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By using a No-Scale Supergravity model, which was proved well to explain WMAP observations appropriately, a mechanism of preheating just after the end of inflation is investigated. By using the canonically normalized and diagonalized…

High Energy Physics - Phenomenology · Physics 2010-03-03 Yuta Koshimizu , Toyokazu Fukuoka , Kenji Takagi , Hikoya Kasari , Mitsuo J. Hayashi

We explore the possibility that inflation is driven by supersymmetry breaking with the superpartner of the goldstino (sgoldstino) playing the role of the inflaton. Moreover, we impose an R-symmetry that allows to satisfy easily the…

High Energy Physics - Theory · Physics 2017-11-22 Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono , Rob Knoops

A small tensor-to-scalar ratio $r$ may lead to distinctive phenomenology of high-scale supersymmetry. Assuming the same origin of SUSY breaking between the inflation and visible sector, we show model independent features. The simplest…

High Energy Physics - Phenomenology · Physics 2015-08-26 Sibo Zheng

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

We analyse the reheating in the modification of \nuMSM (Standard Model with three right handed neutrinos with masses below the electroweak scale) where the sterile neutrino providing the Dark Matter is generated in decays of the additional…

High Energy Physics - Phenomenology · Physics 2009-01-14 Alexey Anisimov , Yannick Bartocci , Fedor L. Bezrukov

We consider F-term hybrid inflation and supersymmetry breaking in the context of a model which largely respects a global U(1) R symmetry. The Kaehler potential parameterizes the Kaehler manifold with an enhanced U(1)x(SU(1,1)/U(1))…

High Energy Physics - Phenomenology · Physics 2023-12-05 G. Lazarides , C. Pallis

Motivated by Refs \cite{am1,am2}, we analyze how the inflaton decay reheats the Universe within supersymmetry. In a non-supersymmetric case the inflaton usually decays via preheating unless its couplings to other fields are very small.…

High Energy Physics - Phenomenology · Physics 2008-11-26 Rouzbeh Allahverdi , Anupam Mazumdar

We consider $R^2$ inflation in the Palatini gravity assuming the existence of scalar fields, coupled to gravity in the most general manner. These theories, in the Einstein frame, and for one scalar field $h$, share common features with $K$…

General Relativity and Quantum Cosmology · Physics 2020-04-08 Ioannis D. Gialamas , A. B. Lahanas

By using a string-inspired modular invariant supergravity, which was proved well to explain WMAP observations appropriately, a mechanism of supersymmetry breaking (SSB) and Gravitino Production just after the end of inflation are…

High Energy Physics - Phenomenology · Physics 2010-03-17 Kenji Takagi , Yuta Koshimizu , Toyokazu Fukuoka , Hikoya Kasari , Mitsuo J. Hayashi

A {\it gauge invariant} combination of LLe {\it sleptons} within the Minimal Supersymmetric Standard Model is one of the few inflaton candidates that can naturally explain population of the observable sector and creation of matter after…

High Energy Physics - Phenomenology · Physics 2015-03-19 Rouzbeh Allahverdi , Andrea Ferrantelli , Juan Garcia-Bellido , Anupam Mazumdar

We present the supersymmetric extension of the unified model for inflation and Dark Matter studied in Ref. arXiv:1811.02302. The scenario is based on the incomplete decay of the inflaton field into right-handed (s)neutrino pairs. By…

High Energy Physics - Phenomenology · Physics 2025-02-14 Mar Bastero-Gil , António Torres Manso

We study a recently proposed running kinetic inflation model in which the inflaton potential becomes flat due to rapid growth of the kinetic term at large inflaton field values. As concrete examples, we build a variety of chaotic inflation…

High Energy Physics - Phenomenology · Physics 2010-12-09 Kazunori Nakayama , Fuminobu Takahashi

We point out some of the outstanding challenges for embedding inflationary cosmology within string theory studying the process of reheating for models where the inflaton is a closed string mode parameterising the size of an internal cycle…

High Energy Physics - Theory · Physics 2011-05-31 Michele Cicoli , Anupam Mazumdar

We reconsider a class of well motivated supersymmetric models in which inflation is associated with the breaking of a gauge symmetry G to H, with the symmetry breaking scale M~10^16 GeV. Starting with a renormalizable superpotential, we…

High Energy Physics - Phenomenology · Physics 2008-11-26 V. N. Senoguz , Q. Shafi

We study reheating processes and its cosmological consequences in the Starobinsky model embedded in the old-minimal supergravity. First, we consider minimal coupling between the gravity and matter sectors in the higher curvature theory, and…

High Energy Physics - Phenomenology · Physics 2015-06-23 Takahiro Terada , Yuki Watanabe , Yusuke Yamada , Jun'ichi Yokoyama

The flat directions LLe and udd within the minimal supersymmetric Standard Model provide all the necessary ingredients for a successful inflation with the right amplitude of the scalar density perturbations, negligible gravity waves and the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Rouzbeh Allahverdi , Bhaskar Dutta , Anupam Mazumdar

No-scale supergravity and the flipped SU(5)$\times$U(1) gauge group provide an ambitious prototype string-inspired scenario for physics below the string scale, which can accommodate the Starobinsky-like inflation favoured by observation…

High Energy Physics - Phenomenology · Physics 2019-04-17 John Ellis , Marcos A. G. Garcia , Natsumi Nagata , Dimitri V. Nanopoulos , Keith A. Olive

A variant of hybrid inflation which is applicable in a wide class of supersymmetric grand unified models and reproduces the observed temperature perturbations of cosmic background radiation with natural values of the parameters is…

High Energy Physics - Phenomenology · Physics 2009-10-30 G. Lazarides

The primordial inflation dilutes all matter except the quantum fluctuations which we see in the cosmic microwave background (CMB) radiation. Therefore the last phases of inflation must be embedded within a beyond the Standard Model (SM)…

High Energy Physics - Phenomenology · Physics 2013-02-06 Celine Boehm , Jonathan Da Silva , Anupam Mazumdar , Ernestas Pukartas

The Minimal Supersymmetry Standard Model contains several hundreds of D- and F-flat directions that are lifted by soft susy breaking terms as well as by non-renormalizable terms. In a recent paper we find that only two of these directions,…

High Energy Physics - Phenomenology · Physics 2010-11-11 Juan Garcia-Bellido
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