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Related papers: Flat direction MSSM (A-term) Inflation

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A novel realization of the Starobinsky inflationary model within a moderate extension of the Minimal Supersymmetric Standard Model (MSSM) is presented. The proposed superpotential is uniquely determined by applying a continuous R and a Z_2…

High Energy Physics - Phenomenology · Physics 2017-07-14 C. Pallis

We investigate a standard minimally-coupled scalar-field inflationary scenario, which is based on a new potential, with suitably generalized plateau features, that leads to extra small tensor-to-scalar ratios. In particular, we consider a…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-13 Gerasimos Kouniatalis , Emmanuel N. Saridakis

We study in detail the possibility that the flat directions of the Minimal Supersymmetric Standard Model (MSSM) could act as a curvaton and generate the observed adiabatic density perturbations. For that the flat direction energy density…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kari Enqvist , Asko Jokinen , Shinta Kasuya , Anupam Mazumdar

We explore the upper bound on the tensor-to-scalar ratio $r$ in supersymmetric (F-term) hybrid inflation models with the gauge symmetry breaking scale set equal to the value $2.86\cdot10^{16} {\rm GeV}$, as dictated by the unification of…

High Energy Physics - Phenomenology · Physics 2014-05-30 Matthew Civiletti , Constantinos Pallis , Qaisar Shafi

A new model for inflation using modified gravity in the Palatini formalism is constructed. Here non-minimal coupling of scalar field h with the curvature R as a general function f(R,h) is considered. Explicit inflation models for some…

General Relativity and Quantum Cosmology · Physics 2021-05-19 Nayan Das , Sukanta Panda

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 study a supergravity model of inflation essentially depending on one parameter which can be identified with the slope of the potential at the origin. In this type of models the inflaton rolls at high energy from negative values and a…

Astrophysics · Physics 2009-11-10 G. German , A. de la Macorra

Considering gravitino dark matter scenarios, we study constraints on the reheating temperature of inflation. We present the gauge-invariant result for the thermally produced gravitino yield to leading order in the Standard Model gauge…

High Energy Physics - Phenomenology · Physics 2008-11-26 Josef Pradler , Frank Daniel Steffen

We consider a supersymmetric hybrid inflation scenario in which the U(1) $R$-symmetry is explicitly broken by Planck scale suppressed operators in the superpotential. We provide an example with minimal K\"ahler potential, with the…

High Energy Physics - Phenomenology · Physics 2015-06-15 Matthew Civiletti , Mansoor Ur Rehman , Eric Sabo , Qaisar Shafi , Joshua Wickman

We investigate a novel scenario of cosmological inflation in a gauged $B-L$ extended minimal supersymmetric Standard Model with R-symmetry. We use a noncanonical K\"{a}hler potential and a superpotential, both preserving the R-symmetry to…

High Energy Physics - Phenomenology · Physics 2014-05-22 Masato Arai , Shinsuke Kawai , Nobuchika Okada

Light scalar fields present during inflation can lead to interesting observable signatures, especially in models with non-equilibrium reheating dynamics. We study a supersymmetric hybrid inflation model with a third scalar whose lightness…

Cosmology and Nongalactic Astrophysics · Physics 2013-08-20 Stefano Orani , Arttu Rajantie

Allowing for the possibility of large extra dimensions, the fundamental Planck scale $M$ could be anywhere in the range $\TeV\lsim M\lsim \mpl$, where $\mpl=2.4\times 10^{18}\GeV$ is the four-dimensional Planck scale. If $M\sim\TeV$,…

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

Models of supersymmetric D-term inflation require a new mass scale near 10^{15-16} GeV in order to match the density perturbation spectrum observed by COBE. Attempts to obtain such a scale from the anomalous U(1) of string theories fail in…

High Energy Physics - Phenomenology · Physics 2007-05-23 Christopher Kolda , David H. Lyth

We point out that for a class of `new inflation' models in supergravity the required initial value of the inflaton field is dynamically set if there is another inflation (`pre-inflation') before the `new inflation'. We study the dynamics of…

High Energy Physics - Phenomenology · Physics 2009-10-30 K. -I. Izawa , M. Kawasaki , T. Yanagida

A simple extension of the minimal left-right symmetric supersymmetric grand unified theory model is constructed by adding two pairs of superfields. This naturally violates the partial Yukawa unification predicted by the minimal model. After…

High Energy Physics - Phenomenology · Physics 2014-03-26 R. Armillis , G. Lazarides , C. Pallis

We consider the possibility that the dark energy responsible for inflation is deposited into extra dimensions outside of our observable universe. Reheating and all matter can then be obtained from the MSSM flat direction condensate…

High Energy Physics - Phenomenology · Physics 2008-11-26 Kari Enqvist , Shinta Kasuya , Anupam Mazumdar

We analyze the cosmological implications of F-term hybrid inflation with a subdominant Fayet--Iliopoulos D-term whose presence explicitly breaks a D-parity in the inflaton-waterfall sector. This scenario of inflation, which is called…

High Energy Physics - Phenomenology · Physics 2009-11-11 Bjorn Garbrecht , Constantinos Pallis , Apostolos Pilaftsis

We propose to address the fine tuning problem of inflection point inflation by the addition of extra vacuum energy that is present during inflation but disappears afterwards. We show that in such a case, the required amount of fine tuning…

High Energy Physics - Phenomenology · Physics 2014-11-20 Kari Enqvist , Anupam Mazumdar , Philip Stephens

We present a general polynomial chaotic inflation model in supergravity, for which the predicted spectral index and tensor-to-scalar ratio can lie within the 1 sigma region allowed by the Planck results. Most importantly, the predicted…

High Energy Physics - Phenomenology · Physics 2015-06-16 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

In this paper, we give a brief review of the Minimal Supersymmetric Standard Model (MSSM) and "$\mu$ from $\nu$" Supersymmetric Standard Model ($\mu \nu$SSM). Then we propose a generalization of $\mu \nu$SSM in order to explain the recent…

High Energy Physics - Phenomenology · Physics 2016-07-07 M. C. Rodriguez , I. V. Vancea
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