Built on

S. R. Coleman and E. J. Weinberg, Radiative Corrections as the Origin of Spontaneous Symmetry Breaking
1910
Earlier work this paper cites.
L. Järv, P. Kuusk, M. Saal, and O. Vilson, Invariant quantities in the scalar-tensor theories of gravitation
Original
1947
Earlier work this paper cites.
A. A. Starobinsky, A New Type of Isotropic Cosmological Models Without Singularity
1980
Earlier work this paper cites.
A. H. Guth, The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems
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
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
1982
Earlier work this paper cites.
A. D. Linde, Coleman-Weinberg Theory and a New Inflationary Universe Scenario
1982
Earlier work this paper cites.
J. R. Ellis, D. V. Nanopoulos, K. A. Olive, and K. Tamvakis, PRIMORDIAL SUPERSYMMETRIC INFLATION
1983
Earlier work this paper cites.
J. R. Ellis, D. V. Nanopoulos, K. A. Olive, and K. Tamvakis, Fluctuations in a Supersymmetric Inflationary Universe
1983
Earlier work this paper cites.
A. R. Liddle, P. Parsons, and J. D. Barrow, Formalizing the slow roll approximation in inflation
1994
Earlier work this paper cites.
W. A. Bardeen, On naturalness in the standard model
1995
Earlier work this paper cites.
R. Hempfling, The Next-to-minimal Coleman-Weinberg model
1996
Earlier work this paper cites.
N. C. Tsamis and R. P. Woodard, Improved estimates of cosmological perturbations
2004
Earlier work this paper cites.
F. L. Bezrukov and M. Shaposhnikov, The Standard Model Higgs boson as the inflaton
Original
2008
Earlier work this paper cites.
F. Bezrukov, A. Magnin, M. Shaposhnikov, and S. Sibiryakov, Higgs inflation: consistency and generalisations
Original
2011
Earlier work this paper cites.
J. Martin, H. Motohashi, and T. Suyama, Ultra Slow-Roll Inflation and the non-Gaussianity Consistency Relation
Original
2013
Earlier work this paper cites.
K. Kannike, A. Racioppi, and M. Raidal, Embedding inflation into the Standard Model - more evidence for classical scale invariance
Original
2014
Earlier work this paper cites.
M. Heikinheimo, A. Racioppi, M. Raidal, C. Spethmann, and K. Tuominen, Physical Naturalness and Dynamical Breaking of Classical Scale Invariance
Original
2014
Earlier work this paper cites.
E. Gabrielli, M. Heikinheimo, K. Kannike, A. Racioppi, M. Raidal, and C. Spethmann, Towards Completing the Standard Model: Vacuum Stability, EWSB and Dark Matter
Original
2014
Earlier work this paper cites.

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2017

Constant-Roll (Quasi-)Linear Inflation

Karam, Alexandros, Marzola, Luca, Pappas, Thomas et al.

Understand

In constant-roll inflation, the scalar field that drives the accelerated expansion of the Universe is rolling down its potential at a constant rate.

Within this framework, we highlight the relations between the Hubble slow-roll parameters and the potential ones, studying in detail the case of a single-field Coleman-Weinberg model characterised by a non-minimal coupling of the inflaton to gravity.
With respect to the exact constant-roll predictions, we find that assuming an approximate slow-roll behaviour yields a difference of $\Delta r = 0.001$ in the tensor-to-scalar ratio prediction.
Such a discrepancy is in principle testable by future satellite missions.

Built on

S. R. Coleman and E. J. Weinberg, Radiative Corrections as the Origin of Spontaneous Symmetry Breaking
1910
Earlier work this paper cites.
L. Järv, P. Kuusk, M. Saal, and O. Vilson, Invariant quantities in the scalar-tensor theories of gravitation
Original
1947
Earlier work this paper cites.
A. A. Starobinsky, A New Type of Isotropic Cosmological Models Without Singularity
1980
Earlier work this paper cites.
A. H. Guth, The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems
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
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
1982
Earlier work this paper cites.
A. D. Linde, Coleman-Weinberg Theory and a New Inflationary Universe Scenario
1982
Earlier work this paper cites.
J. R. Ellis, D. V. Nanopoulos, K. A. Olive, and K. Tamvakis, PRIMORDIAL SUPERSYMMETRIC INFLATION
1983
Earlier work this paper cites.
J. R. Ellis, D. V. Nanopoulos, K. A. Olive, and K. Tamvakis, Fluctuations in a Supersymmetric Inflationary Universe
1983
Earlier work this paper cites.
A. R. Liddle, P. Parsons, and J. D. Barrow, Formalizing the slow roll approximation in inflation
1994
Earlier work this paper cites.
W. A. Bardeen, On naturalness in the standard model
1995
Earlier work this paper cites.
R. Hempfling, The Next-to-minimal Coleman-Weinberg model
1996
Earlier work this paper cites.
N. C. Tsamis and R. P. Woodard, Improved estimates of cosmological perturbations
2004
Earlier work this paper cites.
F. L. Bezrukov and M. Shaposhnikov, The Standard Model Higgs boson as the inflaton
Original
2008
Earlier work this paper cites.
F. Bezrukov, A. Magnin, M. Shaposhnikov, and S. Sibiryakov, Higgs inflation: consistency and generalisations
Original
2011
Earlier work this paper cites.
J. Martin, H. Motohashi, and T. Suyama, Ultra Slow-Roll Inflation and the non-Gaussianity Consistency Relation
Original
2013
Earlier work this paper cites.
K. Kannike, A. Racioppi, and M. Raidal, Embedding inflation into the Standard Model - more evidence for classical scale invariance
Original
2014
Earlier work this paper cites.
M. Heikinheimo, A. Racioppi, M. Raidal, C. Spethmann, and K. Tuominen, Physical Naturalness and Dynamical Breaking of Classical Scale Invariance
Original
2014
Earlier work this paper cites.
E. Gabrielli, M. Heikinheimo, K. Kannike, A. Racioppi, M. Raidal, and C. Spethmann, Towards Completing the Standard Model: Vacuum Stability, EWSB and Dark Matter
Original
2014
Earlier work this paper cites.