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Related papers: Supersymmetric Tuned Inflation

200 papers

Models of cosmological inflation resembling the Starobinsky R + R^2 model emerge naturally among the effective potentials derived from no-scale SU(N,1)/SU(N) x U(1) supergravity when N > 1. We display several examples in the SU(2,1)/SU(2) x…

High Energy Physics - Theory · Physics 2015-06-16 John Ellis , Dimitri V. Nanopoulos , Keith A. Olive

We discuss the possibility that inflation is driven by the sgoldstino, the superpartner of the goldstino. Unlike in generic supergravity scenarios, the sgoldstino decouples from all other fields in the theory, which allows for a simple and…

High Energy Physics - Theory · Physics 2013-12-03 Ana Achúcarro , Sander Mooij , Pablo Ortiz , Marieke Postma

In the present thesis, using an effective field theory point of view, we explore theories of single-field inflation where higher derivative operators become relevant, affecting in a novel way the dynamics and therefore the observations. For…

High Energy Physics - Theory · Physics 2016-12-06 Luca Santoni

We consider gravitationally induced corrections to inflaton potentials driven by supersymmetry breaking in a five-dimensional supergravity, compactified on a $ S_1/Z_2 $ orbifold. The supersymmetry breaking takes place on the hidden brane…

High Energy Physics - Theory · Physics 2024-12-10 G. A. Diamandis , K. Kaskavelis , A. B. Lahanas , G. Pavlopoulos

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

Heavy scalar fields can undergo an instability during inflation as a result of their kinetic couplings with the inflaton. This is known as the geometrical destabilization of inflation, as it relies on the effect of the negative curvature of…

Cosmology and Nongalactic Astrophysics · Physics 2018-11-07 Sebastian Garcia-Saenz , Sébastien Renaux-Petel , John Ronayne

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

Cosmological inflation gives a natural answer for a variety of cosmological questions, including the horizon problem, the flatness problem, and others. However, inflation yields new questions relating to the flatness of the inflaton…

High Energy Physics - Phenomenology · Physics 2009-11-10 David E. Kaplan , Neal Weiner

We review the effects of heavy scalar fields during inflation in the framework of $\mathcal N = 1$ supergravity. Such heavy scalars can be geometric moduli from string compactifications or stabilizer fields from a different sector of the…

High Energy Physics - Theory · Physics 2015-11-12 Emilian Dudas , Clemens Wieck

Moduli fields, which parameterize perturbative flat directions of the potential in supersymmetric theories, are natural candidates to act as inflatons. An inflationary potential on moduli space can result if the scale of dynamical SUSY…

High Energy Physics - Theory · Physics 2009-10-28 Scott Thomas

The positive potential energy required for inflation spontaneously breaks supersymmetry and in general gives any would-be inflaton an effective mass of order the inflationary Hubble parameter thus ruling it out as an inflaton. In this paper…

High Energy Physics - Phenomenology · Physics 2009-10-28 Ewan D. Stewart

It is shown that in the phenomenologically realistic supersymmetric $B-L$ MSSM theory, a linear combination of the neutral, up Higgs field with the third family left-and right-handed sneutrinos can play the role of the cosmological…

High Energy Physics - Phenomenology · Physics 2017-02-15 Rehan Deen , Burt A. Ovrut , Austin Purves

Recently it was found that a broad class of existing inflationary models based on supergravity can be significantly simplified if some of the standard, unconstrained chiral superfields are replaced by nilpotent superfields, associated with…

High Energy Physics - Theory · Physics 2015-06-22 Renata Kallosh , Andrei Linde

Low scale inflation has many virtues and it has been claimed that its natural realisation in supersymmetric standard model can be achieved rather easily. In this letter we have demonstrated that also in this case the dynamics of the hidden…

High Energy Physics - Theory · Physics 2008-11-26 Z. Lalak , K. Turzynski

It has been shown that hybrid inflation may end with the formation of non-topological solitons of inflaton field. As a first step towards a fully realistic picture of the post-inflation era and reheating in supersymmetric hybrid inflation…

High Energy Physics - Phenomenology · Physics 2009-11-10 Matt Broadhead , John McDonald

We present the supersymmetric extension of the unified model for inflation and Dark Matter studied in Ref. arXiv:1811.02302. The scenario is based on the incomplete decay of the inflaton field into right-handed (s)neutrino pairs. By…

High Energy Physics - Phenomenology · Physics 2025-02-14 Mar Bastero-Gil , António Torres Manso

We consider the torsional completion of gravity with spinor and scalar fields: we show how in this environment conditions of extreme symmetry or specific approximations imply the scalar field to be constant, so that slow-roll takes place…

General Relativity and Quantum Cosmology · Physics 2017-07-07 Luca Fabbri

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

The generic embedding of the $R+R^2$ higher curvature theory into old-minimal supergravity leads to models with rich vacuum structure in addition to its well-known inflationary properties. When the model enjoys an exact R-symmetry, there is…

High Energy Physics - Theory · Physics 2015-06-23 I. Dalianis , F. Farakos , A. Kehagias , A. Riotto , R. von Unge

In this paper we show that the new approach to the embedding of the inflationary potentials into supergravity, presented in a quite recent paper [11] of Ferrara, Kallosh, Linde and Porrati can be formulated within the framework of standard…

High Energy Physics - Theory · Physics 2016-01-20 P. Fre , A. S. Sorin