboration). Phys. Rev.,2005, D71: 103515 [arXiv:astro-ph/0407372]; Adelman-McCarthy J K et al. (SDSS Collaboration). Astrophys. J.,2006, 162(Suppl.): 38 [arXiv:astro-ph/0507711]; Abaza-jian K et al. (SDSS Collaboration). Astron. J., 2005, 129:1755. [arXiv:astro-ph/0410239]; Abazajian K et al. (SDSSCollaboration). Astron. J., 2004, 128: 502 [arXiv:astro-ph/0403325]; Abazajian K et al. (SDSS Collaboration). As-tron. J., 2003, 126: 2081 [arXiv:astro-ph/0305492]8. Caldwell R R, Dave R, Steinhardt P J. Phys. Rev. Lett.,1998, 80: 1582 [arXiv:astro-ph/9708069]; Wetterich C.Nucl. Phys., 1998, B302: 668; Peebles P J E, Ratra B.Astrophys. J., 1988, 325: L17; Steinhardt P J, WANG LM, Zlatev I. Phys. Rev., 1999, D59: 123504 [arXiv:astro-ph/9812313]; Zlatev I, Steinhardt P J. Phys. Lett., 1999,B459: 570 [arXiv:astro-ph/9906481]9. Caldwell R R. Phys. Lett., 2002, B545: 23 [arXiv:astro-ph/9908168]; Caldwell R R, Kamionkowski M, WeinbergN N. Phys. Rev. Lett., 2003, 91: 071301 [arXiv:astro-ph/0302506]; Carroll S M, Ho man M, Trodden M. Phys.Rev., 2003, D68: 023509 [arXiv:astro-ph/0301273]; ClineJ M, Jeon S, Moore G D. Phys. Rev., 2004, D70: 043543[arXiv:hep-ph/0311312]10. Huterer D, Cooray A. Phys. Rev., 2005, D71: 023506[arXiv:astro-ph/0404062]; Alam U, Sahni V, StarobinskyA A. JCAP, 2004, 0406: 008 [arXiv:astro-ph/0403687];WANG Y, Tegmark M. Phys. Rev., 2005, D71: 103513[arXiv:astro-ph/0501351]; FENG B, WANG X L, ZHANGX M. Phys. Lett., 2005, B607: 35 [arXiv:astro-ph/0404224]11. Arkani-Hamed N, CHENG H C, Luty M A et al. JHEP,2004, 0405: 074 [arXiv:hep-th/0312099]12. Carroll S M, Duvvuri V, Trodden Met al. Phys. Rev., 2004,D70: 043528 [arXiv:astro-ph/0306438]; Carroll S M, DeFelice A, Duvvuri V et al. Phys. Rev., 2005, D71: 063513[arXiv:astro-ph/0410031]13. SHAO C G, CAI R G, WANG B et al. Phys. Lett., 2006,B633: 164 [arXiv:gr-qc/0511034]14. Randall L, Sundrum R. Phys. Rev. Lett., 1999, 83: 4690[arXiv:hep-th/9906064]15. Dvali G, Gabadadze G, Porrati M. Phys. Lett., 2000, B485:208. hep-th/0005016; Dvali G, Gabadadze