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Related papers: T-Model Higgs Inflation in Supergravity

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We study the cosmology of a recent model of supersymmetry breaking, in the presence of a tuneable positive cosmological constant, based on a gauged shift symmetry of a string modulus that can be identified with the string dilaton. The…

High Energy Physics - Phenomenology · Physics 2016-12-20 I. Antoniadis , A. Chatrabhuti , H. Isono , R. Knoops

$R+R^2$ Supergravity is known to be equivalent to standard Supergravity coupled to two chiral supermultiples with a no-scale K\"ahler potential. Within this framework, that can accomodate vanishing vacuum energy and spontaneous…

High Energy Physics - Theory · Physics 2015-04-08 A. B. Lahanas , K. Tamvakis

We present a supergravity inflationary scenario in which the inflaton field takes values considerably larger than the Planck scale. It is based on a class of inflationary potentials which can be derived from ``singular'' Kaehler potentials…

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

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 consider the simplest and most economic version among the proposed non-minimal supersymmetric models, in which the $\mu$-parameter is promoted to a singlet superfield, whose all self-couplings are absent from the renormalizable…

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

We present viable F-term realizations of the hybrid inflationary scenario in the context of supergravity addressing at the same time the well-known problems of the initial conditions and of the adequate suppression of the inflaton mass. An…

High Energy Physics - Phenomenology · Physics 2009-11-10 C. Panagiotakopoulos

We study reheating after the end of inflation in models where the inflaton is the superpartner of goldstino and is charged under a gauged $U(1)$ R-symmetry. We consider two classes of models -- one is small field characterized by an almost…

High Energy Physics - Theory · Physics 2021-12-10 Yermek Aldabergenov , Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono

We discuss a five dimensional inflationary scenario based on a supersymmetric SO(10) model compactified on $S^1/(Z_2\times Z_2')$. Inflation is implemented through scalar potentials on four dimensional branes, and a brane-localized…

High Energy Physics - Phenomenology · Physics 2011-05-12 Bumseok Kyae , Qaisar Shafi

We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in $N=1$ supergravity with the dilaton-axion chiral superfield $T$ in the presence of an $N=1$ vector multiplet with…

High Energy Physics - Theory · Physics 2019-08-28 Yermek Aldabergenov , Auttakit Chatrabhuti , Sergei V. Ketov

Theories with elementary scalar degrees of freedom seem nowadays required for simple descriptions of the Standard Model and of the Early Universe. It is then natural to embed theories of inflation in supergravity, also in view of their…

High Energy Physics - Theory · Physics 2015-09-30 S. Ferrara , A. Sagnotti

We investigate a scenario of cosmological inflation realised along a flat direction of the minimal seesaw model embedded in supergravity with a noncanonical R-parity violating K\"{a}hler potential. It is shown that with appropriate seesaw…

High Energy Physics - Phenomenology · Physics 2013-11-07 Masato Arai , Shinsuke Kawai , Nobuchika Okada

We construct a chaotic inflation model in which the Higgs fields play the role of the inflaton in the standard model as well as in the singlet extension of the supersymmetric standard model. The key idea is to allow a non-canonical kinetic…

High Energy Physics - Phenomenology · Physics 2011-02-15 Kazunori Nakayama , Fuminobu Takahashi

Combination of Plank and BICEP2 data reported that tensor to scalar ratio $r\simeq 0.16$ and scalar spectral index $n_{s}\simeq 0.96$. In this short note, it is shown that chaotic inflation with quadratic potential, which perfectly accounts…

High Energy Physics - Phenomenology · Physics 2015-02-25 Sibo Zheng

In this paper we will illustrate how to constrain unavoidable K\"ahler corrections for ${\cal N}=1$ supergravity (SUGRA) inflation from the recent Planck data. We will show that the non-renormalizable K\"ahler operators will induce in…

High Energy Physics - Theory · Physics 2014-04-15 Sayantan Choudhury , Anupam Mazumdar , Ernestas Pukartas

We investigate a topological inflation model in supergravity. By means of numerical simulations, it is confirmed that topological inflation can take place in supergravity. We also show that the condition for successful inflation depends not…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Kawasaki , Nobuyuki Sakai , Masahide Yamaguchi , T. Yanagida

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical Abelian projection and centerization. The underlying gauge symmetry is…

High Energy Physics - Phenomenology · Physics 2009-11-07 Ralf Hofmann , Mathias Th. Keil

We discuss five dimensional (5D) supersymmetric SO(10) compactified on the orbifold $S^1/(Z_2\times Z_2')$ such that the SO(10) gauge symmetry is broken on the fixed point(s) to its maximal subgroup(s). The MSSM gauge symmetry is recovered…

High Energy Physics - Phenomenology · Physics 2007-05-23 Bumseok Kyae , Qaisar Shafi

We explore a new class of supersymmetric models of inflation where the inflaton is realised as a combination of a Higgs field and (gauge non-singlet) matter fields, using a "tribrid" structure of the superpotential. Inflation is associated…

High Energy Physics - Phenomenology · Physics 2015-03-20 Stefan Antusch , David Nolde , Mansoor Ur Rehman

We study a supergravity model of inflation with R-symmetry and a single scalar field, the inflaton, slowly rolling away from the origin. The scales of inflation can be as low as the supersymmetry breaking scale of 10^10 GeV or even the…

High Energy Physics - Theory · Physics 2009-10-31 G. German , A. de la Macorra , M. Mondragon

Gravitino-condensate-induced inflation via the super-Higgs effect is a UV-motivated scenario for both inflating the early universe and breaking local supersymmetry dynamically, entirely independent of any coupling to external matter. As an…

General Relativity and Quantum Cosmology · Physics 2015-06-22 Jean Alexandre , Nick Houston , Nick E. Mavromatos