×
近期发现有不法分子冒充我刊与作者联系,借此进行欺诈等不法行为,请广大作者加以鉴别,如遇诈骗行为,请第一时间与我刊编辑部联系确认(《中国物理C》(英文)编辑部电话:010-88235947,010-88236950),并作报警处理。
本刊再次郑重声明:
(1)本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
(2)本刊采编系统作者中心是投稿的唯一路径,该系统为ScholarOne远程稿件采编系统,仅在本刊投稿网网址(https://mc03.manuscriptcentral.com/cpc)设有登录入口。本刊不接受其他方式的投稿,如打印稿投稿、E-mail信箱投稿等,若以此种方式接收投稿均为假冒。
(3)所有投稿均需经过严格的同行评议、编辑加工后方可发表,本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿,并收取发表费用,均为假冒。
                  
《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.
  • 加载中
  • [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]
  • 加载中

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
Milestone
Received: 2007-04-25
Revised: 1900-01-01
Article Metric

Article Views(3073)
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

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

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.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return