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研究生: 羅令崴
Luo, Ling-Wei
論文名稱: 替代的引力理論與其宇宙學中的應用
Alternative Gravitational Theories and Their Cosmological Applications
指導教授: 耿朝強
Geng, Chao-Qiang
口試委員: 張維甫
Chang, We-Fu
何小剛
He, Xiao-Gang
倪維斗
Ni, Wei-Tou
高文芳
Kao, Win-Fun
學位類別: 博士
Doctor
系所名稱: 理學院 - 物理學系
Department of Physics
論文出版年: 2014
畢業學年度: 102
語文別: 英文
論文頁數: 68
中文關鍵詞: 引力理論規範理論宇宙學替代引力理論暗能量撓率絕對平行引力f(T) 理論大尺度磁場額外空間膜理論Kaluza-Klein 理論
外文關鍵詞: gravitational theory, gauge theory, cosmology, alternative gravitational theories, dark energy, torsion, teleparallel gravity, f(T) theories, large-scale magnetic fields, extra dimension, braneworld theory, Kaluza-Klein theory
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  • We study the cosmological evolutions of the equation of state for dark energy $w_{\mathrm{DE}}$ in the exponential and logarithmic as well as their combination $f(T)$ theories. We show that the crossing of the phantom divide line of $w_{\mathrm{DE}} = -1$ can be realized in the combined $f(T)$ theory even though it cannot be in the pure exponential or logarithmic $f(T)$ theory. In particular, the crossing is from $w_{\mathrm{DE}} > -1$ to $w_{\mathrm{DE}} < -1$, in the opposite manner from $f(R)$ gravity models. We also demonstrate that this feature is favored by the recent observational data.

    We explore the generation of large-scale magnetic fields from inflation in teleparallelism, in which the gravitational theory is described by the torsion scalar instead of the scalar curvature in general relativity. In particular, we examine the case that the conformal invariance of the electromagnetic field during inflation is broken by a non-minimal gravitational coupling between the torsion scalar and the electromagnetic field. It is shown that for a power-law type coupling, the magnetic field on 1~Mpc scale with its strength of $\sim 10^{-9}$~G at the present time can be generated.

    We study teleparallel gravity in five-dimensional spacetime with particular discussions on Kaluza-Klein (KK) and braneworld theories. We directly perform the dimensional reduction by differential forms. In the braneworld theory, the teleparallel gravity formalism in the Friedmann-Lema\^{i}tre-Robertson-Walker cosmology is equivalent to GR due to the same Friedmann equation, whereas in the KK case the reduction of our formulation does not recover the effect as GR of 4-dimensional spacetime due to an additional coupling between the derivative of scalar field and torsion, which results in some different behavior from general relativity.


    We study the cosmological evolutions of the equation of state for dark energy $w_{\mathrm{DE}}$ in the exponential and logarithmic as well as their combination $f(T)$ theories. We show that the crossing of the phantom divide line of $w_{\mathrm{DE}} = -1$ can be realized in the combined $f(T)$ theory even though it cannot be in the pure exponential or logarithmic $f(T)$ theory. In particular, the crossing is from $w_{\mathrm{DE}} > -1$ to $w_{\mathrm{DE}} < -1$, in the opposite manner from $f(R)$ gravity models. We also demonstrate that this feature is favored by the recent observational data.

    We explore the generation of large-scale magnetic fields from inflation in teleparallelism, in which the gravitational theory is described by the torsion scalar instead of the scalar curvature in general relativity. In particular, we examine the case that the conformal invariance of the electromagnetic field during inflation is broken by a non-minimal gravitational coupling between the torsion scalar and the electromagnetic field. It is shown that for a power-law type coupling, the magnetic field on 1~Mpc scale with its strength of $\sim 10^{-9}$~G at the present time can be generated.

    We study teleparallel gravity in five-dimensional spacetime with particular discussions on Kaluza-Klein (KK) and braneworld theories. We directly perform the dimensional reduction by differential forms. In the braneworld theory, the teleparallel gravity formalism in the Friedmann-Lema\^{i}tre-Robertson-Walker cosmology is equivalent to GR due to the same Friedmann equation, whereas in the KK case the reduction of our formulation does not recover the effect as GR of 4-dimensional spacetime due to an additional coupling between the derivative of scalar field and torsion, which results in some different behavior from general relativity.

