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Related papers: Phases of Inflation

200 papers

We study the multifield dynamics of axion models nonminimally coupled to gravity. As usual, we consider a canonical $U(1)$ symmetry-breaking model in which the axion is the phase of a complex scalar field. If the complex scalar field has a…

High Energy Physics - Theory · Physics 2024-06-07 Evan McDonough , Alan H. Guth , David I. Kaiser

Inflation generally assumes a field with nonzero potential that leads to inflationary expansion happening at arbitrarily early times. We demonstrate potentially observable consequences of inflation with a finite initial time in a model in…

High Energy Physics - Theory · Physics 2025-12-05 Rashmish K. Mishra , Michael Nee , Lisa Randall

In models of natural inflation, the inflaton is an axion-like particle. Unfortunately, axion potentials in UV-complete theories appear to be too steep to drive inflation. We show that, even for a steep potential, natural inflation can occur…

High Energy Physics - Theory · Physics 2015-05-14 Mohamed M. Anber , Lorenzo Sorbo

In this paper we incorporate gauge fields into the tachyon field theory models for unstable D-branes in bosonic and in Type II string theories. The chosen couplings yield massless gauge fields and an infinite set of equally spaced massive…

High Energy Physics - Theory · Physics 2009-10-31 Joseph A. Minahan , Barton Zwiebach

We study inflation driven by a dilaton and an axion, both of which are coupled to a SU(2) gauge field. We find that the inflation driven by the dilaton occurs in the early stage of inflation during which the gauge field grows due to the…

High Energy Physics - Theory · Physics 2016-06-08 Ippei Obata , Jiro Soda

Intersecting D-brane models and their T-dual magnetic compactifications yield attractive models of particle physics where magnetic flux plays a twofold role, being the source of fermion chirality as well as supersymmetry breaking. A…

High Energy Physics - Theory · Physics 2020-02-11 Wilfried Buchmuller , Emilian Dudas , Yoshiyuki Tatsuta

We propose a new inflation scenario in flux compactification, where a zero mode scalar field of extra components of the higher dimensional gauge field is identified with an inflaton. The scalar field is a pseudo Nambu-Goldstone boson of…

High Energy Physics - Theory · Physics 2021-10-04 Takuya Hirose , Nobuhito Maru

We propose a model for large field inflation in heterotic string theory. The construction applies the near alignment mechanism of Kim, Nilles, and Peloso. By including gaugino condensates and world-sheet instanton non-perturbative effects,…

High Energy Physics - Theory · Physics 2015-04-16 Tibra Ali , S. Shajidul Haque , Vishnu Jejjala

I review a (3+1)-dimensional, string-inspired cosmological model with gravitational anomalies (of Chern-Simons (CS) type) at early epochs, and a totally-antisymmetric torsion, dual to a massless axion-like field ("gravitational axion"),…

High Energy Physics - Theory · Physics 2022-12-29 Nick E. Mavromatos

The recent discovery of B-mode polarizations in the CMB by the BICEP2 collaboration motivates the study of large-field inflation models which can naturally lead to significant tensor-to-scalar ratios. A class of such models in string theory…

High Energy Physics - Theory · Physics 2015-06-19 Eran Palti , Timo Weigand

We investigate the reheating process in an axion inflation model where the inflaton couples to non-Abelian gauge fields via the Chern-Simons coupling. The Chern-Simons coupling leads to the efficient production of gauge fields via a…

High Energy Physics - Phenomenology · Physics 2025-03-04 Tomohiro Fujita , Kyohei Mukaida , Tenta Tsuji

The inflationary paradigm has enjoyed phenomenological success, however, a compelling particle physics realization is still lacking. The key obstruction is that the requirement of a suitably flat scalar potential is sensitive to…

High Energy Physics - Phenomenology · Physics 2011-05-12 Neil Barnaby , Marco Peloso

Axion monodromy models can always be described in terms of an axion coupled to 3-form gauge fields with non-canonical kinetic terms. The presence of the saxions parametrising the kinetic metrics of the 3-form fields leads to backreaction…

High Energy Physics - Theory · Physics 2017-08-25 Irene Valenzuela

In this paper, we study the dynamics of the Chern-Simons Inflation Model proposed by Alexander, Marciano and Spergel. According to this model, inflation begins when a fermion current interacts with a turbulent gauge field in a space larger…

General Relativity and Quantum Cosmology · Physics 2014-04-01 David Garrison

The mechanism of dynamical chiral symmetry breaking is studied in the Abelian version of the gauged Nambu-Jona-Lasinio model in four dimensions. The most interesting feature of the gauged Nambu-Jona-Lasinio model is the appearance of…

High Energy Physics - Theory · Physics 2007-05-23 Manuel Reenders

We analyze the signatures of inflationary models that are coupled to strongly interacting field theories, a basic class of multifield models also motivated by their role in providing dynamically small scales. Near the squeezed limit of the…

High Energy Physics - Theory · Physics 2015-06-12 Daniel Green , Matthew Lewandowski , Leonardo Senatore , Eva Silverstein , Matias Zaldarriaga

We use a lattice simulation to study a model of axion inflation where the inflaton is coupled to a U(1) gauge field through Chern-Simons interaction. These kinds of models have already been studied with a lattice simulation in the context…

Cosmology and Nongalactic Astrophysics · Physics 2022-06-28 Angelo Caravano , Eiichiro Komatsu , Kaloian D. Lozanov , Jochen Weller

Axion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. This is particularly true in the strong backreaction regime, where the gauge…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-15 Valerie Domcke , Yohei Ema , Stefan Sandner

We study the non-linear dynamics of axion inflation, capturing for the first time the inhomogeneity and full dynamical range during strong backreaction, till the end of inflation. Accounting for inhomogeneous effects leads to a number of…

Cosmology and Nongalactic Astrophysics · Physics 2023-05-01 Daniel G. Figueroa , Joanes Lizarraga , Ander Urio , Jon Urrestilla

We propose an inflationary scenario, M-flation, in which inflation is driven by three $N\times N$ hermitian matrices $\Phi_i, i=1,2,3$. The inflation potential of our model, which is strongly motivated from string theory, is constructed…

High Energy Physics - Theory · Physics 2010-10-13 Amjad Ashoorioon , Hassan Firouzjahi , M. M. Sheikh-Jabbari