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《中国物理C》(英文)编辑部
2024年10月30日

On Theoretical Models of Dark Energy

  • 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.
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  • [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]
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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
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Received: 2007-04-25
Revised: 1900-01-01
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On Theoretical Models of Dark Energy

    Corresponding author: CAI Rong-Gen,
  • Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080, China

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.

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