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By using a No-Scale Supergravity model, which was proved to explain WMAP observations appropriately, a mechanism of supersymmetry breaking and a preheating just after the end of inflation are investigated. Non-thermal production rate of…

High Energy Physics - Phenomenology · Physics 2010-01-29 Kenji Takagi , Yuta Koshimizu , Toyokazu Fukuoka , Takao Sakai , Hikoya Kasari , Mitsuo J. Hayashi

We have investigated moduli stabilization leading to hierarchical supersymmetry breakdown in racetrack models with two moduli fields simultaneously present in the effective racetrack superpotential. We have shown that stabilization of…

High Energy Physics - Phenomenology · Physics 2009-11-07 Rafal Ciesielski , Zygmunt Lalak

We propose an inflationary scenario where the inflaton field is non-minimally coupled to spacetime curvature and inflation is driven by a vacuum energy symmetry breaking potential without specifying \emph{a priori} whether the inflaton…

General Relativity and Quantum Cosmology · Physics 2024-06-04 Alessio Belfiglio , Youri Carloni , Orlando Luongo

We consider a supersymmetric hybrid inflation model with two inflaton fields. The superpotential during inflation is dominated by W=(\kappa S+\kappa' S')M^2, where S, S' are inflatons carrying the same U(1)_R charge, \kappa, \kappa' are…

High Energy Physics - Phenomenology · Physics 2015-05-14 Bumseok Kyae

Supergravity provides the natural supersymmetric framework for early universe cosmology. A broad class of inflationary models in no-scale supergravity yields tree-level predictions for cosmic microwave background (CMB) observables that…

High Energy Physics - Phenomenology · Physics 2026-03-04 John Ellis , Tony Gherghetta , Kunio Kaneta , Wenqi Ke , Keith A. Olive

We consider the abundance of gravitinos created from the vacuum fluctuation, in a class of `new' inflation models for which global supersymmetry is a good approximation. Immediately after inflation, gravitinos are produced, with number…

High Energy Physics - Phenomenology · Physics 2009-10-31 David H Lyth

We present $\mathcal{N}=1$ supergravity models of mutated hilltop inflation (MHI) for both large and small field sectors. Models with canonical kinetic terms are developed based on a shift symmetric K\"ahler potential in inflaton…

High Energy Physics - Theory · Physics 2019-08-02 Tony Pinhero , Supratik Pal

In this paper, we employ the Palatini formalism to investigate the dynamics of large-field inflation using a renormalizable polynomial inflaton potential in the context of $f(R,\phi)$ gravity. Assuming instant reheating, we make a…

Cosmology and Nongalactic Astrophysics · Physics 2025-02-20 Nilay Bostan , Canan Karahan , Ozan Sargın

We present a unified model where the same scalar field can drive inflation and account for the present dark matter abundance. This scenario is based on the incomplete decay of the inflaton field into right-handed neutrino pairs, which is…

High Energy Physics - Phenomenology · Physics 2025-02-14 Antonio Torres Manso , Joao G. Rosa

The shortcomings of the Standard Big Bang Cosmological Model as well as their resolution in the context of inflationary cosmology are discussed. The inflationary scenario and the subsequent oscillation and decay of the inflaton field are…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Lazarides

We utilize a recently proposed cubic nilpotent superfield to realize inflation in supergravity with the minimal degrees of freedom: the inflaton, graviton, and massive gravitino. As an advantage, the resultant model is free from the…

High Energy Physics - Theory · Physics 2021-06-30 Takahiro Terada

We analyse the consequences of a new gauge invariant Fayet-Iliopoulos (FI) term proposed recently to a class of inflation models driven by supersymmetry breaking with the inflaton being the superpartner of the goldstino. We first show that…

High Energy Physics - Theory · Physics 2018-06-19 Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono , Rob Knoops

An alternative inflationary model is proposed predicated upon a consideration of the form of the uncertainty principle in a curved background spacetime. An argument is presented suggesting a possible curvature dependence in the correct…

General Relativity and Quantum Cosmology · Physics 2014-05-12 Paul J. Camp , John L. Safko

The simplicity of the CMB data, so well described by single-field inflation, raises the question whether there might be an equally simple multi-field realization consistent with the observations. We explore the idea that an approximate…

High Energy Physics - Theory · Physics 2019-07-04 Ana Achucarro , Yvette Welling

We propose a modification on the super-potential of (arXiv: 1901.09046) which discusses the simplest construction of inflationary $\alpha$ attractor models (also called T/E models) in supergravity without the sinflaton. This can make all…

High Energy Physics - Phenomenology · Physics 2020-12-09 Ping Kwan Man Ellgan

In F-term supergravity inflation models, scalar fields other than the inflaton generically receive a Hubble induced mass, which may restore gauge symmetries during inflation and phase transitions may occur during or after inflation as the…

High Energy Physics - Phenomenology · Physics 2013-05-30 Kohei Kamada , Kazunori Nakayama , Jun'ichi Yokoyama

We propose a cosmological framework in which neutrino masses evolve dynamically through coupling with a scalar field that simultaneously drives inflation. The neutrino mass is modeled as a power-law, exponential, or hybrid function of the…

Cosmology and Nongalactic Astrophysics · Physics 2025-12-01 Hemanshi Bundeliya , Gaurav Bhandari , S. D. Pathak , V. K. Sharma

It has been argued that supergravity models of inflation with vanishing sound speeds, $c_s$, lead to an unbounded growth in the production rate of gravitinos. We consider several models of inflation to delineate the conditions for which…

High Energy Physics - Theory · Physics 2021-06-16 Emilian Dudas , Marcos A. G. Garcia , Yann Mambrini , Keith A. Olive , Marco Peloso , Sarunas Verner

We study multifield inflation in scenarios where the fields are coupled non-minimally to gravity via $\xi_I(\phi^I)^n g^{\mu\nu}R_{\mu\nu}$, where $\xi_I$ are coupling constants, $\phi^I$ the fields driving inflation, $g_{\mu\nu}$ the…

Cosmology and Nongalactic Astrophysics · Physics 2018-06-29 Pedro Carrilho , David Mulryne , John Ronayne , Tommi Tenkanen

We discuss how the inflation induced supersymmetry breaking affects the flat directions of SUSY vacua. We show that under general assumptions all gauge nonsinglet fields, parameterizing flat directions (and in particular squarks and…

High Energy Physics - Phenomenology · Physics 2016-09-01 Gia Dvali