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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 2009-11-19 Anna Kaminska , Pawel Pacholek

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 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

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 review the cosmological implications of the flat directions of the Minimally Supersymmetric Standard Model (MSSM). We describe how field condensates are created along the flat directions because of inflationary fluctuations. The…

High Energy Physics - Phenomenology · Physics 2011-07-19 Kari Enqvist , Anupam Mazumdar

We consider the possibility that the vacuum energy density of the MSSM (Minimal Supersymmetric Standard Model) flat direction condensate involving the Higgses H_1 and H_2 is responsible for inflation. We also discuss how the finely tuned…

High Energy Physics - Phenomenology · Physics 2015-05-27 Arindam Chatterjee , Anupam Mazumdar

Supersymmetric flat directions allow a generic counterexample to the phenomenon of symmetry restoration at high temperatures. We show that (exponentially) large VEVs can be developed along these directions through temperature-induced…

High Energy Physics - Phenomenology · Physics 2007-05-23 Gia Dvali , Lawrence M. Krauss

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

One interpretation of proton stability is the existence of extra-flat directions of the MSSM, in particular $u^{c}u^{c}d^{c}e^{c}$ and $QQQL$, where the operators lifting the potential are suppressed by a mass scale $\Lambda$ which is much…

High Energy Physics - Phenomenology · Physics 2008-11-26 John McDonald , Osamu Seto

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

Supersymmetric theories, including the minimal supersymmetric standard model, usually contain many scalar fields whose potentials are absent in the exact supersymmetric limit and within the renormalizable level. Since their potentials are…

High Energy Physics - Phenomenology · Physics 2015-10-14 Ayuki Kamada , Masaki Yamada

Curvaton is an effectively massless field whose energy density during inflation is negligible but which later becomes dominant. This is a novel mechanism to generate the scale invariant perturbations. I discuss the possibility that the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kari Enqvist

Non-perturbative preheating decay of post-inflationary condensates often results in a high density, low momenta, non-thermal gas. In the case where the non-perturbative classical evolution also leads to Q-balls, this effect shields them…

High Energy Physics - Phenomenology · Physics 2009-11-11 Micha Berkooz , Daniel J. H. Chung , Tomer Volansky

Coherently oscillating scalar condensates formed along flat directions of the MSSM scalar potential are unstable with respect to spatial perturbations if the potential is flatter than phi^2, resulting in the formation of non-topological…

High Energy Physics - Phenomenology · Physics 2009-10-31 K. Enqvist , A. Jokinen , J. McDonald

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

We perform a general algebraic analysis on the possibility of realising slow-roll inflation in the moduli sector of string models. This problem turns out to be very closely related to the characterisation of models admitting metastable…

High Energy Physics - Theory · Physics 2014-11-18 Laura Covi , Marta Gomez-Reino , Christian Gross , Jan Louis , Gonzalo A. Palma , Claudio A. Scrucca

We examine the constraints on F-term hybrid inflation by considering the flat directions in the Minimal Supersymmetric Standard Model (MSSM). We find that some coupling terms between the flat direction fields and the field which dominates…

High Energy Physics - Phenomenology · Physics 2008-11-26 Fuqiang Xu , Jin Min Yang

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 study in detail the possibility that the flat directions of the Minimal Supersymmetric Standard Model (MSSM) could act as a curvaton and generate the observed adiabatic density perturbations. For that the flat direction energy density…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kari Enqvist , Asko Jokinen , Shinta Kasuya , Anupam Mazumdar

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
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