[1] A. H. Guth, "Inflationary universe: A possible solution to the horizon and flatness problems", Phys. Rev. D 23, 347 (1981). DOI: 10.1103/PhysRevD.23.347
[2] A. D. Linde, "A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems", Phys. Lett. B 108 (1982). DOI: 10.1016/0370-2693(82)91219-9
[3] A. Albrecht and P. Steinhardt, "Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking", Phys. Rev. Lett. 48, 1220 (1982). DOI: 10.1103/PhysRevLett.48.1220
[4] A. D. Linde, Particle Physics and Inflationary Cosmology. Harwood, Chur, Switzerland (1990).
[5] A. Liddle and D. Lyth, Cosmological Inflation and Large-Scale Structure. Cambridge University Press (2000).
36 Mozhdeh Bitaj et al.
[6] J. E. Lidsey et al, "Reconstructing the inflaton potential|an overview", Rev. Mod. Phys. 69, 373 (1997). DOI: 10.1103/RevModPhys.69.373
[7] A. Riotto, "Inflation and the theory of cosmological perturbations", ICTP Lect. Notes Ser. 14 (2003) 317-413, [arXiv: hep-ph/0210162]. DOI: 10.48550/arXiv.hep-ph/0210162
[8] D. H. Lyth and A. R. Liddle, The Primordial Density Perturbation. Cambridge University Press (2009).
[9] J. M. Maldacena, "Non-gaussian features of primordial fluctuations in single field inflationary models", JHEP 0305, 013 (2003). DOI: 10.1088/1126-6708/2003/05/013
[10] N. D. Birrell and P. C.W. Davies, Quantum Fields in Curved Space. Cambridge Univ Press (1982).
[11] V. Faraoni, "Nonminimal coupling of the scalar field and inflation", Phys. Rev. D 53, 6813 (1996). DOI: 10.1103/PhysRevD.53.6813
[12] V. Faraoni, "Inflation and quintessence with nonminimal coupling", Phys. Rev. D 62, 023504 (2000). DOI: 10.1103/PhysRevD.62.023504
[13] A. Zee, "Broken-Symmetric Theory of Gravity", Phys. Rev. Lett. 42, 417 (1979). DOI: 10.1103/PhysRevLett.42.417
[14] F. S. Accetta, D. J. Zoller and M. S. Turner, "Induced-gravity inflation", Phys. Rev. D 31, 3046 (1985). DOI: 10.1103/PhysRevD.31.3046
[15] S. Randjbar-Daemi, A. Salam, and J. Strathdee, "On Kaluza-Klein cosmology", Phys. Lett. B 135, 388 (1984). DOI:
10.1016/0370-2693(84)90300-9
[16] T. Futamase and K. I. Maeda, "Chaotic inflationary scenario of the Universe with a nonminimally coupled "inflaton" field", Phys. Rev. D 39, 399 (1989). DOI: 10.1103/PhysRevD.39.399
[17] D. S. Salopek, J. R. Bond and J. M. Bardeen, "Designing density fluctuation spectra in inflation", Phys. Rev. D 40, 1753 (1989). DOI: 10.1103/PhysRevD.40.1753
[18] R. Fakir and W. G. Unruh, "Improvement on cosmological chaotic inflation through nonminimal coupling", Phys. Rev. D 41, 1783 (1990). DOI: 10.1103/PhysRevD.41.1783
[19] N. Makino and M. Sasaki, "The Density Perturbation in the Chaotic Inflation with Non-Minimal Coupling", Progress of Theoretical Physics, 86, 103 (1991). DOI: 10.1143/ptp/86.1.103
[20] J. Hwang and H. Noh, "COBE constraints on inflation models with a massive nonminimal scalar field", Phys. Rev. D 60, 123001 (1999). DOI: 10.1103/PhysRevD.60.123001
[21] S. Tsujikawa and H. Yajima, "New constraints on multifield inflation with nonminimal couplin", Phys. Rev. D 62, 123512 (2000). DOI: 10.1103/PhysRevD.62.123512
[22] C. Pallis, N. Toumbas, "Non-minimal sneutrino inflation, Peccei-Quinn phase transition and non-thermal leptogenesis", JCAP 1102, 019 (2011). DOI: 10.1088/1475-7516/2011/02/019
