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Related papers: No-scale D-term inflation with stabilized moduli

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Inflation universally produces classical almost scale free Gaussian inhomogeneities of any light scalars. Assuming the coupling constants at the time of inflation depend on some light moduli fields, we encounter the generation of modulated…

Astrophysics · Physics 2009-11-10 Francis Bernardeau , Lev Kofman , Jean-Philippe Uzan

We assess the range of validity of sgoldstino-less inflation in a scenario of low energy supersymmetry breaking. We first analyze the consistency conditions that an effective theory of the inflaton and goldstino superfields should satisfy…

High Energy Physics - Theory · Physics 2017-08-10 Riccardo Argurio , Dries Coone , Lucien Heurtier , Alberto Mariotti

We discuss phenomenological aspects of no-scale supergravity inflationary models motivated by compactified string models, in which the inflaton may be identified either as a K\"ahler modulus or an untwisted matter field, focusing on models…

High Energy Physics - Phenomenology · Physics 2015-10-07 John Ellis , Marcos A. G. Garcia , Dimitri V. Nanopoulos , Keith A. Olive

In the presence of fields without superpotential but with large vevs through D-terms the mass-squared of the inflaton in the context of supergravity hybrid inflation receives positive contributions which could cancel the possibly negative…

High Energy Physics - Phenomenology · Physics 2009-10-31 C. Panagiotakopoulos

We review the realization of Starobinsky-type inflation within induced-gravity Supersymmetric (SUSY) and non-SUSY models. In both cases, inflation is in agreement with the current data and can be attained for subplanckian values of the…

High Energy Physics - Phenomenology · Physics 2017-06-20 C. Pallis , N. Toumbas

In the present paper, certain inflation models are shown to have large non-Gaussianity in special cases. Namely, finite length inflation models with an effective higher derivative interaction, in which slow-roll inflation is adopted as…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-26 Shiro Hirai , Tomoyuki Takami

We discuss a general bound on the possibility to realise inflation in any minimal supergravity with F-terms. The derivation crucially depends on the sGoldstini, the scalar field directions that are singled out by spontaneous supersymmetry…

High Energy Physics - Theory · Physics 2015-06-04 Andrea Borghese , Diederik Roest , Ivonne Zavala

The recently proposed trans-Planckian censorship conjecture (TCC) amounts to the claim that inflation models with an inflationary energy scale larger than Lambda_inf^max ~ 10^9 GeV belong to the swampland, i.e., cannot be embedded into a…

High Energy Physics - Phenomenology · Physics 2020-03-05 Kai Schmitz

An inflationary stage dominated by a $D$-term avoids the slow-roll problem of inflation in supergravity and may emerge in theories with a non-anomalous or anomalous U(1) gauge symmetry. The most intriguing and commonly invoked possibility…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. R. Espinosa , A. Riotto , G. G. Ross

Chaotic inflation predicts a large gravitational wave signal which can be tested by the upcoming Planck satellite. We discuss a SUGRA implementation of chaotic inflation in the presence of moduli fields, and find that inflation does not…

High Energy Physics - Phenomenology · Physics 2008-11-26 Stephen C. Davis , Marieke Postma

As a first step towards inflation in genuinely F-theoretic setups, we propose a scenario where the inflaton is the relative position of two 7-branes on holomorphic 4-cycles. Non-supersymmetric gauge flux induces an attractive inter-brane…

High Energy Physics - Theory · Physics 2013-02-27 Arthur Hebecker , Sebastian C. Kraus , Dieter Lust , Stephan Steinfurt , Timo Weigand

We analyze the cosmological consequences of locked inflation, a model recently proposed by Dvali and Kachru that can produce significant amounts of inflation without requiring slow-roll. We pay particular attention to the end of inflation…

High Energy Physics - Theory · Physics 2009-11-10 Richard Easther , Justin Khoury , Koenraad Schalm

We consider a supersymmetric hybrid inflation in the framework of the Randall-Sundrum type II Braneworld model. We drive an analytical expression for the scalar potential and find that the F-term dominates hybrid inflation process. We show…

General Relativity and Quantum Cosmology · Physics 2010-10-28 A. Bouaouda , R. Zarrouki , H. Chakir , M. Bennai

We consider a class of well motivated supersymmetric models of F-term hybrid inflation (FHI) which can be linked to the supersymmetric grand unification. The predicted scalar spectral index n_s cannot be smaller than 0.97 and can exceed…

High Energy Physics - Phenomenology · Physics 2010-01-26 C. Pallis

We revisit some questions in supersymmetric hybrid inflation (SHI). We analyze the amount of fine tuning required in various models, the problem of decay at the end of inflation and the generation of baryons after inflation. We find that…

High Energy Physics - Phenomenology · Physics 2009-11-10 Micha Berkooz , Michael Dine , Tomer Volansky

In models of cosmological inflation motivated by dynamical supersymmetry breaking, the potential driving inflation may be characterized by inverse powers of a scalar field. These models produce observables similar to those typical of the…

High Energy Physics - Phenomenology · Physics 2009-10-31 William H. Kinney , Antonio Riotto

Hybrid inflation is a natural scenario in the absence of supersymmetry. In the context of supergravity, however, it has to face the naturalness problems of the initial conditions and of the adequate suppression of the inflaton mass. Both…

High Energy Physics - Phenomenology · Physics 2007-05-23 C. Panagiotakopoulos

A scheme of simplified smooth hybrid inflation is realized in the framework of supersymmetric $SU(5)$. The smooth model of hybrid inflation provides a natural solution to the monopole problem that appears in the breaking of $SU(5)$ gauge…

High Energy Physics - Phenomenology · Physics 2017-10-06 Mansoor Ur Rehman , Umer Zubair

We perform the complete stability study of the model of chromo-natural inflation (Adshead and Wyman '12), where, due to its coupling to a SU(2) vector, a pseudo-scalar inflaton chi slowly rolls on a steep potential. As a typical example,…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-15 Emanuela Dimastrogiovanni , Marco Peloso

The simple chaotic inflation is highly consistent with the BICEP2 experiment, and no-scale supergravity can be realized naturally in various string compactifications. Thus, we construct a chaotic inflation model in no-scale supergravity…

High Energy Physics - Theory · Physics 2015-06-19 Tianjun Li , Zhijin Li , Dimitri V. Nanopoulos
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