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Related papers: Hybrid Inflation from Supergravity D Terms

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Realising $F$-term slow-roll inflation in supergravity is non-trivial due to the well-known $\eta$-problem. The common strategy to solve the problem is to impose a shift symmetry on the K\"ahler potential, but this often leads to a negative…

High Energy Physics - Theory · Physics 2025-12-15 Jinn-Ouk Gong , Sergei V. Ketov , Takahiro Terada

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

We elucidate the counting of the relevant small parameters in inflationary perturbation theory. Doing this allows for an explicit delineation of the domain of validity of the semi-classical approximation to gravity used in the calculation…

High Energy Physics - Theory · Physics 2018-02-21 Peter Adshead , C. P. Burgess , R. Holman , Sarah Shandera

We propose a new realisation of hybrid inflation in supergravity where the inflaton field does not appear in the superpotential but contributes only through the Kahler potential. The scalar potential derived from an R-invariant…

High Energy Physics - Phenomenology · Physics 2015-06-25 H. Boutaleb-J , A. Chafik , A. L. Marrakchi

We consider "new inflation" inflationary models at small fields, embedded in minimal ${\cal N}=1$ supergravity with a single chiral superfield. Imposing a period of inflation compatible with experiment severely restricts possible models,…

High Energy Physics - Theory · Physics 2016-10-12 Heliudson Bernardo , Horatiu Nastase

It is shown that racetrack inflation can be implemented in a moduli stabilisation scenario with a supersymmetric uplifting D-term. The resulting model is completely described by an effective supergravity theory, in contrast to the original…

High Energy Physics - Theory · Physics 2008-11-26 Philippe Brax , Anne-Christine Davis , Stephen C. Davis , Rachel Jeannerot , Marieke Postma

We study a $D$-term inflation scenario in a model extended from the minimal supersymmetric standard model (MSSM) by two additional abelian factor groups focussing on its particle physics aspects. Condensates of the fields related to the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Daijiro Suematsu

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

We present a superstring-inspired version of D-term inflation which does not lead to cosmic string formation and appears to satisfy the current CMB constraints. It differs from minimal D-term inflation by a second pair of charged…

High Energy Physics - Theory · Physics 2009-11-10 J. Urrestilla , A. Achucarro , A. C. Davis

The Hubble constant during the last stages of inflation in a broad class of models based on the KKLT mechanism should be smaller than the gravitino mass, H <~ m_{3/2}. We point out that in the models with large volume of compactification…

High Energy Physics - Theory · Physics 2009-09-29 Joseph P. Conlon , Renata Kallosh , Andrei Linde , Fernando Quevedo

We show that a non-minimal coupling to gravity can not only make some inflationary models consistent with cosmological data, similar to the case of Higgs inflation, but can also invoke slow-roll violation to realize graceful exit from…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-09 Tomo Takahashi , Tommi Tenkanen , Shuichiro Yokoyama

We study the dynamics of the standard model Higgs field in the inflationary cosmology. Since metastability of our vacuum is indicated by the current experimental data of the Higgs boson and top quark, inflation models with a large Hubble…

High Energy Physics - Phenomenology · Physics 2015-06-22 Kohei Kamada

We discuss inflation in models with large extra dimensions, driven by a bulk scalar field. The brane inflaton is then a single effective field, obtained from the bulk scalar field by scaling. The self interaction terms of the effective…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. N. Mohapatra , A. Pérez-Lorenzana , C. A. de S. Pires

We show that the recently proposed multi-natural inflation can be realized within the framework of 4D ${\cal N}=1$ supergravity. The inflaton potential mainly consists of two sinusoidal potentials that are comparable in size, but have…

High Energy Physics - Phenomenology · Physics 2014-06-09 Michael Czerny , Tetsutaro Higaki , Fuminobu Takahashi

We discuss the emergence of an inflationary phase in supergravity with the super-Higgs effect due to dynamical spontaneous breaking of supersymmetry, in which the role of the inflaton is played by the gravitino condensate. Realistic models…

High Energy Physics - Theory · Physics 2013-10-30 John Ellis , Nick E. Mavromatos

We discuss a realization of a small field inflation based on string inspired supergravities. In theories accompanying extra dimensions, compactification of them with small radii is required for realistic situations. Since the extra…

High Energy Physics - Theory · Physics 2017-08-01 Tetsutaro Higaki , Yoshiyuki Tatsuta

We study the effect of inflation on gaugino condensation in supergravity. Unless the Hubble scale H is significantly below the gaugino condensation scale, the gaugino condensate is a dynamical variable which cannot be integrated out. For a…

High Energy Physics - Theory · Physics 2010-02-01 Oleg Lebedev , Chloe Papineau , Marieke Postma

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

Whichever could be the real theory of gravitation, the corresponding low-energy effective lagrangian will probably contain higher derivative terms. In this work we study the general conditions on those terms in order to produce enough…

High Energy Physics - Phenomenology · Physics 2014-11-17 A. Dobado , A. Lopez

We describe methods for building "semi-realistic" models of F-term inflation. By semi-realistic we mean that they are built in, and obey the requirements of, "semi-realistic" particle physics models. The particle physics models are taken to…

High Energy Physics - Phenomenology · Physics 2008-11-26 Ben Kain
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