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Related papers: Inflection point inflation within supersymmetry

200 papers

We address an issue what kind of tuning realizes a flat potential for inflaton in supergravity. We restrict ourselves to the case that inflationary dynamics is not affected by separate supersymmetry-breaking effects, and consider examples…

High Energy Physics - Phenomenology · Physics 2007-10-08 K. -I. Izawa , Y. Shinbara

We investigate inflation driven by the Higgs boson in the Palatini formulation of General Relativity. Our analysis primarily focuses on a small non-minimal coupling of the Higgs field to gravity in the range $0<\xi\lesssim 1$. We…

High Energy Physics - Phenomenology · Physics 2023-06-07 Arthur Poisson , Inar Timiryasov , Sebastian Zell

A model of inflation is proposed in which compact extra dimensions allow a graceful exit without recourse to flat potentials or super-Planckian field values. Though bubbles of true vacuum are too sparse to uniformly reheat the Universe by…

High Energy Physics - Theory · Physics 2008-12-18 Adam R. Brown

Hybrid inflation faces two well-known problems: the blue spectrum of the non-supersymmetric version of the model and the fine-tuning of the initial conditions of the fields leading to sufficient inflation to account for the standard…

High Energy Physics - Phenomenology · Physics 2010-04-15 Sebastien Clesse , Jonathan Rocher

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

Following \cite{Lin:2009yt}, we explore the parameter space of the case when the supersymmetry (SUSY) breaking scale is lower, for example, in gauge mediated SUSY breaking model. During inflation, the form of the potential is $V_0$ plus…

High Energy Physics - Phenomenology · Physics 2014-11-18 Chia-Min Lin , Kingman Cheung

We consider the potential problems due to the production of inflatinos and gravitinos after inflation. Inflationary models with a single scale set by the microwave background anisotropies have a low enough reheat temperature to avoid…

High Energy Physics - Phenomenology · Physics 2009-09-15 Hans Peter Nilles , Keith A. Olive , Marco Peloso

We propose to study a smooth variant of the $\mu$-hybrid inflation model and a non-minimal Higgs model of inflation with quartic non-minimal coupling between the Higgs field and gravity within the context of a realistic GUT gauge group…

High Energy Physics - Phenomenology · Physics 2025-02-17 Umer Zubair

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

A scheme of simplified smooth hybrid inflation is realized in the framework of supersymmetric $SU(5)$. The smooth model of hybrid inflation provides a natural solution to the monopole problem that appears in the breaking of $SU(5)$ gauge…

High Energy Physics - Phenomenology · Physics 2017-10-06 Mansoor Ur Rehman , Umer Zubair

We revisit Higgs inflation in the framework of a minimal extension of the Standard Model gauge symmetry by a $U(1)_{B-L}$ factor. Various aspects are taken into account with particular focus on the role of the supersymmetry breaking (SUSY)…

High Energy Physics - Phenomenology · Physics 2021-09-29 Waqas Ahmed , Athanasios Karozas , George K. Leontaris

Usually one expectes the inflaton field to be coupled to some gauge-charged particles allowing for its decay during reheating. Such particles then play a role of the messengers for the gauge-mediated supersymmetry breaking during and…

High Energy Physics - Phenomenology · Physics 2009-10-28 G. Dvali , A. Riotto

We propose a model of inflation driven by minimal extension of SUSY, commonly known as MSSM. Starting from gauge invariant flat directions in the n = 4 level comprising of QQQL,QuQd,QuLe and uude, we construct the inflaton potential and…

High Energy Physics - Phenomenology · Physics 2012-04-19 Sayantan Choudhury , Supratik Pal

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 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 reconsider the fine-tuning problem of scalar-driven inflation arising from the need to couple the inflaton to ordinary matter in order to make reheating efficient. Quantum fluctuations of this matter induce Coleman-Weinberg corrections…

General Relativity and Quantum Cosmology · Physics 2019-11-13 S. P. Miao , S. Park , R. P. Woodard

We consider non-minimal \lambda \phi^4 inflation in a gauged non-supersymmetric U(1)_{B-L} model containing the gravitational coupling \xi \mathcal{R} \Phi^\dagger \Phi, where \mathcal{R} denotes the Ricci scalar and the standard model…

High Energy Physics - Phenomenology · Physics 2015-05-27 Nobuchika Okada , Mansoor Ur Rehman , Qaisar Shafi

The relation between the Hubble constant and the scale of supersymmetry breaking is investigated in models of inflation dominated by a string modulus. Usually in this kind of models the gravitino mass is of the same order of magnitude as…

High Energy Physics - Theory · Physics 2014-11-18 M. Badziak , M. Olechowski

We analyse the prospects for constructing hybrid models of inflation that provide a dynamical realisation of the apparent closeness between the supersymmetric GUT scale and the possible scale of cosmological inflation. In the first place,…

High Energy Physics - Phenomenology · Physics 2015-08-04 John Ellis , Tomas E. Gonzalo , Julia Harz , Wei-Chih Huang

We generalize the Effective Field Theory of Inflation to include additional light scalar degrees of freedom that are in their vacuum at the time the modes of interest are crossing the horizon. In order to make the scalars light in a natural…

High Energy Physics - Theory · Physics 2015-05-19 Leonardo Senatore , Matias Zaldarriaga
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