    Contents Abstract v Acknowledgments vii Contents ix List of Figures xi List of Tables xiii 1 Introduction 1 2 f(T)Gravity 7 2.1 Formulation................................ 7 2.2 Cosmologicalevolution.......................... 10 2.2.1 Exponentialf(T)theory..................... 11 2.2.2 Logarithmicf(T)theory..................... 17 2.3 Realizingthecrossingofthephantomdivide. . . . . . . . . . . . . . . 19 2.4 Observational constraints on the combined f (T ) theory . . . . . . . . . 23 3 Large-Scale Magnetic Field 27 3.1 Teleparallelism .............................. 27 3.2 Non-minimalI(T)-Maxwelltheory ................... 28 3.2.1 Modeloftheelectromagneticsector . . . . . . . . . . . . . . . 28 3.2.2 Quantization ........................... 30 3.2.3 Proceduretoobtainanalyticsolutions . . . . . . . . . . . . . . 32 3.3 Large-scale magnetic field generated in Teleparallelism . . . . . . . . . 34 3.3.1 Currentstrengthofthemagneticfield . . . . . . . . . . . . . . 34 3.3.2 Estimation of the current strength of the large-scale magnetic field ............................... 36 4 Five Dimensional Theories in Teleparallism 39 4.1 Teleparallel Gravity in Five-Dimensional Spacetime . . . . . . . . . . . 39 4.2 Effective Gravitational Action on the Hypersurface M . . . . . . . . . 43 4.2.1 BraneworldScenario....................... 44 4.2.2 Kaluza-KleinTheory....................... 45 4.3 Friemann Equation of Braneworld Scenario in TEGR . . . . . . . . . . 46 4.3.1 FLRWBraneUniverse...................... 46 4.3.2 EquationsofMotion ....................... 47 5 Conclusion 51 Bibliography 55 Appendix 63 A Analysis Method for the Observational Data 63 A.1 TypeIaSupernovae(SNeIa)....................... 63 A.2 BaryonAcousticOscillations(BAO)................... 65 A.3 Cosmic Microwave Background (CMB) radiation . . . . . . . . . . . . 67

    Bibliography
    [1] S. Perlmutter et al. [SNCP Collaboration], Astrophys. J. 517, 565 (1999) [arXiv:astro-ph/9812133]; A. G. Riess et al. [Supernova Search Team Collabo- ration], Astron. J. 116, 1009 (1998) [arXiv:astro-ph/9805201].
    [2] M. Tegmark et al. [SDSS Collaboration], Phys. Rev. D 69, 103501 (2004) [arXiv:astro-ph/0310723]; U. Seljak et al. [SDSS Collaboration], Phys. Rev. D 71, 103515 (2005) [arXiv:astro-ph/0407372].
    [3] D. J. Eisenstein et al. [SDSS Collaboration], Astrophys. J. 633, 560 (2005) [arXiv:astro-ph/0501171].
    [4] D. N. Spergel et al. [WMAP Collaboration], Astrophys. J. Suppl. 148, 175 (2003) [arXiv:astro-ph/0302209]; Astrophys. J. Suppl. 170, 377 (2007) [arXiv:astro-ph/ 0603449].
    [5] E. Komatsu et al. [WMAP Collaboration], Astrophys. J. Suppl. 180, 330 (2009) [arXiv:0803.0547 [astro-ph]].
    [6] E. Komatsu et al. [WMAP Collaboration], Astrophys. J. Suppl. 192, 18 (2011) [arXiv:1001.4538 [astro-ph.CO]].
    [7] B. Jain and A. Taylor, Phys. Rev. Lett. 91, 141302 (2003) [arXiv:astro-ph/ 0306046].
    [8] E. J. Copeland, M. Sami and S. Tsujikawa, Int. J. Mod. Phys. D 15, 1753 (2006) [arXiv:hep-th/0603057].
    [9] R. R. Caldwell and M. Kamionkowski, Ann. Rev. Nucl. Part. Sci. 59, 397 (2009) [arXiv:0903.0866 [astro-ph.CO]].
    [10] L.AmendolaandS.Tsujikawa,DarkEnergy(CambridgeUniversitypress,2010).
