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Y. Akrami et al
Original
1905
Earlier work this paper cites.
R. Kallosh and A. Linde, “B-mode Targets,” arXiv:1906.04729 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
M. Sasaki, “Large Scale Quantum Fluctuations in the Inflationary Universe,” Prog. Theor. Phys. 76
1986
Earlier work this paper cites.
V. F. Mukhanov, “Quantum Theory of Gauge Invariant Cosmological Perturbations,” Sov. Phys. JETP 67
1988
Earlier work this paper cites.
K. Freese, J. A. Frieman and A. V. Olinto, “Natural inflation with pseudo - Nambu-Goldstone bosons,” Phys. Rev. Lett. 65
1990
Earlier work this paper cites.
M. Sasaki and E. D. Stewart, “A General analytic formula for the spectral index of the density perturbations produced during inflation,” Prog. Theor. Phys. 95
1996
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour and V. F. Mukhanov, “k - inflation,” Phys. Lett. B 458
1999
Earlier work this paper cites.
J. Garriga and V. F. Mukhanov, “Perturbations in k-inflation,” Phys. Lett. B 458
1999
Earlier work this paper cites.
C. Gordon, D. Wands, B. A. Bassett and R. Maartens, “Adiabatic and entropy perturbations from inflation,” Phys. Rev. D 63
2001
Earlier work this paper cites.
S. Groot Nibbelink and B. J. W. van Tent, “Scalar perturbations during multiple field slow-roll inflation,” Class. Quant. Grav. 19
2002
Earlier work this paper cites.
M. Alishahiha, E. Silverstein and D. Tong, “DBI in the sky,” Phys. Rev. D 70
2004
Earlier work this paper cites.

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2019

Flattened Axion Monodromy Beyond Two Derivatives

Pedro, Francisco G., Westphal, Alexander

Understand

We study string inspired two-field models of large-field inflation based on axion monodromy in the presence of an interacting heavier modulus.

This class of models has enough structure to approximate at least part of the backreaction effects known in full string theory, such as kinetic mixing with the axion, and flattening of the scalar potential.
Yet, it is simple enough to fully describe the structure of higher-point curvature perturbation interactions driven by the adjusting modulus backreaction dynamics.
We find that the presence of the heavy modulus can be described via two equivalent effective field theories, both of which can incorporate reductions of the speed of sound.

Built on

Y. Akrami et al
Original
1905
Earlier work this paper cites.
R. Kallosh and A. Linde, “B-mode Targets,” arXiv:1906.04729 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
M. Sasaki, “Large Scale Quantum Fluctuations in the Inflationary Universe,” Prog. Theor. Phys. 76
1986
Earlier work this paper cites.
V. F. Mukhanov, “Quantum Theory of Gauge Invariant Cosmological Perturbations,” Sov. Phys. JETP 67
1988
Earlier work this paper cites.
K. Freese, J. A. Frieman and A. V. Olinto, “Natural inflation with pseudo - Nambu-Goldstone bosons,” Phys. Rev. Lett. 65
1990
Earlier work this paper cites.
M. Sasaki and E. D. Stewart, “A General analytic formula for the spectral index of the density perturbations produced during inflation,” Prog. Theor. Phys. 95
1996
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour and V. F. Mukhanov, “k - inflation,” Phys. Lett. B 458
1999
Earlier work this paper cites.
J. Garriga and V. F. Mukhanov, “Perturbations in k-inflation,” Phys. Lett. B 458
1999
Earlier work this paper cites.
C. Gordon, D. Wands, B. A. Bassett and R. Maartens, “Adiabatic and entropy perturbations from inflation,” Phys. Rev. D 63
2001
Earlier work this paper cites.
S. Groot Nibbelink and B. J. W. van Tent, “Scalar perturbations during multiple field slow-roll inflation,” Class. Quant. Grav. 19
2002
Earlier work this paper cites.
M. Alishahiha, E. Silverstein and D. Tong, “DBI in the sky,” Phys. Rev. D 70
2004
Earlier work this paper cites.