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Related papers: Illustrating SUSY breaking effects on various infl…

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We consider dynamical models of supersymmetry breaking which naturally incorporate cosmological inflation. The inflaton plays an inevitable role in dynamical SUSY breaking and the hierarchical scales of inflation and SUSY breaking are…

High Energy Physics - Phenomenology · Physics 2009-10-30 K. -I. Izawa

We consider F-term hybrid inflation and supersymmetry breaking in the context of a model which largely respects a global U(1) R symmetry. The Kaehler potential parameterizes the Kaehler manifold with an enhanced U(1)_Rx(SU(1,1)/U(1))…

High Energy Physics - Phenomenology · Physics 2025-04-04 C. Pallis

We investigate the recently proposed class of chaotic inflation models in supergravity with an arbitrary inflaton potential. These models are extended to include matter fields in the visible sector and we employ a mechanism of SUSY breaking…

High Energy Physics - Theory · Physics 2013-05-29 Renata Kallosh , Andrei Linde , Keith A. Olive , Tomas Rube

In this paper, we study the inflection point inflation generated by a polynomial superpotential and a canonical K\"ahler potential under the supergravity framework, where only one chiral superfield is needed. We find that the special form…

High Energy Physics - Phenomenology · Physics 2025-10-09 Manuel Drees , Wenbin Zhao

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 study the conditions of restoring supersymmetry (SUSY) after inflation in the supergravity-based cosmological models with a single chiral superfield and a quartic stabilization term in the K\"ahler potential. Some new, explicit, and…

High Energy Physics - Theory · Physics 2016-08-09 Sergei V. Ketov , Takahiro Terada

We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in $N=1$ supergravity with the dilaton-axion chiral superfield $T$ in the presence of an $N=1$ vector multiplet with…

High Energy Physics - Theory · Physics 2019-08-28 Yermek Aldabergenov , Auttakit Chatrabhuti , Sergei V. Ketov

We go a step further in the search for a consistent and realistic supergravity model of large-field inflation by building a class of models with the following features: during slow-roll, all the scalar fields other than the inflaton are…

High Energy Physics - Theory · Physics 2015-06-23 Gianguido Dall'Agata , Fabio Zwirner

Effects of soft SUSY-breaking terms on inflation potentials are discussed. There exist generic constraints that must be satisfied in order not for the inflaton potential to loose its flatness. We examine explicitly the constraints in the…

High Energy Physics - Phenomenology · Physics 2009-11-07 Koshiro Suzuki , T. Watari

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 analyze the interplay between K\"ahler moduli stabilization and chaotic inflation in supergravity. While heavy moduli decouple from inflation in the supersymmetric limit, supersymmetry breaking generically introduces non-decoupling…

High Energy Physics - Theory · Physics 2015-06-23 Wilfried Buchmuller , Emilian Dudas , Lucien Heurtier , Alexander Westphal , Clemens Wieck , Martin Wolfgang Winkler

The slow roll inflation requires an extremely flat inflaton potential. The supersymmetry (SUSY) is not only motivated from the gauge hierarchy problem, but also from stabilizing that flatness of the inflaton potential against radiative…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Watari , T. Yanagida

The relation between the Hubble constant and the scale of supersymmetry breaking is investigated in models of inflation dominated by a string modulus. Usually in this kind of models the gravitino mass is of the same order of magnitude as…

High Energy Physics - Theory · Physics 2014-11-18 M. Badziak , M. Olechowski

We study the cosmology of a recent model of supersymmetry breaking, in the presence of a tuneable positive cosmological constant, based on a gauged shift symmetry of a string modulus that can be identified with the string dilaton. The…

High Energy Physics - Phenomenology · Physics 2016-12-20 I. Antoniadis , A. Chatrabhuti , H. Isono , R. Knoops

We argue that in the simplest version of the KKLT model, the maximal value of the Hubble constant during inflation cannot exceed the present value of the gravitino mass, H< m_{3/2}. This may have important implications for string cosmology…

High Energy Physics - Theory · Physics 2010-04-06 Renata Kallosh , Andrei Linde

Combination of Plank and BICEP2 data reported that tensor to scalar ratio $r\simeq 0.16$ and scalar spectral index $n_{s}\simeq 0.96$. In this short note, it is shown that chaotic inflation with quadratic potential, which perfectly accounts…

High Energy Physics - Phenomenology · Physics 2015-02-25 Sibo Zheng

The supergravity (SUGRA) theories with exact global $U(1)$ symmetry or shift symmetry in K\"ahler potential provide the natural frameworks for inflation. However, the quadratic inflation is disfavoured by the new results on primordial…

High Energy Physics - Phenomenology · Physics 2015-09-16 Tianjun Li , Zhijin Li , Dimitri V. Nanopoulos

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

We use a new mechanism for generating a Fayet-Iliopoulos term in supergravity, which is not associated to an R symmetry, to construct a semi-realistic theory of slow-roll inflation for a theory with the same K\"ahler potential and…

High Energy Physics - Theory · Physics 2021-05-14 Hun Jang , Massimo Porrati

Theories with elementary scalar degrees of freedom seem nowadays required for simple descriptions of the Standard Model and of the Early Universe. It is then natural to embed theories of inflation in supergravity, also in view of their…

High Energy Physics - Theory · Physics 2015-09-30 S. Ferrara , A. Sagnotti
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