    [11] S. Tsujikawa, arXiv:1004.1493 [astro-ph.CO].
    [12] M. Li, X. D. Li, S. Wang and Y. Wang, Commun. Theor. Phys. 56, 525 (2011) [arXiv:1103.5870 [astro-ph.CO]].
    [13] M. Kunz, arXiv:1204.5482 [astro-ph.CO].
    [14] K. Bamba, S. Capozziello, S. Nojiri and S. D. Odintsov, arXiv:1205.3421 [gr-qc].
    [15] S. Nojiri and S. D. Odintsov, Phys. Rept. 505, 59 (2011) [arXiv:1011.0544 [gr- qc]]; eConf C0602061, 06 (2006) [Int. J. Geom. Meth. Mod. Phys. 4, 115 (2007)] [arXiv:hep-th/0601213].
    [16] T. P. Sotiriou and V. Faraoni, Rev. Mod. Phys. 82, 451 (2010) [arXiv:0805.1726 [gr-qc]].
    [17] A. De Felice and S. Tsujikawa, Living Rev. Rel. 13, 3 (2010) [arXiv:1002.4928 [gr-qc]].
    [18] S. Capozziello and V. Faraoni, Beyond Einstein Gravity (Springer, 2010).
    [19] S. Tsujikawa, Lect. Notes Phys. 800, 99 (2010) [arXiv:1101.0191 [gr-qc]].
    [20] T. Clifton, P. G. Ferreira, A. Padilla and C. Skordis, Phys. Rept. 513, 1 (2012) [arXiv:1106.2476 [astro-ph.CO]].
    [21] S.CapozzielloandM.DeLaurentis,Phys.Rept.509,167(2011)[arXiv:1108.6266 [gr-qc]].
    [22] T. Harko and F. S. N. Lobo, arXiv:1205.3284 [gr-qc].
    [23] S. Capozziello, M. De Laurentis and S. D. Odintsov, arXiv:1206.4842 [gr-qc].
    [24] F. W. Hehl, P. Von Der Heyde, G. D. Kerlick and J. M. Nester, Rev. Mod. Phys. 48, 393 (1976).
    [25] K.HayashiandT.Shirafuji,Phys.Rev.D19,3524(1979)[Addendum-ibid.D24, 3312 (1982)].
    [26] E. E. Flanagan and E. Rosenthal, Phys. Rev. D 75, 124016 (2007).
    [27] J. Garecki, arXiv:1010.2654 [gr-qc].
    [28] A. Einstein, Sitzungsber. Preuss. Akad. Wiss. Phys. Math. Kl., 217 (1928); 401 (1930); A. Einstein, Math. Ann. 102, 685 (1930).
    [29] G. R. Bengochea and R. Ferraro, Phys. Rev. D 79, 124019 (2009).
    [30] E.V.Linder,Phys.Rev.D81,127301(2010)[Erratum-ibid.D82,109902(2010)].
    [31] R.FerraroandF.Fiorini,Phys.Rev.D75,084031(2007);ibid.78,124019(2008).
    [32] P. Wu and H. W. Yu, Phys. Lett. B 693, 415 (2010); R. Myrzakulov, arXiv: 1006.1120 [gr-qc]; K. K. Yerzhanov, S. R. Myrzakul, I. I. Kulnazarov and R. Myrzakulov, arXiv:1006.3879 [gr-qc]; P. Wu and H. Yu, Phys. Lett. B 692, 176 (2010); R. J. Yang, arXiv:1007.3571 [gr-qc]; P. Y. Tsyba, I. I. Kulnazarov, K. K. Yerzhanov and R. Myrzakulov, arXiv:1008.0779 [astro-ph.CO]; G. R. Ben- gochea, arXiv:1008.3188 [astro-ph.CO]; R. Myrzakulov, arXiv:1008.4486 [astro- ph.CO]; K. Karami and A. Abdolmaleki, arXiv:1009.2459 [gr-qc]; arXiv: 1009.3587 [physics.gen-ph]; R. J. Yang, arXiv:1010.1376 [gr-qc]; R. Zheng and Q. G. Huang, arXiv:1010.3512 [gr-qc].
