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We study models of inflation where the inflaton corresponds to a flat direction in field space and its mass term is generated by gravity mediated soft supersymmetry breaking at high scale. Assuming the inflaton to have non negligible…

High Energy Physics - Phenomenology · Physics 2007-05-23 Laura Covi

Processes of particle production during inflation can increase the amplitude of the scalar metric perturbations. We show that such a mechanism can naturally arise in supergravity models where an axion-like field, whose potential is…

High Energy Physics - Phenomenology · Physics 2021-07-07 Michael A. Roberts , Lorenzo Sorbo

Supersymmetric theories in 5d orbifold can have Fayet-Iliopoulos (FI) terms on the boundaries. These terms induce a 5d mass for the bulk matter fields. We analyze this effect using N=1 superfields and show how it can be understood as a…

High Energy Physics - Phenomenology · Physics 2009-11-07 Daniel Marti , Alex Pomarol

We present novel realizations of E-model inflation within Supergravity which are largely associated with the existence of a pole of order one in the kinetic term of the (gauge-singlet) inflaton superfield. This pole arises due to the…

High Energy Physics - Phenomenology · Physics 2022-06-01 C. Pallis

The slow-roll inflation is a beautiful paradigm, yet the inflaton potential can hardly be sufficiently flat when unknown gravitational effects are taken into account. However, the hybrid inflation models constructed in D = 4 N = 1…

High Energy Physics - Theory · Physics 2014-11-18 Fumikazu Koyama , Yuji Tachikawa , Taizan Watari

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 draw attention to the possibility that inflation (i.e. accelerated expansion) might continue after the end of slow roll, during a period of fast oscillations of the inflaton field \phi . This phenomenon takes place when a mild…

General Relativity and Quantum Cosmology · Physics 2009-10-30 Thibault Damour , Viatcheslav F. Mukhanov

We define a new inflationary scenario in which inflation starts naturally after the Big Bang when the energy density drops below some critical value. As a model, we use recently proposed symmetron field whose effective potential depends on…

Cosmology and Nongalactic Astrophysics · Physics 2014-04-02 Ruifeng Dong , William H. Kinney , Dejan Stojkovic

We show that in string theory or supergravity with supersymmetry breaking through combined F-terms and Fayet-Iliopoulos D-terms, the masses for charged scalars and fermions can be hierarchically split. The mass scale for the gauginos and…

High Energy Physics - Theory · Physics 2010-04-05 Boris Kors , Pran Nath

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 study inflation driven by a slow-rolling inflaton field, characterised by a quadratic potential, and incorporating radiative corrections within the context of supergravity. In this model the energy scale of inflation is not overly…

High Energy Physics - Phenomenology · Physics 2011-02-16 Gabriel German , Graham Ross , Subir Sarkar

We present novel realizations of E- and T-model inflation within Supergravity which are largely associated with the existence of a pole of order one and two respectively in the kinetic term of the inflaton superfield. This pole arises due…

High Energy Physics - Phenomenology · Physics 2022-12-06 C. Pallis

Inflation is well known to be difficult in the context of supergravity, if the potential is dominated by the $F$ term. Non-renormalizable terms generically give $|V''|\sim V/M^2$, where $V(\phi)$ is the inflaton potential and $M$ is the…

High Energy Physics - Phenomenology · Physics 2009-10-30 David Lyth

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

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

We show how we can implement within Supergravity chaotic inflation in the presence of a pole of order one or two in the kinetic mixing of the inflaton sector. This pole arises due to the selected logarithmic Kahler potentials K, which…

High Energy Physics - Phenomenology · Physics 2022-11-28 C. Pallis

We extend a recently proposed framework, dubbed inflation by supersymmetry breaking, to hybrid inflation by introducing a waterfall field that allows to decouple the supersymmetry breaking scale in the observable sector from the inflation…

High Energy Physics - Theory · Physics 2025-12-16 Yermek Aldabergenov , Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono

The continuous shift symmetry of axions is at the heart of several realizations of inflationary models. In particular, axion monodromy inflation aims at achieving super-Planckian field ranges for the inflaton in the context of string…

High Energy Physics - Theory · Physics 2014-11-05 Fernando Marchesano , Gary Shiu , Angel M. Uranga

The three-year data from WMAP are in stunning agreement with the simplest possible quadratic potential for chaotic inflation, as well as with new or symmetry-breaking inflation. We investigate the possibilities for incorporating these…

High Energy Physics - Theory · Physics 2009-11-11 J. Ellis , Z. Lalak , S. Pokorski , K. Turzynski

We describe the coupling of matter fields to an inflationary sector of supergravity, the inflaton $\Phi$ and a stabilizer $S$, in models where the Kahler potential has a flat inflaton direction. Such models include, in particular, advanced…

High Energy Physics - Theory · Physics 2016-04-11 Renata Kallosh , Andrei Linde , Timm Wrase
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