G. Phys. Rev.,2001, D63: 065007. hep-th/000805416. Sahni V, Shtanov Y. JCAP, 2003, 0311: 014 [arXiv:astro-ph/0202346]17. CAI R G, ZHANG H S, WANG A. Commun. Theor. Phys.,2005, 44: 948 [arXiv:hep-th/0505186]18. CAI R G, GONG Y G, WANG B. JCAP, 2006, 0603: 006[arXiv:hep-th/0511301]19. Kolb E W, Matarrese S, Notari A et al. Mod. Phys. Lett.,2005, A20: 2705 [arXiv:astro-ph/0410541]20. Kolb E W, Matarrese S, Notari A et al. arXiv:hep-th/050311721. Kolb E W, Matarrese S, Riotto A. New J. Phys., 2006, 8:322. [arXiv:astro-ph/0506534]22. Wiltshire D L. arXiv:gr-qc/050309923. Gar nkle D. Class. Quant. Grav., 2006, 23: 4811 [arXiv:gr-qc/0605088]24. Cohen A G, Kaplan D B, Nelson A E. Phys. Rev. Lett.,1999, 82: 4971 [arXiv:hep-th/9803132]; Hsu S D H. Phys.Lett., 2004, B594: 13 [arXiv:hep-th/0403052]; LI M. Phys.Lett., 2004, B603: 1 [arXiv:hep-th/0403127]25. Armendariz-Picon C, Mukhanov V F, Steinhardt P J.Phys. Rev. Lett., 2000, 85: 4438 [arXiv:astro-ph/0004134];Armendariz-Picon C, Mukhanov V F, Steinhardt P J. Phys.Rev., 2001, D63: 103510 [arXiv:astro-ph/0006373]; ChibaT, Okabe T, Yamaguchi M. Phys. Rev., 2000, D62: 023511[arXiv:astro-ph/9912463]26. Kamenshchik A Y, Moschella U, Pasquier V. Phys. Lett.,2001, B511: 265 [arXiv:gr-qc/0103004]; Gorini V, Kamen-shchik A, Moschella U. Phys. Rev., 2003, D67: 063509[arXiv:astro-ph/0209395]; Bento M C, Bertolami O, Sen AA. Phys. Rev., 2002, D66: 043507 [arXiv:gr-qc/0202064]27. FENG B, WANG X L, ZHANG X M. Phys. Lett., 2005,B607: 35 [arXiv:astro-ph/0404224]28. WEI H, CAI R G, ZENG D F. Class. Quant. Grav., 2005,22: 3189 [arXiv:hep-th/0501160]; WEI H, CAI R G. Phys.Rev., 2005, D72: 123507 [arXiv:astro-ph/0509328]29. WEI H, CAI R G. Phys. Lett., 2006, B634: 9 [arXiv:astro-ph/0512018]30. Khoury J, Weltman A. Phys. Rev. Lett., 2004, 93: 171104[arXiv:astro-ph/0309300]31. WEI H, CAI R G. Phys. Rev., 2005, D71: 043504[arXiv:hep-th/0412045]32. Armendariz-Picon C. JCAP, 2004, 0407: 007 [arXiv:astro-ph/0405267]33. WEI H, CAI R G. Phys. Rev., 2006, D73: 083002[arXiv:astro-ph/0603052]

