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相关论文: The End for Extended Inflation?

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A short introduction to structure formation is given, followed by a discussion of the possible characteristics of the initial perturbations assuming a generic inflationary origin. Observational data related to large-scale structure and the…

天体物理学 · 物理学 2014-10-13 Pedro Viana

We address the issue of fine-tuning of the initial field configuration that can lead to hybrid inflation in the context of global supersymmetry. This problem is generated by the difference between the energy scale at which the Universe…

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

We examine extended inflation models enhanced by the addition of a coupling between the inflaton field and the space-time curvature. We examine two types of model, where the underlying inflaton potential takes on second-order and…

天体物理学 · 物理学 2009-10-22 Andrew M Laycock , Andrew R Liddle

In the early Universe matter can be described as a conformal invariant ultra-relativistic perfect fluid, which does not contribute, on classical level, to the evolution of the isotropic and homogeneous metric. If we suppose that there is…

高能物理 - 理论 · 物理学 2009-10-31 J. C. Fabris , A. M. Pelinson , I. L. Shapiro

We analyze various phases of inflation based on the anomaly-induced effective action of gravity (modified Starobinsky model), taking the cosmological constant Lambda and k=0, +/- 1 topologies into account. The total number of the…

高能物理 - 唯象学 · 物理学 2009-11-07 A. M. Pelinson , I. L. Shapiro , F. I. Takakura

When Inflation is embedded in a fundamental theory, such as string theory, it typically begins when the Universe is already substantially larger than the fundamental scale [such as the one defined by the string length scale]. This is…

广义相对论与量子宇宙学 · 物理学 2010-09-03 Brett McInnes

We supply fitting formulae enabling the normalization of slow-roll inflation models to the four-year COBE data. We fully include the effect of the gravitational wave modes, including the predicted relation of the amplitude of these modes to…

天体物理学 · 物理学 2008-11-26 Emory F Bunn , Andrew R Liddle , Martin White

Last year we argued that if slow-roll inflation followed the decay of a false vacuum in a large landscape, the steepening of the scalar potential between the inflationary plateau and the barrier generically leads to a potentially observable…

宇宙学与河外天体物理 · 物理学 2015-06-19 Raphael Bousso , Daniel Harlow , Leonardo Senatore

We develop our recent suggestion that inflation may be made past eternal, so that there is no initial cosmological singularity or "beginning of time". Inflation with multiple vacua generically approaches a steady-state statistical…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Anthony Aguirre , Steven Gratton

We derive an extended version of the well-known Lyth Bound on the total variation of the inflaton field, incorporating higher order corrections in slow roll. We connect the field variation $\Delta\phi$ to both the spectral index of scalar…

天体物理学 · 物理学 2009-11-11 Richard Easther , William H. Kinney , Brian A. Powell

This is an old article which has never been posted for public use and which only appeard in a relatively hard-to-get Proceedings of the Sakharov Conference in Moscow (May, 1991). The subject of this article has received a lot of attention…

天体物理学 · 物理学 2007-05-23 A. Mezhlumian , A. Starobinsky

In a recent paper, we suggested that the density fluctuation spectra arising from power-law (or extended) inflation, which are tilted with respect to the Harrison--Zel'dovich spectrum, may provide an explanation for the excess large scale…

天体物理学 · 物理学 2007-05-23 David H Lyth , Andrew A Liddle

We propose a scenario for inflation based upon the braneworld picture, in which high-energy corrections to the Friedmann equation permit inflation to take place with potentials ordinarily too steep to sustain it. Inflation ends when the…

天体物理学 · 物理学 2009-10-31 Edmund J Copeland , Andrew R Liddle , James E Lidsey

We have proposed a new class of inflationary scenarios in which the first stage of expansion is driven by "old" false vacuum inflation. This ends by nucleation of a bubble, which then further inflates. Unlike the standard slow-roll…

高能物理 - 唯象学 · 物理学 2007-05-23 Gia Dvali , Shamit Kachru

The most current observational data corroborate the Starobinsky model as one of the strongest candidates in the description of an inflationary regime. Motivated by such success, extensions of the Starobinsky model have been increasingly…

宇宙学与河外天体物理 · 物理学 2022-03-14 G. Rodrigues-da-Silva , J. Bezerra-Sobrinho , L. G. Medeiros

Higher-order theories of gravity are extensions to general relativity (GR) motivated mainly by high-energy physics searching for GR ultraviolet completeness. They are characterized by the inclusion of correction terms in the…

宇宙学与河外天体物理 · 物理学 2023-11-14 G. Rodrigues-da-Silva , L. G. Medeiros

In a previous paper we proposed a new approach to the beginning of inflation -- a lingering universe. The universe begins in a lingering state with a nearly vanishing Hubble parameter. This calls into question the absolute age of the…

宇宙学与河外天体物理 · 物理学 2025-01-09 Brandon Melcher , Arnab Pradhan , Scott Watson

Inflation is considered as the best theory of the early universe by a very large fraction of cosmologists. However, the validity of a scientific model is not decided by counting the number of its supporters and, therefore, this dominance…

宇宙学与河外天体物理 · 物理学 2019-11-06 Debika Chowdhury , Jerome Martin , Christophe Ringeval , Vincent Vennin

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 this paper, we consider a nonminimal coupling model between gravity and nonlinear electrodynamics with cosmological constant. This cosmological model is designed to account for both the inflationary epoch of the early universe and the…

广义相对论与量子宇宙学 · 物理学 2024-10-10 Chilwatun Nasiroh , Ramy F. Izzah , Fiki T. Akbar , Bobby E. Gunara