[23] K. Nozari and S. Shafizadeh, "Non-minimal inflation revisited", Physica Scripta, 82, 015901 (2010). DOI: 10.1088/0031-8949/82/01/015901
[24] N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, "Erratum: Planck 2018 results: VI. Cosmological parameters", Astronomy and Astrophysics 641, A6 (2020). DOI: 10.1051/0004-6361/201833910e
[25] Y. Akrami, F. Arroja, M. Ashdown, J. Aumont, C. Baccigalupi, "Planck 2018 resultsX. Constraints on inflation", stronomy and Astrophysics 641, A10 (2020). DOI: 10.1051/0004-6361/201833887
[26] P. A. R. Ade, Z. Ahmed, M. Amiri, D. Barkats, R. B. Thakur, "Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season", Phys. Rev. Lett. 127, 151301 (2021). DOI: 10.1103/PhysRevLett.127.151301
[27] D. Paoletti, F. Finelli, J. Valiviita and M. Hazumi, "Planck and BICEP/Keck Array 2018 constraints on primordial gravitational waves and perspectives for future Bmode polarization measurements", Phys. Rev. D 106, 083528 (2022). DOI: 10.1103/PhysRevD.106.083528
[28] Y. Akrami, F. Arroja, M. Ashdown, J. Aumont, C. Baccigalupi, "Planck 2018 results. IX. Constraints on primordial non-Gaussianity", Astronomy and Astrophysics, 641, A9 (2019). DOI: 10.1051/0004-6361/201935891
[29] J. Bardeen, "Gauge-invariant cosmological perturbations", Phys. Rev. D 22, 1882 (1980). DOI: 10.1103/PhysRevD.22.1882
[30] V. F. Mukhanov, H. A. Feldman, R. H. Brandenberger, "Theory of cosmological perturbations", Physics Reports 215, 203 (1992). DOI: 10.1016/0370-1573(92)90044-Z
[31] Daniel Baumann, "TASI Lectures on Inflation", [arXiv:0907.5424] (2009). DOI: 10.48550/arXiv.0907.5424
[32] A. De Felice and S. Tsujikawa, "Inflationary non-Gaussianities in the most general second-order scalar-tensor theories", Phys. Rev. D 84, 083504 (2011). DOI: 10.1103/PhysRevD.84.083504
[33] A. De Felice and S. Tsujikawa, "Primordial non-gaussianities in general modified gravitational models of inflation", JCAP 1104, 029 (2011). DOI: 10.1088/1475-7516/2011/04/029
[34] C. Cheung, P. Creminelli, A. L. Fitzpatrick, J. Kaplan and L. Senatore, "The effective field theory of inflation", JHEP 0803, 014 (2008). DOI: 10.1088/1126-6708/2008/03/014
[35] D. Seery and J. E. Lidsey, "Primordial non-Gaussianities in single-field inflation", JCAP, 0506, 003 (2005). DOI: 10.1088/1475-7516/2005/06/003
[36] A. De Felice, S. Tsujikawa, "Shapes of primordial non-Gaussianities in the Horndeski’s most general scalar-tensor theories", JCAP, 03, 030 (2013). DOI: 10.1088/1475-7516/2013/03/030
[37] J. Martin, C. Ringeval, R. Trotta & V. Vennin, "The best inflationary models after Planck", JCAP, 1403, 039 (2014). DOI: 10.1088/1475-7516/2014/03/039
[38] L. Senatore, "Lectures on inflation", Theoretical Advanced Study Institute in Elementary Particle Physics: new frontiers in fields and strings (2016).
[39] S. Maity, P. Rudra, "Inflation driven by Barrow holographic dark energy", JHAP 2 (1), 1-12 (2022), DOI: 10.22128/jhap.2022.464.1012
[40] S. Upadhyay, "Bouncing universe for deformed non-minimally coupled inflation model", JHAP 3 (1), 57-70 (2023), DOI: 10.22128/jhap.2023.651.1038