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Related papers: D-term chaotic inflation in supergravity

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We revisit the D-term inflation and amend it with ghost-free higher derivative couplings of chiral superfields to super-curvature. These couplings realize a more generic inflationary phase in supergravity. After pointing out that a…

High Energy Physics - Theory · Physics 2015-06-19 Iannis Dalianis , Fotis Farakos

We propose a chaotic inflation model in supergravity based on polynomial interactions of the inflaton. Specifically we study the chaotic inflation model with quadratic, cubic and quartic couplings in the scalar potential and show that the…

High Energy Physics - Phenomenology · Physics 2015-06-15 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We show that inflation which is dominated by the D-term density avoids the `slow-roll' problem of inflation in supergravity. Such an inflationary scenario can naturally emerge in theories with non-anomalous or anomalous U(1) gauge symmetry.…

High Energy Physics - Phenomenology · Physics 2009-10-28 Pierre Binetruy , Gia Dvali

We have constructed a large field N-flation model in the supergravity framework. In this simple set-up, N fields collectively drive inflation where each field traverses sub-Planckian field values. This has been realised with a…

High Energy Physics - Phenomenology · Physics 2015-12-30 Kumar Das , Koushik Dutta

D-term inflation is one of the most interesting and versatile models of inflation. It is possible to implement naturally D-term inflation within high energy physics, as for example SUSY GUTs, SUGRA, or string theories. D-term inflation…

High Energy Physics - Theory · Physics 2009-11-11 Jonathan Rocher , Mairi Sakellariadou

Hybrid inflation, driven by a Fayet-Iliopoulos (FI) D term, is an intriguing inflationary model. In its usual formulation, it however suffers from several shortcomings. These pertain to the origin of the FI mass scale, the stability of…

High Energy Physics - Phenomenology · Physics 2018-06-29 Valerie Domcke , Kai Schmitz

We study models of hybrid inflation in the framework of supergravity with superconformal matter. F-term hybrid inflation is not viable since the inflaton acquires a large tachyonic mass. On the contrary, D-term hybrid inflation can…

High Energy Physics - Phenomenology · Physics 2015-06-11 W. Buchmüller , V. Domcke , K. Schmitz

We propose a natural double inflation model in supergravity. In this model, chaotic inflation first takes place by virtue of the Nambu-Goldstone-like shift symmetry, which guarantees the absence of the exponential factor in the potential…

High Energy Physics - Phenomenology · Physics 2009-11-07 Masahide Yamaguchi

We propose a new model of the D-term hybrid inflation in the framework of supergravity. Although our model introduces, analogously to the conventional D-term inflation, the inflaton and a pair of scalar fields charged under a $U(1)$ gauge…

High Energy Physics - Phenomenology · Physics 2017-12-06 Kenji Kadota , Tatsuo Kobayashi , Keigo Sumita

We consider hybrid inflation in the braneworld scenario. In particular, we consider inflation in global supersymmetry with the D-terms in the scalar potential for the inflaton field to be the dominant ones (D-term inflation). We find that…

High Energy Physics - Phenomenology · Physics 2009-11-11 G. Panotopoulos

We consider D-term hybrid inflation in the framework of superconformal supergravity. In part of the parameter space, inflation continues for subcritical inflaton field value. Consequently, a new type of inflation emerges, which gives…

Cosmology and Nongalactic Astrophysics · Physics 2018-06-04 Koji Ishiwata

We show how we can implement chaotic inflation in the context of supergravity by conveniently selecting the functional form of a strong enough non-minimal coupling between the inflaton and the Ricci scalar curvature. The procedure can be…

High Energy Physics - Phenomenology · Physics 2014-12-12 C. Pallis

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

An inflationary stage dominated by a D-term avoids the slow-roll problem of inflation in supergravity and can naturally emerge in theories with a non-anomalous or anomalous U(1) gauge symmetry. In the latter case, however, the scale of…

High Energy Physics - Phenomenology · Physics 2009-10-30 D. H. Lyth , A. Riotto

We argue that there may arise a relatively flat inflaton potential over super-Planckian field values with an approximate shift symmetry, if the coefficients of the kinetic terms for many singlet scalars are subject to a certain random…

High Energy Physics - Phenomenology · Physics 2015-06-22 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We discuss the general structure and observational consequences of some of the simplest versions of chaotic inflation in supergravity in relation to the data by Planck 2013 and BICEP2. We show that minimal modifications to the simplest…

High Energy Physics - Theory · Physics 2014-08-06 Renata Kallosh , Andrei Linde , Alexander Westphal

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

We present a model of slow-roll inflation in the context of effective Supergravities arising from string theories. The uplifting of the potential (to generate dS or Minkowski vacua) is provided by the D-term associated to an anomalous U(1),…

High Energy Physics - Theory · Physics 2009-11-13 B. de Carlos , J. A. Casas , A. Guarino , J. M. Moreno , O. Seto

We review the main aspects of the warm inflation scenario, focusing on the inflationary dynamics and the predictions related to the primordial spectrum of perturbations, to be compared with the recent cosmological observations. We study in…

High Energy Physics - Phenomenology · Physics 2010-04-21 Mar Bastero-Gil , Arjun Berera

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