[1]	ZHANG Zheng-Jun , HAN Yin-Lu , SHEN Qing-Biao , CAI Chong-Hai . Studies on Energy Spectra of Outgoing Particles in (p,Pb),(p,Bi),(p,Hg) Reactions in Energy Range up to 250MeV. Chinese Physics C, 2007, 31(5): 464-469.
[2]	WANG Bin . Understanding the Interaction between Dark Energy and Dark Matter. Chinese Physics C, 2007, 31(9): 874-879.
[3]	GAO Zao-Cun , SUN Yang , CHEN Yong-Shou . Beta Decay Theory in the Projected Shell Model. Chinese Physics C, 2006, 30(S2): 65-67.
[4]	LI Yan-Heng . Scalar-Field Model for Dark Energy with a Fixed Background Vector Field. Chinese Physics C, 2006, 30(6): 522-525.
[5]	WANG Xiu-Lian , ZHANG Xin-Min . Dark Energy and Baryon Isocurvature Perturbation. Chinese Physics C, 2003, 27(10): 874-878.
[6]	WANG Quan-Jin , YE Yan-Lin , JIANG Dong-Xing , HUA Hui , LI Zhi-Huan , CHEN Tao , LI Xiang-Qing , GE Yu-Cheng . Influence of Energy-Modified Glauber Model on Total Reaction Cross Section at Intermediate-Energy. Chinese Physics C, 2002, 26(8): 818-822.
[7]	LU Zhong-Dao , SA Ben-Hao , Amand Faessler . Analysis of Multi-Particle Production at RHIC by Two-Source Statistical Model. Chinese Physics C, 2002, 26(11): 1166-1171.
[8]	FENG Qing-Guo , DONG Yu-Bing . Relativistic Quark Model and the N-Δ Mass Splitting. Chinese Physics C, 2002, 26(1): 21-27.
[9]	Luo Shuanqun , Wang Zhengxing . Thomas-Fermi Statistical Model Theory for the Surface Energy of Hot Nuclei. Chinese Physics C, 1995, 19(3): 278-283.
[10]	LIU Liang-Gang . ONE LOOP RENORMALIZATION OF NUCLEON ENERGY DENSITY IN NUCLEAR MATTER BY CHIRAL σ MODEL. Chinese Physics C, 1990, 14(9): 822-828.
[11]	XU Xiao-Ming , QIU Xi-Jun . A CHIRAL QUARK-SOLITON MODEL FOR NUCLEAR FORCE. Chinese Physics C, 1990, 14(9): 810-816.
[12]	MIAO Rong-Zhi , WU Guo-Hua , GE Ling-Xiao . THE PROBLFM OF INITIAL VALUE IN GENERALIZED EXCITON MODEL THEORY. Chinese Physics C, 1989, 13(3): 260-268.
[13]	CAI Xu , WU Yuan-Fang , LIU Lian-Shou . ENERGY DEPENDENCE OF MULTIPLICITY MOMENTS AND THREE FIRE BALL MODEL. Chinese Physics C, 1987, 11(4): 554-557.
[14]	CHEN Shi-Hao . ELECTRO-WEAK UNIFIED THEORY——A MODEL IN SU(3)×U(1). Chinese Physics C, 1985, 9(6): 679-686.
[15]	ZHANG Zhong-Can . STRONG-COUPLING EXPANSION IN σ-MODEL. Chinese Physics C, 1984, 8(6): 677-687.
[16]	LI Guang-Lie , K.KNg , T.T.S.Kuo . A FOLDED DIAGRAM METHOD FOR DERIVING AN ENERGY-INDEPENDENT NUCLEON-NUCLEON N-N POTENTIAL FROM MESON EXCHANGES (Ⅰ) THEORY. Chinese Physics C, 1983, 7(1): 67-75.
[17]	YIN LO , LI YANG-GUO , LIU XIAN-HUI . OPERATOR THEORY OF HADRON SCATTERING IN GEOMETRICAL MODEL. Chinese Physics C, 1981, 5(6): 653-663.
[18]	Qiu Xi-jun , Song Hong-qiu , Huang Wei-zhi , Wang Zi-xing . A MODEL OF FISSION. Chinese Physics C, 1980, 4(5): 680-682.
[19]	LI YANG-GUO , JIANG HUAN-QING . THEORY OF （π⁺,d） REACTION. Chinese Physics C, 1979, 3(5): 595-603.
[20]	ZHU WEI , LU JI-ZONG , ZHANG MIN-SHENG , YIN PENG-CHENG . A φ⁴-TYPE BAG MODEL OF HADRONS——THE “RUBBER BAG” MODEL（Ⅰ）——THEORY. Chinese Physics C, 1979, 3(1): 34-42.

Access

Get Citation

CAI Rong-Gen. On Theoretical Models of Dark Energy[J]. Chinese Physics C, 2007, 31(9): 827-834.

CAI Rong-Gen. On Theoretical Models of Dark Energy[J]. Chinese Physics C, 2007, 31(9): 827-834. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2007-04-25
Revised: 1900-01-01

Article Metric

Article Views(3135)
PDF Downloads(693)
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

On Theoretical Models of Dark Energy

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

On Theoretical Models of Dark Energy

Corresponding author: CAI Rong-Gen,

HTML

目录