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The supersymmetric model of hybrid inflation is interesting not only because of its naturalness but also because of another reason. Its energy scale determined by the COBE normalization is 10^15 - 10^16 GeV. It happens to be the energy…

High Energy Physics - Phenomenology · Physics 2014-11-17 Taizan Watari , T. Yanagida

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical abelian projection and centerization. The underlying gauge symmetry is…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ralf Hofmann , Mathias Th. Keil

The Standard Model Higgs boson with large nonminimal coupling to the gravitational curvature can drive cosmological inflation. We study this type of inflationary scenario in the context of supersymmetric grand unification and point out that…

High Energy Physics - Phenomenology · Physics 2013-05-29 Masato Arai , Shinsuke Kawai , Nobuchika Okada

We analyze the adjoint field inflation in supersymmetric (SUSY) SU(5) model. In minimal SUSY SU(5) hybrid inflation monopoles are produced at the end of inflation. We therefore explore the non-minimal model of inflation based on SUSY SU(5),…

High Energy Physics - Phenomenology · Physics 2011-05-10 S. Khalil , M. U. Rehman , Q. Shafi , E. A. Zaakouk

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical Abelian projection and centerization. The underlying gauge symmetry is…

High Energy Physics - Phenomenology · Physics 2009-11-07 Ralf Hofmann , Mathias Th. Keil

Higgs inflation is attractive because it identifies the inflaton with the electroweak Higgs boson. In this work, we construct a new class of supersymmetric Higgs inflationary models in the no-scale supergravity with an SU(5) GUT group.…

High Energy Physics - Phenomenology · Physics 2015-01-22 John Ellis , Hong-Jian He , Zhong-Zhi Xianyu

After reviewing the motivations for cosmological inflation formulated in the formalism of supersymmetry, we argue that the appropriate framework is that of no-scale supergravity. We then show how to construct within this framework…

High Energy Physics - Phenomenology · Physics 2021-02-24 John Ellis , Marcos A. G. Garcia , Natsumi Nagata , Dimitri V. Nanopoulos , Keith A. Olive , Sarunas Verner

We consider models of inflation in supergravity with a shift symmetry. We focus on models with one moduli and one inflaton field. The presence of this symmetry guarantees the existence of a flat direction for the inflaton field. Mildly…

High Energy Physics - Theory · Physics 2009-11-11 Philippe Brax , Jerome Martin

A single field inflation based on a supergravity model with a shift symmetry and $U(1)$ extension of the MSSM is analyzed. We show that one of the real components of the two $U(1)$ charged scalar fields plays the role of inflaton {with} an…

High Energy Physics - Phenomenology · Physics 2015-10-28 Lucien Heurtier , Shaaban Khalil , Ahmad Moursy

We present a new mechanism for slow-roll inflation based on higher dimensional supersymmetric gauge theory compactified to four dimensions with twisted (supersymmetry breaking) boundary conditions. These boundary conditions lead to a…

High Energy Physics - Theory · Physics 2011-01-27 Joshua L. Davis , Thomas S. Levi , Mark Van Raamsdonk , Kevin R. L. Whyte

In a recent paper we proposed a new model of inflation based on the soft-breaking of N=2 supersymmetric SU(2) Yang-Mills theory. The advantage of such a model is the fact that we can write an exact expression for the effective scalar…

High Energy Physics - Phenomenology · Physics 2016-10-26 Juan Garcia-Bellido

We consider a set of scalar fields, consisting of a single flat direction and one or several non-flat directions. We take our cue from the MSSM, considering separately D-flat and F-flat directions, but our results apply to any…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Kari Enqvist , Daniel G. Figueroa , Gerasimos Rigopoulos

We explore the possibility that a multiple-stage inflationary scenario based on supersymmetric GUT models, can account for the break at $k_b \simeq 0.05 h/Mpc$ in the power spectrum of galaxy clustering, while it reproduces the angular…

High Energy Physics - Phenomenology · Physics 2009-10-31 Mairi Sakellariadou

We realize and study a model of hybrid inflation in the context of softly broken supersymmetry. The inflaton is taken to be a flat direction in the superfield space and, due to unsuppressed couplings, its soft supersymmetry breaking mass…

High Energy Physics - Phenomenology · Physics 2016-08-25 Laura Covi

We study inflation in a supersymmetric Pati-Salam model driven by a potential generated in the context of no-scale supergravity. The Pati-Salam gauge group $SU(4)_{c}\times{SU(2)_{L}\times{SU(2)_{R}}}$ , is supplemented with a $Z_{2} $…

High Energy Physics - Phenomenology · Physics 2018-08-01 Waqas Ahmed , Athanasios Karozas

We present possible realizations of gauge inflation arising from a 5D ${\cal N}=1$ supersymmetric U(1) model, where the extra dimension is compactified on a circle. A one-loop inflaton effective 4D potential is generated, with the inflaton…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. Hofmann , F. Paccetti Correia , M. G. Schmidt , Z. Tavartkiladze

We show that simple strongly coupled supersymmetric gauge theories with quantum moduli spaces can naturally lead to hybrid inflation. These theories contain no input dimensionful or small parameters. The effective superpotential is linear…

High Energy Physics - Phenomenology · Physics 2009-10-30 Savas Dimopoulos , Gia Dvali , Riccardo Rattazzi

Inflation, as currently understood, requires the presence of fields with very flat potentials. Supersymmetric models in which supersymmetry breaking is communicated by supergravity naturally yield such fields, but the scales are typically…

High Energy Physics - Phenomenology · Physics 2009-10-30 Michael Dine , Antonio Riotto

An inflation model with inverse symmetry breaking of two scalar fields is proposed. Constraints on the parameters for a successful inflation are obtained. In general the inequality $\lambda_1\ll g <\lambda_2$ should be satisfied, where…

High Energy Physics - Phenomenology · Physics 2014-11-17 Jae-weon Lee , In-guy Koh

A sizeable tensor-to-scalar ratio, such as recently claimed by BICEP2, would imply a scale of inflation at the typical scale of supersymmetric grand unification. This could be an accident, or strong support for supersymmetric theories.…

High Energy Physics - Phenomenology · Physics 2015-06-19 Felix Brummer , Valerie Domcke , Veronica Sanz