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相关论文: Some constraints on brane inflation models with po…

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We investigate inflation in closed Friedmann-Robertson-Walker universe filled with the scalar field with power-law potential. For a wide range of powers and parameters of the potential we numerically calculated the slow-roll parameters and…

天体物理学 · 物理学 2009-11-16 S. A. Pavluchenko

Upper bounds on the energy scale at the end of inflation in the Randall-Sundrum type II braneworld scenario are derived. The analysis is made exact by introducing new parameters that represent extensions of the Hubble flow parameters. Only…

天体物理学 · 物理学 2009-11-07 Rachael M. Hawkins , James E. Lidsey

We study the inflationary dynamics of the universe in the Randall-Sandrum typeII Braneworld model. We consider both an inverse-power law and exponential potentials and apply the Slow-Roll approximation in high energy limit to derive…

广义相对论与量子宇宙学 · 物理学 2014-08-12 M. Bennai , H. Chakir , Z. Sakhi

We are interested on studing various inflationary spectrum perturbation parameters in the context of the Randall-Sandrum type 2 Braneworld model. We consider in particular three types of potentials. We apply the slow-roll approximation in…

高能物理 - 理论 · 物理学 2015-06-03 R. Zarrouki , Z. Sakhi , M. Bennai

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

In the large extra dimensional braneworld inflation, Friedmann equation is modified to include a quadratic term in energy density with an additional parameter $\lambda$ called brane tension in addition to the usual linear term. The high…

广义相对论与量子宇宙学 · 物理学 2020-01-15 Mudassar Sabir , Waqas Ahmed , Yungui Gong , Yizhou Lu

In this paper, warm inflationary models on a brane scenario are studied. Here we consider slow-roll inflation and high-dissipation regime in a high-energy scenario. General conditions required for these models to be realizable are derived.…

天体物理学 · 物理学 2008-11-26 M. Antonella Cid , Sergio del Campo , Ramon Herrera

We study a new inflation potential in the framework of the Randall-Sundrum type 2 Braneworld model. Using the technic developped in(Phys. Rev. D75, 123504 (2007).1), we consider both an monomial and a new inflation potentials and apply the…

高能物理 - 理论 · 物理学 2010-02-02 R. Zarrouki , Z. Sakhi , M. Bennai

In light of the results from the WMAP three-year sky survey, we study an inflationary model based on a single-field polynomial potential, with up to quartic terms in the inflaton field. Our analysis is performed in the context of the…

天体物理学 · 物理学 2009-11-11 M. C. Bento , R. Gonzalez Felipe , N. M. C. Santos

We formalize the Hubble slow-roll formalism for inflationary dynamics in Randall-Sundrum Type II braneworld cosmologies, defining Hubble slow-roll parameters which can be used along with the Hamilton-Jacobi formalism. Focussing on the…

天体物理学 · 物理学 2009-11-10 Erandy Ramirez , Andrew R. Liddle

We analyze the Randal Sundrum brane-world inflation scenario in the context of the latest CMB constraints from Planck. We summarize constraints on the most popular classes of models and explore some more realistic inflaton effective…

宇宙学与河外天体物理 · 物理学 2018-03-19 Mayukh R. Gangopadhyay , Grant J. Mathews

We examine observational constraints on chaotic inflation models in the Randall-Sundrum Type II braneworld. If inflation takes place in the high-energy regime, the perturbations produced by the quadratic potential are further from…

天体物理学 · 物理学 2009-11-10 Andrew R Liddle , Anthony J Smith

We investigate inflation with a class of concave inflaton potentials of the form $\sim \phi^n$ $(0<n<1)$ in the Randall-Sundrum model with an infinite extra spatial dimension. We show that this class of models is much more in good agreement…

高能物理 - 唯象学 · 物理学 2020-08-27 Ngo Phuc Duc Loc

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

Inflationary cosmology is developed in the second Randall-Sundrum braneworld scenario, where the accelerated expansion arises through potentials that are too steep to drive inflation in conventional cosmology. A relationship between the…

天体物理学 · 物理学 2009-11-06 Greg Huey , James E. Lidsey

It has been shown in the last few years that 3-form fields present viable cosmological solutions for inflation and dark energy with particular observable signatures distinct from those of canonical single scalar field inflation. The aim of…

宇宙学与河外天体物理 · 物理学 2016-02-17 Bruno J. Barros , Nelson J. Nunes

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 construct an inflation model on the Randall-Sundrum I (RSI) brane where a bulk scalar field stabilizes the inter-brane separation. We study impact of the bulk scalar field on the inflationary dynamics on the brane. We proceed in two…

高能物理 - 理论 · 物理学 2014-11-20 Kourosh Nozari , Siamak Akhshabi

We propose a model of inflation in the framework of brane cosmology driven by background supergravity. Starting from bulk supergravity we construct the inflaton potential on the brane and employ it to investigate for the consequences to…

高能物理 - 理论 · 物理学 2015-03-19 Sayantan Choudhury , Supratik Pal

In this paper, we study inflation with {\alpha}-attractor potential in the RS braneworlds where high energy corrections to the Friedmann equation facilitate slow roll. In this scenario, we numerically investigate the inflationary parameters…

广义相对论与量子宇宙学 · 物理学 2019-05-22 Nur Jaman , Kairat Myrzakulov
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