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We obtain observational constraints on Randall--Sundrum type II braneworld inflation using a compilation of data including WMAP, the 2dF and latest SDSS galaxy redshift surveys. We place constraints on three classes of inflation models…

天体物理学 · 物理学 2014-10-13 Shinji Tsujikawa , Andrew R. Liddle

We confront the predicted effects of hybrid inflationary models on the Cosmic Microwave Background (CMB) with three years of Wilkinson Microwave Anisotropy Probe (WMAP) observations. Using model selection, we compare the ability of a simple…

天体物理学 · 物理学 2010-10-27 Aurélien A. Fraisse

We make a more general determination of the inflationary observables in the standard 4-D and 5-D single-field inflationary scenarios, by the exact reconstruction of the dynamics of the inflation potential during the observable inflation…

宇宙学与河外天体物理 · 物理学 2009-11-10 L. A. Popa , N. Mandolesi , A. Caramete , C. Burigana

We discuss the important role played during inflation by one of the soft supersymmetry breaking terms in the inflationary potential of supersymmetric hybrid inflation models. With minimal Kaehler potential, the inclusion of this term allows…

高能物理 - 唯象学 · 物理学 2010-01-15 Mansoor Ur Rehman , Qaisar Shafi , Joshua R. Wickman

Many alternatives to canonical slow-roll inflation have been proposed over the years, one of the main motivations being to have a model, capable of generating observable values of non-Gaussianity. In this work, we (re-)explore the physical…

高能物理 - 理论 · 物理学 2016-07-06 David Pirtskhalava , Luca Santoni , Enrico Trincherini

We consider a supersymmetric hybrid inflation in the framework of the Randall-Sundrum type II Braneworld model. We drive an analytical expression for the scalar potential and find that the F-term dominates hybrid inflation process. We show…

广义相对论与量子宇宙学 · 物理学 2010-10-28 A. Bouaouda , R. Zarrouki , H. Chakir , M. Bennai

We propose an open hybrid inflation scenario that produces an open universe with a `tilted' n>1 spectrum of metric perturbations. The model contains a symmetry breaking field that tunnels to its true vacuum, producing a single bubble inside…

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

Noncommutative inflation is based upon the consideration of some effects of the space-time uncertainty principle motivated by ideas from string/M theory. The CMB anisotropies may carry a signature of this very early Universe correction from…

天体物理学 · 物理学 2009-11-11 Xin Zhang , Feng-Quan Wu

In this talk, I shall focus on theories beyond the Standard Model which predict massive neutrinos. Hybrid inflation emerges naturally in these theories: the slow-rolling inflaton field is a gauge singlet which couples with a GUT Higgs field…

高能物理 - 唯象学 · 物理学 2007-05-23 Rachel Jeannerot

Inflation in a five-dimensional brane world model with two boundary branes is studied. We make use of the moduli space approximation whereby the low energy theory reduces to a four-dimensional biscalar-tensor gravity plus a minimally…

天体物理学 · 物理学 2009-11-13 Christophe Ringeval , Philippe Brax , Carsten van de Bruck , Anne-Christine Davis

We analyze the weak (2 sigma) evidence for a running spectral index seen in the three-year WMAP dataset and its implications for single field, slow roll inflation. We assume that the running is comparable to the central value found from the…

天体物理学 · 物理学 2011-05-12 Richard Easther , Hiranya Peiris

We consider a supersymmetric hybrid inflation model with two inflaton fields. The superpotential during inflation is dominated by W=(\kappa S+\kappa' S')M^2, where S, S' are inflatons carrying the same U(1)_R charge, \kappa, \kappa' are…

高能物理 - 唯象学 · 物理学 2015-05-14 Bumseok Kyae

We study the linear perturbation of the recently proposed model of inflation where a uniform gauge-kinetic coupling of the inflaton to multiple vector fields breaks the cosmic no-hair conjecture while maintaining the isotropy. We derive the…

宇宙学与河外天体物理 · 物理学 2012-10-09 Kei Yamamoto

We briefly summarize and update a class of inflationary models from the early eighties based on a quartic (Coleman-Weinberg) potential for a gauge singlet scalar (inflaton) field. For vacuum energy scales comparable to the grand unification…

天体物理学 · 物理学 2011-05-12 Q. Shafi , V. N. Senoguz

Using a principal component (PC) basis that accommodates order unity features in the slow roll parameters as fine as 1/10 of a decade across more than 2 decades of the inflationary expansion, we test slow roll and single field inflation…

宇宙学与河外天体物理 · 物理学 2013-05-29 Cora Dvorkin , Wayne Hu

The recent data from the Boomerang and MAXIMA-1 balloon flights have marked the beginning of the precision era of Cosmic Microwave Background anisotropy (CMB) measurements. We investigate the observational constraints from the current CMB…

天体物理学 · 物理学 2009-10-31 William H. Kinney , Alessandro Melchiorri , Antonio Riotto

WMAP three-year data favors a red power spectrum at the level of 2 standard deviations, which provides a stringent constraint on the inflation models. In this note we use this data to constrain brane inflation models and find that KKLMMT…

高能物理 - 理论 · 物理学 2009-11-11 Qing-Guo Huang , Miao Li , Jian-Huang She

We study here the observational constraints on single-field inflationary models achievable with the next generation of CMB experiments. We particularly focus on a Stage-IV like experiment and forecasts its constraints on inflationary…

宇宙学与河外天体物理 · 物理学 2021-12-01 Guadalupe Cañas-Herrera , Fabrizio Renzi

The dynamics of hybrid models is usually approximated by the evolution of a scalar field slowly rolling along a nearly flat valley. Inflation ends with a waterfall phase, due to a tachyonic instability. This final phase is usually assumed…

宇宙学与河外天体物理 · 物理学 2011-09-27 Sébastien Clesse

The observational constraints on the primordial power spectrum have tightened considerably with the release of the first year analysis of the WMAP observations, especially when combined with the results from other CMB experiments and galaxy…

高能物理 - 唯象学 · 物理学 2009-11-10 Dominik J. Schwarz , Cesar A. Terrero-Escalante