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相关论文: Inflation and The Minimal Supersymmetric Standard …

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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,…

高能物理 - 唯象学 · 物理学 2010-11-11 Juan Garcia-Bellido

We consider the effective evolution of a phenomenological model from FLRW supersymmetric quantum cosmology with a scalar field. The scalar field acts as a clock and inflaton. We examine a family of simple superpotentials that produce an…

广义相对论与量子宇宙学 · 物理学 2022-08-17 N. E. Martínez-Pérez , C. Ramírez , V. M. Vázquez Báez

We explored a Higgs inflationary scenario in the SUGRA embedding of the MSSM in Einstein frame where the inflaton is contained in the $SU(2)$ Higgs doublet. We include all higher order non-renormalizable terms to the MSSM superpotential and…

高能物理 - 唯象学 · 物理学 2016-07-28 Girish Kumar Chakravarty , Gaveshna Gupta , Gaetano Lambiase , Subhendra Mohanty

Inflation has long been the accepted paradigm for understanding the early universe. Most models of inflation have a scalar field acting as the inflaton particle which decays after inflation during a process called reheating into standard…

广义相对论与量子宇宙学 · 物理学 2018-11-30 Abhass Kumar

Detailed analyses of the WMAP data indicate possible oscillatory features in the primordial curvature perturbation, which moreover appears to be suppressed beyond the present Hubble radius. Such deviations from the usual inflationary…

天体物理学 · 物理学 2014-11-18 Paul Hunt , Subir Sarkar

We investigate the Two-Higgs-Doublet-Standard Model-Axion-Seesaw-Higgs-Portal inflation (2hdSMASH) model consisting of two Higgs doublets, a Standard Model (SM) singlet complex scalar and three SM singlet right-handed Majorana neutrinos…

高能物理 - 唯象学 · 物理学 2023-12-22 Juhi Dutta

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…

高能物理 - 唯象学 · 物理学 2009-11-07 Ralf Hofmann , Mathias Th. Keil

We explore in the supergravity context the possibility that a Higgs scalar may drive inflation via a non-minimal coupling to gravity characterised by a large dimensionless coupling constant. We find that this scenario is not compatible with…

高能物理 - 唯象学 · 物理学 2014-11-20 Martin B Einhorn , D R Timothy Jones

Cosmological inflation is the dominating paradigm to account for observations of the Cosmic Microwave Background (CMB). In this thesis, we study the phenomenology of a class of particularly well motivated models of inflation, known under…

宇宙学与河外天体物理 · 物理学 2013-08-27 Stefano Orani

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…

高能物理 - 唯象学 · 物理学 2012-04-19 Sayantan Choudhury , Supratik Pal

The present study connects inflation and freeze-in type dark matter (DM) within the same setup. Although the observables in these two phenomena lie at vastly different energy scales, they have been properly handled using the RG running of…

高能物理 - 唯象学 · 物理学 2025-07-01 Sarif Khan , Sourov Roy , Ananya Tapadar

The Next-to-Minimal Supersymmetric Standard Model (NMSSM) can incorporate inflation, where a combination of the Higgs-doublet fields plays the role of the inflaton. At the high scale, the Higgs doublets are non-minimally coupled to…

高能物理 - 唯象学 · 物理学 2018-12-03 Wolfgang Gregor Hollik , Stefan Liebler , Gudrid Moortgat-Pick , Sebastian Paßehr , Georg Weiglein

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…

高能物理 - 唯象学 · 物理学 2016-12-20 I. Antoniadis , A. Chatrabhuti , H. Isono , R. Knoops

We consider the possibility of using one of the $D$-flat directions in the minimal supersymmetric standard model (MSSM) as the inflaton. We show that the flat direction consisting of (first generation) left- and right-handed up-squarks as…

高能物理 - 唯象学 · 物理学 2014-11-17 Shinta Kasuya , Takeo Moroi , Fuminobu Takahashi

We present a complete particle physics model that explains three major problems of modern cosmology: inflation, dark matter and dark energy, and also gives a mechanism for leptogenesis. The model has a new gauge group $SU(2)_Z$ that grows…

天体物理学 · 物理学 2008-11-26 P. Q. Hung , Eduard Masso , Gabriel Zsembinszki

We consider a minimal supersymmetric extension of the Standard Model, with right-handed neutrinos and local B-L, the difference between baryon and lepton number, a symmetry which is spontaneously broken at the scale of grand unification. To…

高能物理 - 唯象学 · 物理学 2015-04-09 Wilfried Buchmüller , Valerie Domcke , Kohei Kamada , Kai Schmitz

In a recent work, we demonstrated that a modified gravity model in which a scalar "darkon" field is coupled to both the standard Riemannian metric and to another non-Riemannian volume form is compatible with observational data from…

广义相对论与量子宇宙学 · 物理学 2019-11-12 Denitsa Staicova , Michail Stoilov

Inflation is a highly favoured theory for the early Universe. It is compatible with current observations of the cosmic microwave background and large scale structure and is a driver in the quest to detect primordial gravitational waves. It…

宇宙学与河外天体物理 · 物理学 2024-04-19 Tomás Sousa , Deaglan J. Bartlett , Harry Desmond , Pedro G. Ferreira

In this letter I discuss a class of extensions of the standard model that have a minimal number of possible parameters, but can in principle explain dark matter and inflation. It is pointed out that the so-called new minimal standard model…

高能物理 - 唯象学 · 物理学 2009-11-11 J. J. van der Bij

In the first part of this paper, we outline the construction of an inflationary cosmology in the framework where inflation is described by a universally evolving scalar field, with the Lagrangian ${\cal L}_\phi=-{1/2}(\partial\phi)^2…

天体物理学 · 物理学 2009-12-15 Ishwaree P. Neupane , Christoph Scherer