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Related papers: Inflation and Preheating in Supergravity with MSSM…

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Motivated by a recent discussion about the role of flat directions, a typical feature of supersymmetric models, in the process of particle production in the early universe a consistent model of inflation and preheating in supergravity with…

High Energy Physics - Phenomenology · Physics 2009-05-15 Anna Kaminska , Pawel Pacholek

We discuss constraints on which flat directions can have large vacuum expectation values (VEVs) after inflation. We show that only flat directions which are not charged under B-L and develop positive pressure due to renormalization group…

High Energy Physics - Phenomenology · Physics 2008-11-26 Micha Berkooz , Daniel J. H. Chung , Tomer Volansky

We consider the role of supersymmetric flat directions in reheating the Universe after inflation. One or more flat directions can develop large vevs during inflation, which can potentially affect reheating by slowing down scattering…

High Energy Physics - Phenomenology · Physics 2009-09-15 Keith A. Olive , Marco Peloso

Motivated by Refs \cite{am1,am2}, we analyze how the inflaton decay reheats the Universe within supersymmetry. In a non-supersymmetric case the inflaton usually decays via preheating unless its couplings to other fields are very small.…

High Energy Physics - Phenomenology · Physics 2008-11-26 Rouzbeh Allahverdi , Anupam Mazumdar

The Minimal Supersymmetry Standard Model contains several hundreds of D- and F-flat directions that are lifted by soft susy breaking terms as well as by non-renormalizable terms. In a recent paper we find that only two of these directions,…

High Energy Physics - Phenomenology · Physics 2010-11-11 Juan Garcia-Bellido

We show that a class of Wess--Zumino models lead to inflation in supersymmetry and supergravity. This is due to the existence of a classically flat direction generic to these models. The pseudomodulus that parametrizes this flat direction…

High Energy Physics - Phenomenology · Physics 2010-01-28 Edi Halyo

The potential during inflation must be very flat in, at least, the direction of the inflaton. In renormalizable global supersymmetry, flat directions are ubiquitous, but they are not preserved in a generic supergravity theory. It is known…

High Energy Physics - Theory · Physics 2009-09-29 Mary K. Gaillard , David H. Lyth , Hitoshi Murayama

We argue that all necessary ingredients for successful inflation are present in the flat directions of the minimal supersymmetric standard model (MSSM). Out of many gauge invariant combinations of the squarks, sleptons and Higgses, there…

High Energy Physics - Phenomenology · Physics 2008-11-26 Rouzbeh Allahverdi

It is well known that large Hubble-induced supergravity corrections to the inflaton field can ruin the flatness of the potential, thus creating a tension between slow-roll inflation and supergravity. In this paper we show that it is…

High Energy Physics - Theory · Physics 2012-02-13 Anupam Mazumdar , Seshadri Nadathur , Philip Stephens

We consider a possibility that one of the flat directions in the minimal supersymmetric standard model plays the role of the inflaton field and realizes large-field inflation. This is achieved by introducing a generalized shift symmetry on…

High Energy Physics - Phenomenology · Physics 2015-06-19 Shinta Kasuya , Fuminobu Takahashi

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 study the effects of primordial magnetic fields on the inflationary potential in the context of a warm inflation scenario. The model, based on global supersymmetry with a new-inflation-type potential and a coupling between the inflaton…

High Energy Physics - Phenomenology · Physics 2014-10-08 Gabriella Piccinelli , Angel Sanchez , Alejandro Ayala , Ana Julia Mizher

Most models of inflation have small parameters, either to guarantee sufficient inflation or the correct magnitude of the density perturbations. In this paper we show that, in supersymmetric theories with weak scale supersymmetry breaking,…

High Energy Physics - Phenomenology · Physics 2009-09-15 Lisa Randall , Marin Soljacic , Alan Guth

Most models of inflation have small parameters, either to guarantee sufficient inflation or the correct magnitude of the density perturbations. In this paper we show that, in supersymmetric theories with weak scale supersymmetry breaking,…

High Energy Physics - Phenomenology · Physics 2007-05-23 Lisa Randall , Marin Soljacic , Alan Guth

We compute the nonperturbative decay of supersymmetric flat directions due to their D-term potential. Flat directions can develop large vacuum expectation values (vevs) during inflation, and, if they are long-lived, this can strongly affect…

High Energy Physics - Phenomenology · Physics 2008-12-19 A. E. Gumrukcuoglu , Keith A. Olive , Marco Peloso , Matthew Sexton

We consider instant preheating as the mechanism for generating the curvature perturbation at the end of chaotic inflation. Then we examine if inflation could be driven by a Minimal Supersymmetric Standard Model (MSSM) flat direction or a…

High Energy Physics - Phenomenology · Physics 2010-10-27 Tomohiro Matsuda

We point out that for a class of `new inflation' models in supergravity the required initial value of the inflaton field is dynamically set if there is another inflation (`pre-inflation') before the `new inflation'. We study the dynamics of…

High Energy Physics - Phenomenology · Physics 2009-10-30 K. -I. Izawa , M. Kawasaki , T. Yanagida

We consider low scale slow roll inflation driven by the gauge invariant flat directions {\bf udd} and {\bf LLe} of the Minimally Supersymmetric Standard Model at the vicinity of a saddle point of the scalar potential. We study the stability…

High Energy Physics - Phenomenology · Physics 2010-10-27 Rouzbeh Allahverdi , Kari Enqvist , Juan Garcia-Bellido , Asko Jokinen , Anupam Mazumdar

We investigate a topological inflation model in supergravity. By means of numerical simulations, it is confirmed that topological inflation can take place in supergravity. We also show that the condition for successful inflation depends not…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Kawasaki , Nobuyuki Sakai , Masahide Yamaguchi , T. Yanagida

Supersymmetric Unified theories which incorporate a renormalizable Type I seesaw mechanism for small neutrino masses can also provide slow roll inflection point inflation along a flat direction associated with a gauge invariant combination…

High Energy Physics - Phenomenology · Physics 2012-09-21 Charanjit S. Aulakh , Ila Garg
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