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相关论文: Coherent Phase Argument for Inflation

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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

An introductory account is given of the inflationary cosmology, which postulates a period of accelerated expansion during the Universe's earliest stages. The historical motivation is briefly outlined, and the modelling of the inflationary…

天体物理学 · 物理学 2007-05-23 Andrew R Liddle

Models of cosmic inflation posit an early phase of accelerated expansion of the universe, driven by the dynamics of one or more scalar fields in curved spacetime. Though detailed assumptions about fields and couplings vary across models,…

宇宙学与河外天体物理 · 物理学 2014-05-09 Alan H. Guth , David I. Kaiser , Yasunori Nomura

Inflationary cosmology explains the homogeneity and large-scale structure of the universe through a brief epoch of accelerated expansion following the Big Bang. Cyclic cosmologies, in contrast, describe a universe undergoing successive…

广义相对论与量子宇宙学 · 物理学 2026-05-18 Kanabar Jay , Maxim Khlopov , Jan Novák

An introductory account is given of the modern understanding of the physics of the early Universe. Particular emphasis is placed on the paradigm of cosmological inflation, which postulates a period of accelerated expansion during the…

天体物理学 · 物理学 2008-02-03 Andrew R Liddle

The hypothesis that the Universe underwent a period of exponential expansion at very early times has become the most popular theory of the early Universe. Not only does it solve some of the problems of standard big bang cosmology, but it…

天体物理学 · 物理学 2007-05-23 Robert H. Brandenberger

I present a brief review of astro-ph/0406099, which argues that there is a limit on the number of efolds of inflation which are observable in a universe which undergoes an eternally accelerated expansion in the future. Such an acceleration…

高能物理 - 理论 · 物理学 2007-05-23 Matthew Kleban

Observations of the cosmic microwave sky are revealing the primordial non-uniformities from which all structure in the Universe grew. The only known physical mechanism for generating the inhomogeneities we see involves the amplification of…

天体物理学 · 物理学 2009-10-31 Neil Turok

The standard model of cosmology is based on the hot Big Bang theory and the inflationary paradigm. Recent precise observations of the temperature and polarization anisotropies in the cosmic microwave background and the matter distribution…

宇宙学与河外天体物理 · 物理学 2010-04-02 Juan Garcia-Bellido

The standard model of cosmology is based on the hot Big Bang theory and the inflationary paradigm. Recent precise observations of the temperature and polarization anisotropies in the cosmic microwave background and the matter distribution…

高能物理 - 唯象学 · 物理学 2016-10-05 Juan Garcia-Bellido

Inflation has been the driving idea in cosmology for two decades and is a pillar of the New Cosmology. The inflationary paradigm has now passed its first round of significant tests, with two of its three basics predictions confirmed at…

天体物理学 · 物理学 2014-10-13 Michael S. Turner

With the recent measurements of temperature and polarization anisotropies in the microwave background by WMAP, we have entered a new era of precision cosmology, with the cosmological parameters of a Standard Cosmological Model determined to…

高能物理 - 唯象学 · 物理学 2007-05-23 Juan Garcia-Bellido

An exact inhomogeneous solution of Einstein's field equations is shown to be able to inflate in a non-uniform way in the early universe and explain anomalies in the WMAP power spectrum data. It is also possible for the model to explain the…

天体物理学 · 物理学 2007-06-13 J. W. Moffat

In inflation cosmologies, cosmic structure develops through the gravitational instability of the inevitable quantum noise in primordial scalar fields. I show how the acceleration of the universe defines the shape of the primordial spectrum…

天体物理学 · 物理学 2009-09-25 J. Richard Bond

The early Universe inflation is well known as a promising theory to explain the origin of large scale structure of the Universe, a causal theory for the origin of primordial density fluctuations which may explain the observed density…

天体物理学 · 物理学 2007-05-23 Xin-he Meng

Inflation provides a natural mechanism to account for the origin of cosmic structures. The generation of primordial inhomogeneities during inflation can be understood via the spontaneous creation of quanta from the vacuum. We show that when…

宇宙学与河外天体物理 · 物理学 2015-05-28 Ivan Agullo , Leonard Parker

The early Universe inflation is well known as a promising theory to explain the origin of large scale structure of Universe and to solve the early universe pressing problems. For a resonable inflation model, the potential during inflation…

高能物理 - 唯象学 · 物理学 2007-05-23 Xin He Meng

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

Inflation has been the leading early universe scenario for two decades, and has become an accepted element of the successful `cosmic concordance' model. However, there are many puzzling features of the resulting theory. It requires both…

高能物理 - 理论 · 物理学 2009-11-10 Neil Turok , Paul J. Seinhardt

Cosmic inflation provides a window to the highest energy densities accessible in nature, far beyond those achievable in any realistic terrestrial experiment. Theoretical insights into the inflationary era and its observational probes may…

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