    [33] S. H. Chen, J. B. Dent, S. Dutta and E. N. Saridakis, arXiv:1008.1250 [astro-
    ph.CO].
    [34] P. Wu and H. Yu, arXiv:1008.3669 [gr-qc].
    [35] K. Bamba, C. Q. Geng and C. C. Lee, arXiv:1008.4036 [astro-ph.CO]; see also C. Q. Geng, talk presented at the 2nd Chuang-Xin group meeting on “Dark Energy and Dark Matter” , Weihai, China, July 19–Aug. 3, 2010.
    [36] B.Li,T.P.SotiriouandJ.D.Barrow,arXiv:1010.1041[gr-qc];T.P.Sotiriou,B.Li and J. D. Barrow, arXiv:1012.4039 [gr-qc].
    [37] J. B. Dent, S. Dutta and E. N. Saridakis, arXiv:1010.2215 [astro-ph.CO].
    [38] C. Q. Geng, C. C. Lee, E. N. Saridakis and Y. P. Wu, Phys. Lett. B704, 384 (2011) [arXiv:1109.1092 [hep-th]]; C. Q. Geng, C. C. Lee and E. N. Saridakis, JCAP 1201, 002 (2012) [arXiv:1110.0913 [astro-ph.CO]]; H. Wei, Phys. Lett. B 712, 430 (2012) [arXiv:1109.6107 [gr-qc]]. C. Xu, E. N. Saridakis and G. Leon, JCAP 1207, 005 (2012) [arXiv:1202.3781 [gr-qc]]. J. A. Gu, C. C. Lee and C. Q. Geng, arXiv:1204.4048 [astro-ph.CO].
    [39] W. Hu and I. Sawicki, Phys. Rev. D 76, 064004 (2007).
    [40] U. Alam, V. Sahni and A. A. Starobinsky, JCAP 0406, 008 (2004); 0702, 011 (2007); S. Nesseris and L. Perivolaropoulos, ibid. 0701, 018 (2007); P. U. Wu and H. W. Yu, Phys. Lett. B 643, 315 (2006); H. K. Jassal, J. S. Bagla and T. Padman- abhan, Mon. Not. Roy. Astron. Soc. 405, 2639 (2010).
    [41] P. Zhang, Phys. Rev. D 73, 123504 (2006); B. Li and M. C. Chu, ibid. 74, 104010 (2006); R. Bean, D. Bernat, L. Pogosian, A. Silvestri and M. Trodden, ibid. 75, 064020 (2007); P. J. Zhang, ibid. 76, 024007 (2007); P. Zhang, M. Liguori, R. Bean and S. Dodelson, Phys. Rev. Lett. 99, 141302 (2007); S. Tsujikawa, Phys. Rev. D 77, 023507 (2008); G. Cognola, E. Elizalde, S. Nojiri, S. D. Odintsov, L. Sebastiani and S. Zerbini, ibid. 77, 046009 (2008); E. V. Linder, ibid. 80, 123528 (2009); G. Calcagni and G. Nardelli, arXiv:1004.5144 [hep-th].
    [42] K. Bamba, C. Q. Geng and C. C. Lee, JCAP 1008, 021 (2010) [arXiv:1005.4574 [astro-ph.CO]]; ibid. 1011, 001 (2010) [arXiv:1007.0482 [astro-ph.CO]].
    [43] L. Yang, C. C. Lee, L. W. Luo and C. Q. Geng, Phys. Rev. D 82, 103515 (2010) arXiv:1010.2058 [astro-ph.CO].
    [44] P. P. Kronberg, Rept. Prog. Phys. 57, 325 (1994); D. Grasso and H. R. Rubin- stein, Phys. Rept. 348, 163 (2001) [arXiv:astro-ph/0009061]; C. L. Carilli and G. B. Taylor, Ann. Rev. Astron. Astrophys. 40, 319 (2002) [astro-ph/0110655]; L. M. Widrow, Rev. Mod. Phys. 74, 775 (2002) [arXiv:astro-ph/0207240]; M. Gio- vannini, Int. J. Mod. Phys. D 13, 391 (2004) [arXiv:astro-ph/0312614]; Int. J. Mod. Phys. D 14, 363 (2005) [astro-ph/0412601]; Lect. Notes Phys. 737, 863 (2008) [arXiv:astro-ph/0612378]; A. Kandus, K. E. Kunze and C. G. Tsagas, Phys. Rept. 505, 1 (2011) [arXiv:1007.3891 [astro-ph.CO]].
