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Related papers: Inflation and long-range force from clockwork $D$-…

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In this paper we study some models where non-Abelian gauge vector fields endowed with a SU(2) group representation are the unique source of inflation and dark energy. These models were first introduced under the name of gaugeflation and…

General Relativity and Quantum Cosmology · Physics 2020-10-13 Alejandro Guarnizo , J. Bayron Orjuela-Quintana , César A. Valenzuela-Toledo

The scale at which supersymmetry is broken and the mechanism by which supersymmetry breaking is fed down to the observable sector has rich implications on the way Nature may have chosen to accomplish inflation. We discuss a simple model for…

High Energy Physics - Phenomenology · Physics 2014-11-17 Antonio Riotto

Two distinct classes of realistic inflationary models consistent with present observations are reviewed. The first example relies on the Coleman-Weinberg potential and is readily realized within the framework of spontaneously broken global…

High Energy Physics - Phenomenology · Physics 2007-10-02 Qaisar Shafi , V. Nefer Senoguz

The shift-symmetric coupling of a pseudo-scalar particle driving inflation to gauge fields provides a unique way of probing cosmic inflation. We show for an SU(2) gauge group how a classical isotropic background gauge field develops from…

High Energy Physics - Phenomenology · Physics 2019-04-24 Valerie Domcke , Ben Mares , Francesco Muia , Mauro Pieroni

Comparisons of cosmological models to current data show that the presence of a non-trivial feature in the primordial power spectrum of fluctuations, around the scale k=0.05 h/Mpc, is an open and exciting possibility, testable in a near…

High Energy Physics - Phenomenology · Physics 2009-10-31 Julien Lesgourgues

Within supersymmetry we provide an example where the inflaton sector is derived from a gauge invariant polynomial of SU(N) or SO(N) gauge theory. Inflation in our model is driven by multi-flat directions, which assist accelerated expansion.…

High Energy Physics - Theory · Physics 2009-11-10 Asko Jokinen , Anupam Mazumdar

In this work, we propose a model of warm inflation driven by axion-like particles interacting with $U(1)$ gauge fields, with implications for the early universe's thermal evolution. By extending traditional warm inflation models, we…

Cosmology and Nongalactic Astrophysics · Physics 2025-07-24 Asma Alaei , Sukannya Bhattacharya , Vahid Kamali

An inflationary stage dominated by a D-term avoids the slow-roll problem of inflation in supergravity and can naturally emerge in theories with a non-anomalous or anomalous U(1) gauge symmetry. In this talk different aspects of D-term…

High Energy Physics - Phenomenology · Physics 2016-10-26 Antonio Riotto

We present a solution to the cosmological problem encountered in (supersymmetric) grand unified theories due to copious monopole production at the end of hybrid inflation. By employing thermal inflation ``driven'' by the U(1) axion…

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

Two of the most attractive realizations of inflation in supergravity are based upon the presence of a constant Fayet-Iliopoulos (FI) term. In D-term hybrid inflation it is the FI term itself which sets the energy scale of inflation.…

High Energy Physics - Theory · Physics 2014-11-11 Clemens Wieck , Martin Wolfgang Winkler

Models of chaotic inflation with a fractional power-law potential are not only viable but also testable in the foreseeable future. We show that such models can be realized in simple strongly coupled supersymmetric gauge theories. In these…

High Energy Physics - Phenomenology · Physics 2015-06-12 Keisuke Harigaya , Masahiro Ibe , Kai Schmitz , Tsutomu T. Yanagida

We propose a cosmological framework in which neutrino masses evolve dynamically through coupling with a scalar field that simultaneously drives inflation. The neutrino mass is modeled as a power-law, exponential, or hybrid function of the…

Cosmology and Nongalactic Astrophysics · Physics 2025-12-01 Hemanshi Bundeliya , Gaurav Bhandari , S. D. Pathak , V. K. Sharma

When Inflation is embedded in a fundamental theory, such as string theory, it typically begins when the Universe is already substantially larger than the fundamental scale [such as the one defined by the string length scale]. This is…

General Relativity and Quantum Cosmology · Physics 2010-09-03 Brett McInnes

We present a new model of D-term dominated chaotic inflation in supergravity. The F-flat direction present in this model is lifted by the dominant D-term, which leads to chaotic inflation and subsequent reheating. No cosmic string is formed…

High Energy Physics - Phenomenology · Physics 2008-11-26 Kenji Kadota , Teruhiko Kawano , Masahide Yamaguchi

We consider an inflationary scenario where the energy scale of inflation stems from gauge theory dynamics. We point out its generic implications on vacuum selection of our universe, in particular, on determination of spacetime symmetries…

High Energy Physics - Phenomenology · Physics 2009-10-31 K. -I. Izawa , T. Yanagida

The large hierarchy between the Planck scale and the weak scale can be explained by the dynamical breaking of supersymmetry in strongly coupled gauge theories. Similarly, the hierarchy between the Planck scale and the energy scale of…

High Energy Physics - Phenomenology · Physics 2017-11-22 Keisuke Harigaya , Kai Schmitz

We explore the possibility that inflation is driven by supersymmetry breaking with the superpartner of the goldstino (sgoldstino) playing the role of the inflaton. Moreover, we impose an R-symmetry that allows to satisfy easily the…

High Energy Physics - Theory · Physics 2017-11-22 Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono , Rob Knoops

Standard D-term inflation is studied in the framework of supergravity. D-term inflation produces cosmic strings, however it can still be compatible with CMB measurements without invoking any new physics. The cosmic strings contribution to…

High Energy Physics - Phenomenology · Physics 2009-11-10 Jonathan Rocher , Mairi Sakellariadou

We study the inflation due to the D-flat direction of an extra $U(1)$. This scenario is a hybrid of a right-handed sneutrino inflaton scenario and a gauge non-singlet inflaton scenario. The inflaton is a gauge non-singlet field which…

High Energy Physics - Phenomenology · Physics 2009-10-28 Daijiro Suematsu , Yoshio Yamagishi

Dynamical models of inflation are given with composite inflatons by means of massive supersymmetric gauge theory. Nearly flat directions and stable massive ones in the potential are identified and slow-roll during inflation is examined.…

High Energy Physics - Phenomenology · Physics 2008-11-26 K. Hamaguchi , K. -I. Izawa , H. Nakajima