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相关论文: A dark radiation era prior to the inflationary pha…

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In brane world scenarios inflationary vacuum energy may escape into the higher dimensional bulk leaving behind a dark radiation effect on the brane. The paper analyses the damping of an inflaton by massless bulk scalar radiation and the…

高能物理 - 唯象学 · 物理学 2009-11-10 Cheng-Ji Chang , I. G. Moss

We investigate the effects on cosmological density perturbations of dark radiation in a Randall-Sundrum 2 type brane-world. Dark radiation in the background is limited by observational constraints to be a small fraction of the radiation…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Burin Gumjudpai , Roy Maartens , Christopher Gordon

It is commonly believed that our Universe has experienced two different stages of accelerated expansion. The early stage is known as inflation and the current acceleration is driven by dark energy. Observing inflation and dark energy…

天体物理学 · 物理学 2009-11-11 Jun-Qing Xia , Gong-Bo Zhao , Bo Feng , Xinmin Zhang

In this work, we are going to study the inflationary era of the Universe evolution by using second type of Randall-Sundrum model (RS-II) braneworld gravity. It is supposed that the Universe is dominated by scalar field with noncanonical…

宇宙学与河外天体物理 · 物理学 2014-05-27 T. Golanbari , A. Mohammadi , Kh. Saaidi

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 behaviour of scalar perturbations in the radiation-dominated era of Randall-Sundrum braneworld cosmology by numerically solving the coupled bulk and brane master wave equations. We find that density perturbations with…

天体物理学 · 物理学 2009-05-18 Antonio Cardoso , Takashi Hiramatsu , Kazuya Koyama , Sanjeev S. Seahra

We present several features of a cosmological model based on the Brans-Dicke-Jordan-Thirry action which is scale invariant with a quartic potential for the Jordan scalar field. We show that the radiation dominated era starts with a closed…

广义相对论与量子宇宙学 · 物理学 2025-08-28 Metin Arik , Medine Ildes , Mikhail B. Sheftel

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

We propose an alternative inflationary universe scenario in the context of Randall-Sundrum braneworld cosmology. In this new scenario the existence of extra-dimension(s) plays an essential role. First, the brane universe is initially in the…

高能物理 - 理论 · 物理学 2009-11-07 Uchida Gen , Akihiro Ishibashi , Takahiro Tanaka

Here $f(R)$-cosmology is discussed using a different approach. This model explains early-inflation, emergence of cosmic background radiation at the exit from inflation, cosmic deceleration during radiation-dominance followed by deceleration…

广义相对论与量子宇宙学 · 物理学 2008-10-09 S. K. Srivastava

The standard cosmological model, based on general relativity with an inflationary era, is very effective in accounting for a broad range of observed features of the universe. However, the ongoing puzzles about the nature of dark matter and…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Roy Maartens

Kination dominated quintessence models of dark energy have the intriguing feature that the relic abundance of thermal cold dark matter can be significantly enhanced compared to the predictions from standard cosmology. Previous treatments of…

高能物理 - 唯象学 · 物理学 2008-11-26 Daniel J. H. Chung , Lisa L. Everett , Konstantin T. Matchev

A unified description of inflation, dark energy, and dark matter is presented within a two-scalar-field cosmological model. Inflation, assumed to be of the warm type, is driven by one of the scalar fields, which, shortly after the end of…

广义相对论与量子宇宙学 · 物理学 2020-11-24 Paulo M. Sá

In the context of an inflationary Randall-Sundrum Type II braneworld (RS2) we calculate spectral indices and amplitudes of cosmological scalar and tensor perturbations, up to second order in slow-roll parameters. Under very simple…

高能物理 - 唯象学 · 物理学 2009-11-10 Gianluca Calcagni

A novel scalar field free approach to cosmic inflation is presented. The inflationary Universe and the radiation dominated Universe are shown, within the framework of unified brane cosmology, to be two different phases governed by one and…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Aharon Davidson , Ilya Gurwich

In the present work we discuss inflation, dark matter and cosmological evolution in the context of the brane-world scenario. Being string theory inspired, the brane-world models provide corrections to the General Relativity, which is…

高能物理 - 唯象学 · 物理学 2012-05-28 G. Panotopoulos

We develop a four-dimensional effective theory for Randall-Sundrum models which allows us to calculate long wavelength adiabatic perturbations in a regime where the $\rho ^2$ terms characteristic of braneworld cosmology are significant.…

高能物理 - 理论 · 物理学 2009-11-10 Claudia de Rham

An epoch of accelerated expansion, or inflation, in the early universe solves several cosmological problems. While there are many models of inflation only recently has it become possible to discriminate between some of the models using…

高能物理 - 唯象学 · 物理学 2007-06-29 Raghavan Rangarajan

We investigate the dynamics of a bulk scalar field with various decay channels in the Randall-Sundrum infinite braneworld scenario. A bulk scalar field in this scenario has a quasi-localized mode which dominates the late-time behavior near…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Takahiro Tanaka , Yoshiaki Himemoto

We have developed a formalism to study an inflationary scenario driven by a bulk inflaton in the two-brane system. The 4-dimensional low energy effective action is obtained using the gradient expansion method. It is also found that the dark…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Jiro Soda , Sugumi Kanno
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