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相关论文: Flat-Directions in Grand Unification With $U(1)_R$…

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Within supersymmetry we provide an example where the inflaton sector is derived from a gauge invariant polynomial of SU(N) or SO(N) gauge theory. Inflation in our model is driven by multi-flat directions, which assist accelerated expansion.…

高能物理 - 理论 · 物理学 2009-11-10 Asko Jokinen , Anupam Mazumdar

The flat-space limit of the one-loop effective potential for SO(10) GUT theories in spatially flat Friedmann-Robertson-Walker cosmologies is applied to study the dynamics of the early universe. The numerical integration of the corresponding…

广义相对论与量子宇宙学 · 物理学 2011-08-11 Giampiero Esposito , Gennaro Miele , Pietro Santorelli

We discuss inflationary cosmology in a five dimensional SO(10) model compactified on $S^1/(Z_2\times Z_2')$, which yields $SU(3)_c\times SU(2)_L\times U(1)_Y\times U(1)_X$ below the compactification scale. The gauge symmetry $SU(5)\times…

高能物理 - 唯象学 · 物理学 2014-11-17 Bumseok Kyae , Qaisar Shafi

In a class of realistic four and five dimensional supersymmetric grand unified models, the scalar spectral index is found to be $n_s=0.98 (\pm 0.01)$, in excellent agreement with the values determined by several previous experiments and…

天体物理学 · 物理学 2011-05-12 Bumseok Kyae , Qaisar Shafi

We develop a new class of chaotic inflation models with spontaneously broken conformal invariance. Observational consequences of a broad class of such models are stable with respect to strong deformations of the scalar potential. This…

高能物理 - 理论 · 物理学 2015-06-16 Renata Kallosh , Andrei Linde

We suggest a systematic procedure to study D- and F-flat directions in a large class of models with an anomalous U(1). This class of models is characterized by the existence of a vacuum that breaks all Abelian gauge symmetries connecting…

高能物理 - 唯象学 · 物理学 2009-10-30 Nikolaos Irges , Stéphane Lavignac

We consider a set of scalar fields, consisting of a single flat direction and one or several non-flat directions. We take our cue from the MSSM, considering separately D-flat and F-flat directions, but our results apply to any…

宇宙学与河外天体物理 · 物理学 2015-05-30 Kari Enqvist , Daniel G. Figueroa , Gerasimos Rigopoulos

We show that a class of Wess--Zumino models lead to inflation in supersymmetry and supergravity. This is due to the existence of a classically flat direction generic to these models. The pseudomodulus that parametrizes this flat direction…

高能物理 - 唯象学 · 物理学 2010-01-28 Edi Halyo

Inflationary models with a superheavy scale F-term hybrid inflation followed by an intermediate scale modular inflation are considered. The restrictions on the power spectrum P_R of curvature perturbation and the spectral index n_s from the…

高能物理 - 唯象学 · 物理学 2008-11-26 George Lazarides

A supersymmetric hybrid inflation framework is employed to realize a class of non-minimal inflation models with $U(1)_R \times Z_n$ global symmetry. This framework naturally incorporates models based on grand unified theories by avoiding…

高能物理 - 唯象学 · 物理学 2020-02-17 Muhammad Atif Masoud , Mansoor Ur Rehman , Mian Muhammad Azeem Abid

We have investigated a number of GUT models for the possibility that their Higgs fields might be responsible for inflation in the early universe. In addition to models having an intrinsic Planck mass parameter, we have entertained…

高能物理 - 唯象学 · 物理学 2015-06-05 Martin B. Einhorn , D. R. Timothy Jones

The Standard Model Higgs boson with large nonminimal coupling to the gravitational curvature can drive cosmological inflation. We study this type of inflationary scenario in the context of supersymmetric grand unification and point out that…

高能物理 - 唯象学 · 物理学 2013-05-29 Masato Arai , Shinsuke Kawai , Nobuchika Okada

We present a model where early inflation and late accelerating expansion of the Universe are driven by the real and imaginary parts of a single complex scalar field, which we identified as inflaton and phantom field, respectively. This…

天体物理学 · 物理学 2008-11-26 Abdel Pérez-Lorenzana , Merced Montesinos , Tonatiuh Matos

Recently it was shown that discrete R-invariance in superpotential can lead to a successful flat potential in inflation. We suggest that this discrete R-symmetry arises from an underlying supersymmetric gauge theory, which gives rise to a…

高能物理 - 唯象学 · 物理学 2008-02-03 Tomohiro Matsuda

We show that the natural presence of flat directions in supersymmetric theories allows for nonrestoration of global and/or gauge symmetries. This has important cosmological consequences for supersymmetric GUTs and in particular it offers a…

高能物理 - 唯象学 · 物理学 2009-10-31 Borut Bajc , Goran Senjanovic

We study the impact of the symmetry breaking patterns from supersymmetric SO(10) down to the standard model on the standard big-bang cosmology through the formation of topological defects. None of the models is consistent with the standard…

高能物理 - 唯象学 · 物理学 2010-11-01 Rachel Jeannerot , Anne-Christine Davis

Supersymmetric flat directions can have a number of important consequences in the very early universe. Depending on the form of the SUSY breaking potential arising from the finite energy density at early times, coherent production of scalar…

高能物理 - 唯象学 · 物理学 2008-02-03 Scott Thomas

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,…

高能物理 - 唯象学 · 物理学 2015-08-04 John Ellis , Tomas E. Gonzalo , Julia Harz , Wei-Chih Huang

Moduli fields, which parameterize perturbative flat directions of the potential in supersymmetric theories, are natural candidates to act as inflatons. An inflationary potential on moduli space can result if the scale of dynamical SUSY…

高能物理 - 理论 · 物理学 2009-10-28 Scott Thomas

It is well known that large Hubble-induced supergravity corrections to the inflaton field can ruin the flatness of the potential, thus creating a tension between slow-roll inflation and supergravity. In this paper we show that it is…

高能物理 - 理论 · 物理学 2012-02-13 Anupam Mazumdar , Seshadri Nadathur , Philip Stephens
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