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相关论文: Blue Perturbation Spectra from Hybrid Inflation wi…

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We construct a hybrid inflationary model associated with the superheavy scale of the minimal supersymmetric standard model which is based on the simplest superpotential for symmetry breaking and in which the inflaton potential along the…

高能物理 - 唯象学 · 物理学 2009-06-19 C. Panagiotakopoulos

We propose a simple realization of hybrid inflation in supergravity, which does not require any unnaturally small parameters. Inflation in this scenario is relatively short, and inflationary density perturbations fall down on large scales,…

高能物理 - 唯象学 · 物理学 2009-06-19 Andrei Linde , Antonio Riotto

Within the context of supersymmetric hybrid inflation, we study a multiple-stage inflationary scenario that can generate a primordial spectrum of adiabatic density perturbations with a break at $k_b \simeq 0.05 h Mpc^{-1}$. The presence of…

高能物理 - 唯象学 · 物理学 2007-05-23 Mairi Sakellariadou , Nikos Tetradis

We propose a new version of the hybrid inflation scenario that produces a significantly tilted n>1 spectrum of curvature perturbations. This may happen in supersymmetric models where the inflaton field acquires a mass proportional to the…

天体物理学 · 物理学 2009-09-29 Juan Garcia-Bellido , Andrei Linde

We show explicitly some exciting features of double-inflation: (i) it can often lead to strongly correlated adiabatic and entropy (isocurvature) power spectra. (ii) The two-field slow-roll consistency relations can be violated when the…

天体物理学 · 物理学 2009-11-07 Shinji Tsujikawa , David Parkinson , Bruce A. Bassett

We consider a supersymmetric grand unified model which leads to hybrid inflation and solves the strong CP and mu problems via a Peccei-Quinn symmetry, with the Peccei-Quinn field acting as a curvaton generating together with the inflaton…

高能物理 - 唯象学 · 物理学 2009-11-11 George Lazarides

We investigate inflationary models leading to density perturbations with a spectral index $n>1$ (``blue spectra"). These perturbation spectra may be useful to simultaneously account for both the amount of ultra large-scale power required to…

天体物理学 · 物理学 2010-12-09 S. Mollerach , S. Matarrese , F. Lucchin

We propose an inflation model in supergravity, in which chaotic and hybrid inflation occurs successively, followed by new inflation. During hybrid inflation, adiabatic fluctuations with a running spectral index with $\ns >1$ on a large…

高能物理 - 唯象学 · 物理学 2009-11-10 Masahide Yamaguchi , Jun'ichi Yokoyama

If an adiabatic density perturbation is responsible for large scale structure and the cmb anisotropy, its spectral index $n$ will be measured in the forseeable future with an accuracy $\Delta n\sim .01$. This is precisely the kind of…

高能物理 - 唯象学 · 物理学 2016-09-06 David H. Lyth

Motivated by the reported discovery of inflationary gravity waves by the BICEP2 experiment, we propose an inflationary scenario in supergravity, based on the standard superpotential used in hybrid inflation. The new model yields a…

高能物理 - 唯象学 · 物理学 2014-08-05 Constantinos Pallis , Qaisar Shafi

We propose a new class of inflationary models in which the scalar field potential governing inflation is generated by the same non-perturbative gauge dynamics that may lead to supersymmetry breaking. Such models satisfy constraints from…

高能物理 - 唯象学 · 物理学 2011-05-23 William H. Kinney , Antonio Riotto

We present a class of very simple inflationary models of two scalar fields which leads to nongaussian isothermal perturbations with "blue" spectrum, n > 1. One of the models is inspired by supersymmetric theories where light scalar fields…

天体物理学 · 物理学 2009-09-29 A. Linde , V. Mukhanov

The cosmological implication of a double inflation model with hybrid + new inflations in supergravity is studied. The hybrid inflation drives an inflaton for new inflation close to the origin through supergravity effects and new inflation…

高能物理 - 唯象学 · 物理学 2009-10-31 Toshiyuki Kanazawa , M. Kawasaki , Naoshi Sugiyama , T. Yanagida

Spectrum of density perturbations in the Universe generated from quantum-gravitational fluctuations in slow-roll-over inflationary scenarios with the Brans-Dicke gravity is calculated. It is shown that after inflation the isocurvature mode…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Alexei A. Starobinsky , Jun'ichi Yokoyama

We make a detailed calculation of the amplitude of isocurvature perturbations arising from inflationary models in which the cold dark matter is represented by a scalar field which acquires perturbations during inflation. We use this to…

天体物理学 · 物理学 2009-10-31 Andrew R Liddle , Anupam Mazumdar

We identify a new inflationary regime for which more than 60 e-folds are generated classically during the waterfall phase occuring after the usual hybrid inflation. By performing a bayesian Monte-Carlo-Markov-Chain analysis, this scenario…

广义相对论与量子宇宙学 · 物理学 2011-03-22 Sebastien Clesse

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

In multi-field inflation one or more non-adiabatic modes may become light, potentially inducing large levels of isocurvature perturbations in the cosmic microwave background. If in addition these light modes are coupled to the adiabatic…

宇宙学与河外天体物理 · 物理学 2017-04-19 Ana Achúcarro , Vicente Atal , Cristiano Germani , Gonzalo A. Palma

We show how supersymmetric hybrid inflation with scalar spectral index $n_{\rm s}\simeq 0.96 - 0.97$ is realized in the context of quasi-minimal supergravity if we insist that the inflationary potential not exhibit any local minima. We also…

高能物理 - 唯象学 · 物理学 2018-02-21 C. Panagiotakopoulos

In hybrid inflation, the inflaton generically has a tadpole due to gravitational effects in supergravity, which significantly changes the inflaton dynamics in high-scale supersymmetry. We point out that the tadpole can be cancelled if there…

高能物理 - 唯象学 · 物理学 2015-06-12 Tetsutaro Higaki , Kwang Sik Jeong , Fuminobu Takahashi
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