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相关论文: The Oscillating Universe: an Alternative to Inflat…

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The evolution of a scalar field is explored taking into account the presence of a background fluid in a positively curved Universe in the framework of loop quantum cosmology. Though the mechanism that provides the initial conditions for…

天体物理学 · 物理学 2009-11-13 N. J. Nunes

We consider the oscillating dark energy with periodic equation of state in two equivalent formulations: ideal fluid or scalar-tensor theory. It is shown that such dark energy suggests the natural way for the unification of early-time…

高能物理 - 理论 · 物理学 2009-09-17 Shin'ichi Nojiri , Sergei D. Odintsov

The inflationary scenario has become the paradigm of early universe cosmology, and - in conjuction with ideas from superstring theory - has led to speculations about an "inflationary multiverse". From a point of view of phenomenology, the…

宇宙学与河外天体物理 · 物理学 2012-05-09 Robert Brandenberger

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

Yes, if the universe has compact topology. Inflation is currently the most elegant explanation of why the universe is old, large, nearly flat, homogeneous on large scales and structured on small scales. One of the weaknesses of the…

天体物理学 · 物理学 2009-10-28 Neil J. Cornish , David N. Spergel , Glenn D. Starkman

We investigate the inflationary universe in a theory where two scalar fields non-minimally coupling to the scalar curvature and an extra $R^2$ term exist and the conformal invariance is broken. In particular, the slow-roll inflation is…

高能物理 - 理论 · 物理学 2016-03-01 Kazuharu Bamba

There exists the "entropy problem" of the early universe, that is, why did the universe begin with an extremely low entropy and how did it evolve into such high entropy at late times? It has been long believed that inflation cannot be the…

宇宙学与河外天体物理 · 物理学 2016-02-12 Pisin Chen , Po-Shen Hsin , Yuezhen Niu

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

We analyze the dynamics of a homogeneous and isotropic universe in the Einstein$--$Cartan theory of gravity. The coupling between the spin and torsion prevents gravitational singularities and replaces the Big Bang with a nonsingular big…

广义相对论与量子宇宙学 · 物理学 2019-03-05 Gabriel Unger , Nikodem Popławski

The mechanism for triggering the universe inflation could be that at very early periods the time variable was discrete instead of smooth. Alternatively, and perhaps equivalently, it could be the consequence that the metrics of the early…

高能物理 - 理论 · 物理学 2016-12-28 Laurent Baulieu

This review article aims at presenting the theory of inflation. We first describe the background spacetime behavior during the slow-roll phase and analyze how inflation ends and the Universe reheats. Then, we present the theory of…

高能物理 - 理论 · 物理学 2009-11-10 Jerome Martin

Using numerical solutions of the full Einstein field equations coupled to a scalar inflaton field in 3+1 dimensions, we study the conditions under which a universe that is initially expanding, highly inhomogeneous and dominated by gradient…

高能物理 - 理论 · 物理学 2016-09-07 William E. East , Matthew Kleban , Andrei Linde , Leonardo Senatore

We investigate the inflationary expansion of the universe induced by higher curvature corrections in M-theory. The inflationary evolution of the geometry is discussed in ref.[1], thus we succeed to analyse metric perturbations around the…

高能物理 - 理论 · 物理学 2020-09-15 Kazuho Hiraga , Yoshifumi Hyakutake

Loop quantum cosmology provides a nice solution of avoiding the big bang singularity through a big bounce mechanism in the high energy region. In loop quantum cosmology an inflationary universe is emergent after the big bounce, no matter…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Xin Zhang , Yi Ling

We study a class of non-local, action-based, and purely gravitational models. These models seek to describe a cosmology in which inflation is driven by a large, bare cosmological constant that is screened by the self-gravitation between the…

广义相对论与量子宇宙学 · 物理学 2016-08-17 N. C. Tsamis , R. P. Woodard

After decades of successful hot big-bang paradigm, Cosmology still lacks a framework in which the early inflationary phase of the universe smoothly matches the radiation epoch and evolves to the present `quasi' de Sitter spacetime. No less…

宇宙学与河外天体物理 · 物理学 2015-06-16 S. Basilakos , J. A. S. Lima , J. Solà

The basic workings of inflationary models are summarized, along with the arguments that strongly suggest that our universe is the product of inflation. It is argued that essentially all inflationary models lead to (future-)eternal…

天体物理学 · 物理学 2015-06-24 Alan H. Guth

Slow-roll inflation generically makes several predictions: a flat Universe, primordial adiabatic density perturbations, and a stochastic gravity-wave background. Each inflation model will further predict specific relations between the…

天体物理学 · 物理学 2007-05-23 Marc Kamionkowski

We consider alternative inflationary cosmologies in massive gravity with degenerate reference metrics and study the feasibilities of the emergent universe scenario, bouncing and cyclic universes. We focus on the construction of the Einstein…

广义相对论与量子宇宙学 · 物理学 2019-05-28 Shou-Long Li , H. Lü , Hao Wei , Puxun Wu , Hongwei Yu

The main objective of this study is to investigate the phenomenon of the bouncing scenario of the universe. The most widely recognized cosmological framework is the standard cosmological model, sometimes referred to as the Big Bang model.…

广义相对论与量子宇宙学 · 物理学 2024-02-13 A. S. Agrawal