    [45] L. Biermann and A. Schlüter, Phys. Rev. 82, 863 (1951).
    [46] E. S. Weibel, Phys. Rev. Lett. 2, 83 (1959).
    [47] J. M. Quashnock, A. Loeb, and D. N. Spergel, Astrophys. J. 344, L49 (1989); G. Baym, D. Bodeker and L. D. McLerran, Phys. Rev. D 53, 662 (1996) [arXiv:hep-ph/9507429]; D. Boyanovsky, H. J. de Vega and M. Simionato, Phys. Rev. D 67, 123505 (2003) [arXiv:hep-ph/0211022]; D. Boyanovsky, M. Simion- ato and H. J. de Vega, Phys. Rev. D 67, 023502 (2003) [arXiv:hep-ph/0208272]; R. Durrer and C. Caprini, JCAP 0311, 010 (2003) [arXiv:astro-ph/0305059]; T. Kahniashvili, A. G. Tevzadze and B. Ratra, Astrophys. J. 726, 78 (2011) [arXiv: 0907.0197 [astro-ph.CO]].
    [48] Z. Berezhiani and A. D. Dolgov, Astropart. Phys. 21, 59 (2004) [arXiv:astro-ph/ 0305595]; S. Matarrese, S. Mollerach, A. Notari and A. Riotto, Phys. Rev. D 71, 043502 (2005) [arXiv:astro-ph/0410687]; K. Takahashi, K. Ichiki, H. Ohno and H. Hanayama, Phys. Rev. Lett. 95, 121301 (2005) [arXiv:astro-ph/0502283]; K. Ichiki, K. Takahashi, H. Ohno, H. Hanayama, and N. Sugiyama, Science 311, 827 (2006); E. R. Siegel and J. N. Fry, Astrophys. J. 651, 627 (2006) [arXiv:astro-ph/0604526]; T. Kobayashi, R. Maartens, T. Shiromizu and K. Taka- hashi, Phys. Rev. D 75, 103501 (2007) [arXiv:astro-ph/0701596]; K. E. Kunze, Phys. Rev. D 77, 023530 (2008) [arXiv:0710.2435 [astro-ph]]; L. Campanelli, P. Cea, G. L. Fogli and L. Tedesco, Phys. Rev. D 77, 043001 (2008) [arXiv: 0710.2993 [astro-ph]]; S. Maeda, S. Kitagawa, T. Kobayashi and T. Shiromizu, Class. Quant. Grav. 26, 135014 (2009) [arXiv:0805.0169 [astro-ph]]; E. Fenu, C. Pitrou and R. Maartens, Mon. Not. Roy. Astron. Soc. 414, 2354 (2011) [arXiv: 1012.2958 [astro-ph.CO]].
    [49] E.N.Parker,Astrophys.J.163,255(1971);CosmicalMagneticFields(Clarendon, Oxford, England, 1979); Ya. B. Zel’dovich, A. A. Ruzmaikin, and D. D. Sokoloff, Magnetic Fields in Astrophysics (Gordon and Breach, New York, 1983).
    [50] M. S. Turner and L. M. Widrow, Phys. Rev. D 37, 2743 (1988).
    [51] I. T. Drummond and S. J. Hathrell, Phys. Rev. D 22, 343 (1980).
    [52] F. D. Mazzitelli and F. M. Spedalieri, Phys. Rev. D 52, 6694 (1995) [astro-ph/ 9505140]; G. Lambiase and A. R. Prasanna, Phys. Rev. D 70, 063502 (2004) [gr-qc/0407071]; K. Bamba and S. D. Odintsov, JCAP 0804, 024 (2008) [arXiv: 0801.0954 [astro-ph]]; K. Bamba, S. Nojiri and S. D. Odintsov, Phys. Rev. D 77, 123532 (2008) [arXiv:0803.3384 [hep-th]]; K. Bamba and S. Nojiri, arXiv: 0811.0150 [hep-th]; L. Campanelli, P. Cea, G. L. Fogli and L. Tedesco, Phys. Rev. D 77, 123002 (2008) [arXiv:0802.2630 [astro-ph]]; G. Lambiase, S. Mohanty and G. Scarpetta, JCAP 0807, 019 (2008); K. E. Kunze, Phys. Rev. D 81, 043526 (2010) [arXiv:0911.1101 [astro-ph.CO]]; J. B. Jimenez and A. L. Maroto, JCAP 1012, 025 (2010) [arXiv:1010.4513 [astro-ph.CO]].
