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A. H. Guth, “The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems”, Phys.Rev
1981
Earlier work this paper cites.
A. D. Linde, “A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems”, Phys.Lett
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, “Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking”, Phys.Rev.Lett
1982
Earlier work this paper cites.
A. D. Linde, “Chaotic Inflation”, Phys.Lett
1983
Earlier work this paper cites.
K. Freese, J. A. Frieman, and A. V. Olinto, “Natural inflation with pseudo - Nambu-Goldstone bosons”, Phys.Rev.Lett
1990
Earlier work this paper cites.
A. D. Linde, “Hybrid inflation”, Phys.Rev
1994
Earlier work this paper cites.
D. H. Lyth, “What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?”, Phys.Rev.Lett
1997
Earlier work this paper cites.

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Original
2012

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2014

Garcia-Bellido, Juan, Roest, Diederik, Scalisi, Marco et al.

We study to what extent the spectral index $n_s$ and the tensor-to-scalar ratio $r$ determine the field excursion $\Delta\phi$ during inflation.

We analyse the possible degeneracy of $\Delta \phi$ by comparing three broad classes of inflationary models, with different dependence on the number of e-foldings $N$, to benchmark models of chaotic inflation with monomial potentials.
The classes discussed cover a large set of inflationary single field models.
We find that the field range is not uniquely determined for any value of $(n_s, r)$; one can have the same predictions as chaotic inflation and a very different $\Delta \phi$.

A. H. Guth, “The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems”, Phys.Rev
1981
Earlier work this paper cites.
A. D. Linde, “A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems”, Phys.Lett
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, “Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking”, Phys.Rev.Lett
1982
Earlier work this paper cites.
A. D. Linde, “Chaotic Inflation”, Phys.Lett
1983
Earlier work this paper cites.
K. Freese, J. A. Frieman, and A. V. Olinto, “Natural inflation with pseudo - Nambu-Goldstone bosons”, Phys.Rev.Lett
1990
Earlier work this paper cites.
A. D. Linde, “Hybrid inflation”, Phys.Rev
1994
Earlier work this paper cites.
D. H. Lyth, “What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?”, Phys.Rev.Lett
1997
Earlier work this paper cites.

D. J. Schwarz, C. A. Terrero-Escalante, and A. A. Garcia, “Higher order corrections to primordial spectra from cosmological inflation”, Phys.Lett
2001
Cited alongside, same era.
A. R. Liddle and S. M. Leach, “How long before the end of inflation were observable perturbations produced?”, Phys.Rev
2003
Cited alongside, same era.
D. J. Schwarz and C. A. Terrero-Escalante, “Primordial fluctuations and cosmological inflation after WMAP 1.0”, JCAP
2004
Cited alongside, same era.
D. Boyanovsky, H. J. de Vega, and N. G. Sanchez, “Clarifying Inflation Models: Slow-roll as an expansion in 1 / N e f o l d s 1/N_{efolds} ”, Phys.Rev
2006
Cited alongside, same era.
S. Hotchkiss, A. Mazumdar, and S. Nadathur, “Observable gravitational waves from inflation with small field excursions”, JCAP
Original
2012