• [1]

    A. H. Guth, Phys. Rev. D, 23: 347-356 (1981)

  • [2]

    A. D. Linde, Phys. Lett. B, 108: 389-393 (1982)

  • [3]

    A. Albrecht and P. J. Steinhardt, Phys. Rev. Lett., 48: 1220-1223 (1982)

  • [4]

    S. W. Hawking and I. G. Moss, Phys. Lett. B, 110: 35-38 (1982)

  • [5]

    A. D. Linde, Phys. Lett. B, 129: 177-181 (1983)

  • [6]

    V. F. Mukhanov and G. Chibisov, JETP Lett., 33: 532-535 (1981)

  • [7]

    S. W. Hawking, Phys. Lett. B, 115: 295-297 (1982)

  • [8]

    A. H. Guth and S. Y. Pi, Phys. Rev. Lett., 49: 1110-1113 (1982)

  • [9]

    Starobinsky and Alexei A., Phys. Lett. B, 91: 99-102 (1980)

  • [10]

    L. Boubekeur and D. H. Lyth, JCAP, 0507: 010 (2005)

  • [11]

    K. Freese, J. A. Frieman, and A. V. Olinto, Phys. Rev. Lett., 65: 3233 (1990)

  • [12]

    F. C. Adams, J. R. Bond, K. Freese et al., Phys. Rev. D, 47: 427 (1993)

  • [13]

    R. Kallosh and A. Linde, JCAP, 1306: 028 (2013)

  • [14]

    R. Kallosh, A. Linde, and D. Roest, JHEP, 1311: 198 (2013)

  • [15]

    A. R. Liddle and D. H. Lyth, Phys. Lett. B, 291: 391-398 (1992)

  • [16]

    A. R. Liddle, P. Parsons, and J. D. Barrow, Phys. Rev. D, 50: 7222-7232 (1994)

  • [17]

    P. J. Steinhardt and M. S. Turner, Phys. Rev. D, 29: 2162-2171 (1984)

  • [18]

    J. B. Munoz and M. Kamionkowski, Phys. Rev. D, 91: 043521 (2015)

  • [19]

    R-G. Cai, Z-K. Guo, and S-J. Wang, Phys. Rev. D, 92: 063506 (2015)

  • [20]

    Q-G Huang, K Wang, and S Wang, Phy. Rev. D, 93: 103516 (2016)

  • [21]

    J. Martin, C. Ringeval, and V. Vennina, Phys. Dark Univ., 5-6: 75 (2014)

  • [22]

    P. A. R. Ade et al. (Planck Collaboration), Astronomy. Astrophysics, 571: A16 (2014)

  • [23]

    P. A. R. Ade et al. (Planck Collaboration), Astronomy. Astrophysics, 571: A22 (2014)

  • [24]

    P. A. R. Ade et al. (Planck Collaboration), Astronomy. Astrophysics, 594: A13 (2016)

  • [25]

    P. A. R. Ade et al. (Planck Collaboration), Astronomy. Astrophysics, 594: A20 (2016)

  • [26]

    N. Aghanim et al. (Planck Collaboration), “Planck 2018 results. VI. Cosmological parameters,” arXiv: 1807.06209

  • [27]

    Y. Akrami et al. (Planck Collaboration), “Planck 2018 results. X. Constraints on inflation,” arXiv: 1807.06211

  • [28]

    P. A. R. Ade et al. (Keck Array and BICEP2 Collaborations), Phys. Rev. Lett., 116: 031302 (2016)

  • [29]

    D. I. Podolsky, G. N. Felder, L, Kofman et al., Phys. Rev. D, 73: 023501 (2006)

  • [30]

    P. A. R. Ade et al. (Keck Array and BICEP2 Collaborations), Phys. Rev. Lett., 121: 221301 (2018)

  • [31]

    L. F. Abbott, E. Farhi, and M. B. Wise, Phus. Lett. B, 117: 28 (1982)

  • [32]

    L. Kofman, A. D. Linde, and A. A. Starobinsky, Phys. Rev. D, 56: 3258-3295 (1997)

  • [33]

    R. Allahverdi, R. Brandenberger, F.Y. Cyr-Racine et al., Annu. Rev. Nucl. Part. Sci, 60: 27 (2010)

  • [34]

    A. Lewis and S. Bridle, Phys. Rev. D, 66: 103511 (2002)

  • [35]

    M. Drewes, JCAP, 03: 013 (2016)

  • [36]

    Y. Ueno and K. Yamamoto, Phys. Rev. D, 93: 083524 (2016)

  • [37]

    C. Cheng, Q. G. Huang, and W. Zhao, Sci. China Phys. Mech. Astron., 57: 1460 (2014)

  • [38]

    Q. G. Huang, S. Wang, and W. Zhao, JCAP, 1510: 035 (2015)

  • [39]

    D. H. Lyth, Phys. Rev. Lett., 78: 1861 (1997)

  • [40]

    J. Martin and C. Ringeval, Phys. Rev. D, 82: 023511 (2010)

  • [41]

    L. Dai, M. Kamionkowski, and J. Wang, Phys. Rev. Lett., 113: 041302 (2014)

  • [42]

    S. Dodelson, Modern Cosmology, (Amsterdam, Boston: Academic Press, 2003)

  • [43]

    V. F. Mukhanov, Physical Foundations of Cosmology, (Cambridge Universe Press, Cambridge, England, 2005)