    [53] L. Parker, Phys. Rev. Lett. 21, 562 (1968).
    [54] C. G. Tsagas, Class. Quant. Grav. 22, 393 (2005) [arXiv:gr-qc/ 0407080]; C. G. Tsagas and A. Kandus, Phys. Rev. D 71, 123506 (2005) [arXiv:astro- ph/0504089]; J. D. Barrow and C. G. Tsagas, Phys. Rev. D 77, 107302 (2008) [Erratum-ibid. D 77, 109904 (2008)] [arXiv:0803.0660 [astro-ph]]; Mon. Not.
    Roy. Astron. Soc. 414, 512 (2011) [arXiv:1101.2390 [astro-ph.CO]].
    [55] A. L. Maroto, Phys. Rev. D 64, 083006 (2001) [arXiv:hep-ph/0008288].
    [56] V. Demozzi, V. Mukhanov and H. Rubinstein, JCAP 0908, 025 (2009) [arXiv: 0907.1030 [astro-ph.CO]]; S. Kanno, J. Soda and M. a. Watanabe, JCAP 0912, 009 (2009) [arXiv:0908.3509 [astro-ph.CO]].
    [57] T. Fujita and S. Mukohyama, arXiv:1205.5031 [astro-ph.CO].
    [58] T. Suyama and J. Yokoyama, arXiv:1204.3976 [astro-ph.CO].
    [59] B. Ratra, Astrophys. J. 391, L1 (1992).
    [60] D. Lemoine and M. Lemoine, Phys. Rev. D 52, 1955 (1995);
    [61] M. Gasperini, M. Giovannini and G. Veneziano, Phys. Rev. Lett. 75, 3796 (1995) [arXiv:hep-th/9504083].
    [62] K. Bamba and J. Yokoyama, Phys. Rev. D 69, 043507 (2004) [astro-ph/0310824]; Phys. Rev. D 70, 083508 (2004) [hep-ph/0409237].
    [63] J.MartinandJ.Yokoyama,JCAP0801,025(2008)[arXiv:0711.4307[astro-ph]].
    [64] K. Bamba and M. Sasaki, JCAP 0702, 030 (2007) [astro-ph/0611701]; K. Bamba,
    JCAP 0710, 015 (2007) [arXiv:0710.1906 [astro-ph]].
    [65] K. Bamba, N. Ohta and S. Tsujikawa, Phys. Rev. D 78, 043524 (2008) [arXiv:
    0805.3862 [astro-ph]].
    [66] K. Bamba, C. Q. Geng and S. H. Ho, JCAP 0811, 013 (2008) [arXiv:0806.1856 [astro-ph]].
    [67] K. Bamba, C. Q. Geng, S. H. Ho and W. F. Kao, Eur. Phys. J. C 72, 1978 (2012) [arXiv:1108.0151 [astro-ph.CO]]; S. H. Ho, W. F. Kao, K. Bamba and C. Q. Geng, arXiv:1008.0486 [hep-ph].
    [68] M. Giovannini, Phys. Rev. D 64, 061301 (2001) [astro-ph/0104290].
    [69] M. Giovannini, Phys. Lett. B 659, 661 (2008) [arXiv:0711.3273 [astro-ph]].
    [70] M. Giovannini, JCAP 1004, 003 (2010) [arXiv:0911.0896 [astro-ph.CO]].
    [71] T. Kaluza, Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys. ) 1921, 966 (1921).
    [72] O. Klein, Z. Phys. 37, 895 (1926) [Surveys High Energ. Phys. 5, 241 (1986)].
    [73] J. M. Overduin and P. S. Wesson, Phys. Rept. 283, 303 (1997).
