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Related papers: Chaotic Inflation from the MSSM Along Flat $D$-Ter…

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The inflation within the MSSM is proposed, where the inflaton field is a combination of the Higgs, squark and slepton states. While the inflationary phase is fully governed by the electron Yukawa superpotential coupling, the fields'…

High Energy Physics - Phenomenology · Physics 2020-04-01 Zurab Tavartkiladze

We show that the seesaw mechanism as well as leptogenesis are natural outcomes of a viable chaotic inflation in supergravity. The inflation model contains two superfields, the inflaton and stabilizer fields, which, being singlets under the…

High Energy Physics - Phenomenology · Physics 2016-03-23 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We construct a chaotic inflation model in which the Higgs fields play the role of the inflaton in the standard model as well as in the singlet extension of the supersymmetric standard model. The key idea is to allow a non-canonical kinetic…

High Energy Physics - Phenomenology · Physics 2011-02-15 Kazunori Nakayama , Fuminobu Takahashi

We consider a phenomenological extension of the minimal supersymmetric standard model which incorporates chaotic inflation and a radiatively generated intermediate mass scale. Initially a period of chaotic inflation is driven by a quartic…

High Energy Physics - Phenomenology · Physics 2009-10-28 Tony Gherghetta , Gordon L. Kane

We present a general polynomial chaotic inflation model in supergravity, for which the predicted spectral index and tensor-to-scalar ratio can lie within the 1 sigma region allowed by the Planck results. Most importantly, the predicted…

High Energy Physics - Phenomenology · Physics 2015-06-16 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We consider D-term inflation for small couplings of the inflaton to matter fields. Standard hybrid inflation then ends at a critical value of the inflaton field that exceeds the Planck mass. During the subsequent waterfall transition the…

High Energy Physics - Phenomenology · Physics 2015-06-22 W. Buchmuller , V. Domcke , K. Schmitz

A simple model for chaotic inflation in supergravity is proposed. The model is N=1 supersymmetric massive U(1) gauge theory via the Stuckelberg superfield and gives rise to D-term inflation with a quadratic term of inflaton in the…

High Energy Physics - Theory · Physics 2008-12-23 Teruhiko Kawano

We consider the possibility of using one of the $D$-flat directions in the minimal supersymmetric standard model (MSSM) as the inflaton. We show that the flat direction consisting of (first generation) left- and right-handed up-squarks as…

High Energy Physics - Phenomenology · Physics 2014-11-17 Shinta Kasuya , Takeo Moroi , Fuminobu Takahashi

We consider chaotic inflation models with a pseudo-scalar field containing the general couplings to the four-form flux. The four-form mixing with the pseudo-scalar field induces a quadratic potential for inflaton while the coexisting…

High Energy Physics - Phenomenology · Physics 2020-02-26 Hyun Min Lee

We propose a modification to the standard hybrid inflation model \cite{Linde:1993cn}, that connects a successful hybrid inflation scenario to the standard model Higgs sector, via the electroweak vacuum stability. The proposed model results…

High Energy Physics - Phenomenology · Physics 2023-02-23 Merna Ibrahim , Mustafa Ashry , Esraa Elkhateeb , Adel M. Awad , Ahmad Moursy

A simple extension of the minimal left-right symmetric supersymmetric grand unified theory model is constructed by adding two pairs of superfields. This naturally violates the partial Yukawa unification predicted by the minimal model. After…

High Energy Physics - Phenomenology · Physics 2014-03-26 R. Armillis , G. Lazarides , C. Pallis

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

We discuss the constraints on the inhomogeneous reheating scenario. In particular, we discuss the prospects for low scale inflation with a Hubble constant of the order of the gravitino mass, and the possibility that an MSSM flat direction…

Astrophysics · Physics 2009-11-10 Marieke Postma

We propose that inflation is driven by a (complex) neutral Higgs of the MSSM extension of the SM, in a chaotic-like inflation setting. The SUSY breaking soft term masses are of order $10^{12}-10^{13}$ GeV, which is identified with the…

High Energy Physics - Theory · Physics 2015-06-23 Luis E. Ibanez , Fernando Marchesano , Irene Valenzuela

The measurements of the Higgs mass and top Yukawa coupling indicate that we live in a very special Universe, at the edge of the absolute stability of the electroweak vacuum. If fully stable, the Standard Model (SM) can be extended all the…

High Energy Physics - Phenomenology · Physics 2015-10-27 Fedor Bezrukov , Javier Rubio , Mikhail Shaposhnikov

A single field inflation based on a supergravity model with a shift symmetry and $U(1)$ extension of the MSSM is analyzed. We show that one of the real components of the two $U(1)$ charged scalar fields plays the role of inflaton {with} an…

High Energy Physics - Phenomenology · Physics 2015-10-28 Lucien Heurtier , Shaaban Khalil , Ahmad Moursy

We study chaotic inflation driven by a real, massive, homogeneous minimally coupled scalar field in a flat Robertson-Walker spacetime. The semiclassical limit for gravity is considered, whereas the scalar field is treated quantum…

General Relativity and Quantum Cosmology · Physics 2008-11-26 F. Finelli , G. P. Vacca , G. Venturi

We show, within the single-field inflationary paradigm, that a linear non-minimal interaction $\xi\,M_P\,\phi\,R$ between the inflaton field $\phi$ and the Ricci scalar $R$ can result in successful inflation that concludes with an efficient…

High Energy Physics - Phenomenology · Physics 2024-04-18 Basabendu Barman , Nicolás Bernal , Javier Rubio

In the framework of MSSM inflation, matter and gravitino production are here investigated through the decay of the fields which are coupled to the udd inflaton, a gauge invariant combination of squarks. After the end of inflation, the flat…

High Energy Physics - Phenomenology · Physics 2017-10-31 Andrea Ferrantelli

We study the inflation due to the D-flat direction of an extra $U(1)$. This scenario is a hybrid of a right-handed sneutrino inflaton scenario and a gauge non-singlet inflaton scenario. The inflaton is a gauge non-singlet field which…

High Energy Physics - Phenomenology · Physics 2009-10-28 Daijiro Suematsu , Yoshio Yamagishi
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