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We study an inflationary scenario in supergravity model with a gauge kinetic function. We find exact anisotropic power-law inflationary solutions when both the potential function for an inflaton and the gauge kinetic function are…

High Energy Physics - Theory · Physics 2011-03-10 Sugumi Kanno , Jiro Soda , Masa-aki Watanabe

Inflationary models driven by a large number of axion fields are discussed in the context of type IIB compactifications with N=1 supersymmetry. The inflatons arise as the scalar modes of the R-R two-forms evaluated on vanishing two-cycles…

High Energy Physics - Theory · Physics 2008-06-13 Thomas W. Grimm

The $N=1$ supergravity models of cosmological inflation with inflaton belonging to a massive vector multiplet and spontaneous SUSY breaking after inflation are reformulated as the supersymmetric $U(1)$ gauge theories of a massless vector…

High Energy Physics - Theory · Physics 2017-05-24 Yermek Aldabergenov , Sergei V. Ketov

A supersymmetric inflationary stage dominated by an $F$-term has the problem that the flatness of the potential is spoiled by supergravity corrections, that is the slow-roll parameter $\eta$ gets contributions of order unity. We show that…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. A. Casas , G. B. Gelmini , A. Riotto

In the context of supersymmetric models, we analyze the production of topological defects at the end of inflation driven by a conjugate pair of inflaton fields which are non-singlets under the continuous symmetry group of the theory. We…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides , Q. Shafi

A model of chaotic inflation based on the theory of a scalar field with potential \lambda\phi^4 perfectly matches the observational data if one adds to it a tiny non-minimal coupling to gravity -\xi/2 \phi^2 R with \xi > 0.002. We describe…

High Energy Physics - Theory · Physics 2015-06-16 Renata Kallosh , Andrei Linde

The main problem of inflation in string theory is finding the models with a flat potential, consistent with stabilization of the volume of the compactified space. This can be achieved in the theories where the potential has (an approximate)…

High Energy Physics - Theory · Physics 2009-11-10 Jonathan P. Hsu , Renata Kallosh

The idea of gauge theories of gravity predicts that there should exist not only the massless graviton but also massive particles carrying the gravitational force. We study the cosmology in a quadratic gravity with dynamical torsion where…

High Energy Physics - Theory · Physics 2020-06-17 Katsuki Aoki , Shinji Mukohyama

We investigate axion-inflation baryogenesis models, embedded into U(1) gauge symmetric extensions of the Standard Model (SM), in which the new gauge field couples to the pseudo-scalar inflaton via the Chern-Simons coupling. The motion of…

High Energy Physics - Phenomenology · Physics 2024-09-30 Wei Chao , Yonghua Wang , Chenhui Xie

Gaugino condensation is discussed in the context of a consistent new version of low energy heterotic M-theory. The four dimensional reduction of the theory is described, based on simple boson and fermion backgrounds. This is generalised to…

High Energy Physics - Theory · Physics 2009-01-14 Nasr Ahmed , Ian G Moss

Slow-roll inflation is a successful paradigm. However we find that even a small coupling of the inflaton to other light fields can dramatically alter the dynamics and predictions of inflation. As an example, the inflaton can generically…

High Energy Physics - Phenomenology · Physics 2023-09-19 Kim V. Berghaus , Peter W. Graham , David E. Kaplan

Viewing gravitational energy momentum $p_G^\mu$ as equal by observation, but different in essence from inertial energy-momentum $p_I^\mu$ requires two different symmetries to account for their independent conservations - spacetime and inner…

Mathematical Physics · Physics 2012-02-28 C. Wiesendanger

The recently suggested generalized unimodular gravity theory, which was originally put forward as a model of dark energy, can serve as a model of cosmological inflation driven by the effective perfect fluid -- the dark purely gravitational…

General Relativity and Quantum Cosmology · Physics 2019-12-11 A. O. Barvinsky , N. Kolganov

Axions with broken discrete shift symmetry (axion monodromy) have recently played a central role both in the discussion of inflation and the `relaxion' approach to the hierarchy problem. We suggest a very minimalist way to constrain such…

High Energy Physics - Theory · Physics 2016-07-21 Arthur Hebecker , Fabrizio Rompineve , Alexander Westphal

We present a simple argument which seems to favor, when applied to a large class of strongly-coupled chiral gauge theories, a dynamical-Higgs-phase scenario, characterized by certain bifermion condensates. Flavor symmetric confining vacua…

High Energy Physics - Theory · Physics 2021-09-01 Stefano Bolognesi , Kenichi Konishi , Andrea Luzio

Starting from the previously constructed effective supergravity theory below the scale of U(1) breaking in orbifold compactifications of the weakly coupled heterotic string, we study the effective theory below the scale of supersymmetry…

High Energy Physics - Theory · Physics 2014-11-18 Mary K. Gaillard , Joel Giedt , Aleksey L. Mints

We show that inflation which is dominated by the D-term density avoids the `slow-roll' problem of inflation in supergravity. Such an inflationary scenario can naturally emerge in theories with non-anomalous or anomalous U(1) gauge symmetry.…

High Energy Physics - Phenomenology · Physics 2009-10-28 Pierre Binetruy , Gia Dvali

We present a formulation of gravity in terms of a theory based on complex SU(2) gauge fields with a general coordinate invariant action functional quadratic in the field strength. Self-duality or anti-self-duality of the field strength…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Romesh K. Kaul

Automorphic inflation is an application of the framework of automorphic scalar field theory, based on the theory of automorphic forms and representations. In this paper the general framework of automorphic and modular inflation is described…

High Energy Physics - Theory · Physics 2016-07-12 Rolf Schimmrigk

The QCD axion in the pre-inflation scenario faces a stringent isocurvature constraint, which requires a relatively low Hubble scale during inflation. If the axion was heavier than the Hubble scale during inflation, its isocurvature is…

High Energy Physics - Phenomenology · Physics 2026-01-19 Priyesh Chakraborty , Junyi Cheng , Matthew Reece , Zekai Wang
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