    [74] N.Arkani-Hamed,S.DimopoulosandG.R.Dvali,Phys.Lett.B429,263(1998); N. Arkani-Hamed, S. Dimopoulos and G. R. Dvali, Phys. Rev. D 59, 086004 (1999)
    [75] P. Horava and E. Witten, Nucl. Phys. B 460, 506 (1996).
    [76] L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 3370 (1999); L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 4690 (1999).
    [77] Y. S. Song, W. Hu and I. Sawicki, Phys. Rev. D 75, 044004 (2007).
    [78] P. K. S. Dunsby, E. Elizalde, R. Goswami, S. Odintsov and D. S. Gomez, Phys.
    Rev. D 82, 023519 (2010).
    [79] B. Li, J. D. Barrow and D. F. Mota, Phys. Rev. D 76, 044027 (2007).
    [80] R. Amanullah et al., Astrophys. J. 716, 712 (2010).
    [81] W. J. Percival et al., Mon. Not. Roy. Astron. Soc. 401, 2148 (2010).
    [82] E. W. Kolb and M. S. Turner, The Early Universe (Addison-Wesley, Redwood City, California, 1990).
    [83] W. L. Freedman et al. [HST Collaboration], Astrophys. J. 553, 47 (2001) [arXiv:astro-ph/0012376].
    [84] A.G.Riessetal.,Astrophys.J.699,539(2009)[arXiv:0905.0695[astro-ph.CO]].
    [85] V. A. Rubakov, M. V. Sazhin and A. V. Veryaskin, Phys. Lett. B 115, 189 (1982);
    L. F. Abbott and M. B. Wise, Nucl. Phys. B 244, 541 (1984).
    [86] V. C. de Andrade, L. C. T. Guillen and J. G. Pereira, Phys. Rev. D 61, 084031
    (2000).
    [87] A. L. Barbosa, L. C. T. Guillen and J. G. Pereira, Phys. Rev. D 66, 064028 (2002).
    [88] F. Fiorini, P. A. Gonzalez and Y. Vasquez, arXiv:1304.1912 [gr-qc].
    [89] K. Bamba, S. ’i. Nojiri and S. D. Odintsov, Phys. Lett. B 725, 368 (2013).
    [90] K. Nozari, A. Behboodi and S. Akhshabi, Phys. Lett. B 723, 201 (2013).
    [91] F. Gronwald, Int. J. Mod. Phys. D 6, 263 (1997).
    [92] Y..N.ObukhovandJ.G.Pereira,Phys.Rev.D67,044016(2003);Y.N.Obukhov, Int. J. Geom. Meth. Mod. Phys. 3, 95 (2006).
    [93] T. Shiromizu, K. -i. Maeda and M. Sasaki, Phys. Rev. D 62, 024012 (2000).
    [94] P. Binetruy, C. Deffayet and D. Langlois, Nucl. Phys. B 565, 269 (2000); P. Bi-
    netruy, C. Deffayet, U. Ellwanger and D. Langlois, Phys. Lett. B 477, 285 (2000).
    [95] V. D. Gladush and R. A. Konoplya, J. Math. Phys. 40, 955 (1999).
    [96] Y.P.WuandC.Q.Geng,Phys.Rev.D86,104058(2012);JHEP1211,142(2012).
    [97] J. Ponce De Leon, Mod. Phys. Lett. A 16, 2291 (2001).
    [98] R. Maartens and K. Koyama, Living Rev. Rel. 13, 5 (2010).
    [99] K. Subramanian and J. D. Barrow, Phys. Rev. Lett. 81, 3575 (1998) [arXiv:astro- ph/9803261]; T. R. Seshadri and K. Subramanian, Phys. Rev. Lett. 87, 101301 (2001) [arXiv:astro-ph/0012056]; K. Subramanian and J. D. Barrow, Mon. Not. Roy. Astron. Soc. 335, L57 (2002) [arXiv:astro-ph/0205312]; K. Subramanian, T. R. Seshadri and J. D. Barrow, Mon. Not. Roy. Astron. Soc. 344, L31 (2003) [arXiv:astro-ph/0303014]; H. Tashiro, N. Sugiyama and R. Banerjee, Phys. Rev. D 73, 023002 (2006) [arXiv:astro-ph/0509220]; D. G. Yamazaki, K. Ichiki, T. Ka- jino and G. J. Mathews, Phys. Rev. D 77, 043005 (2008) [arXiv:0801.2572 [astro- ph]]; T. Kahniashvili, Y. Maravin and A. Kosowsky, Phys. Rev. D 80, 023009 (2009) [arXiv:0806.1876 [astro-ph]]; D. G. Yamazaki, K. Ichiki, T. Kajino and G. J. Mathews, Phys. Rev. D 81, 023008 (2010) [arXiv:1001.2012 [astro-ph.CO]]; J. R. Shaw and A. Lewis, arXiv:1006.4242 [astro-ph.CO]; P. Trivedi, K. Subra- manian and T. R. Seshadri, Phys. Rev. D 82, 123006 (2010) [arXiv:1009.2724 [astro-ph.CO]]; M. Shiraishi, D. Nitta, S. Yokoyama, K. Ichiki and K. Takahashi, Phys. Rev. D 82, 121302 (2010) [Erratum-ibid. D 83, 029901 (2011)] [Phys. Rev. D 83, 029901 (2011)] [arXiv:1009.3632 [astro-ph.CO]].
    [100] M. Giovannini and K. E. Kunze, arXiv:0804.2238 [astro-ph].
    [101] J. D. Barrow, P. G. Ferreira and J. Silk, Phys. Rev. Lett. 78, 3610 (1997).
    [102] D.G.Yamazaki,K.Ichiki,T.KajinoandG.J.Mathews,Phys.Rev.D78,123001 (2008) [arXiv:0811.2221 [astro-ph]]; Phys. Rev. D 81, 103519 (2010) [arXiv: 1005.1638 [astro-ph.CO]].
    [103] S. Wang, Phys. Rev. D 81, 023002 (2010) [arXiv:0810.5620 [astro-ph]]. [104] H. Tashiro, K. Takahashi and K. Ichiki, arXiv:1010.4407 [astro-ph.CO]. [105] K. Bamba, Phys. Rev. D 75, 083516 (2007) [arXiv:astro-ph/0703647].
    [106] D. Grasso and H. R. Rubinstein, Phys. Lett. B 379, 73 (1996) [arXiv:astro-ph/ 9602055]; B. l. Cheng, A. V. Olinto, D. N. Schramm and J. W. Truran, Phys. Rev. D 54, 4714 (1996) [arXiv:astro-ph/9606163].
    [107] C. Caprini, R. Durrer and T. Kahniashvili, Phys. Rev. D 69, 063006 (2004) [arXiv:astro-ph/0304556]; T. Kahniashvili and B. Ratra, Phys. Rev. D 71, 103006 (2005) [arXiv:astro-ph/0503709]; T. Kahniashvili, New Astron. Rev. 50, 1015 (2006) [arXiv:astro-ph/0605440]; J. R. Kristiansen and P. G. Ferreira, Phys. Rev. D 77, 123004 (2008) [arXiv:0803.3210 [astro-ph]].
    [108] See http://www.sciops.esa.int/index.php?project=PLANCK.
    [109] http:// www.rssd.esa.int/ SA/ PLANCK/ docs/ Bluebook-ESA- SCI(2005)1_V2.pdf.
    [110] See http://quiet.uchicago.edu/index.php.
    [111] D. Samtleben and f. t. Q. Collaboration, Nuovo Cim. 122B, 1353 (2007) [arXiv: 0802.2657 [astro-ph]].
    [112] See http://www.b-pol.org/index.php.
    [113] See http://cmbpol.kek.jp/litebird/.
    [114] M. Li, X. D. Li and X. Zhang, Sci. China Phys. Mech. Astron. 53, 1631 (2010) [arXiv:0912.3988 [astro-ph.CO]].
    [115] L. Perivolaropoulos, Phys. Rev. D 71, 063503 (2005); S. Nesseris and L. Perivolaropoulos, ibid. 72, 123519 (2005).
    [116] D. J. Eisenstein and W. Hu, Astrophys. J. 496, 605 (1998).
    [117] J.R.Bond,G.EfstathiouandM.Tegmark,Mon.Not.Roy.Astron.Soc.291,L33 (1997).
    [118] W. Hu and N. Sugiyama, Astrophys. J. 471, 542 (1996). [119] A. Lewis and S. Bridle, Phys. Rev. D 66, 103511 (2002).

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