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相关论文: Taxonomy of Dark Energy Models

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Dark energy is an elusive concept, which has been introduced two decades ago in order to make the acceleration of the universe a comprehensible phenomenon. However, the nature of this energy is far from being understood, both from a…

高能物理 - 唯象学 · 物理学 2023-07-04 Miguel Hoyuelos , Pablo Sisterna

One of the great endeavors of the past decade has been the evaluation of different observational techniques for measuring dark energy properties and of theoretical techniques for constraining models of cosmic acceleration given cosmological…

宇宙学与河外天体物理 · 物理学 2010-04-28 Eric V. Linder

According to the recent astronomical data, the most part of energy in the Universe is in the 'dark' form, which is effectively described by Lambda-term in Einstein equations. All arguments in favor of the dark energy were obtained so far…

天体物理学 · 物理学 2016-11-15 Yurii V. Dumin

Cosmology is living through fascinating times, where new observations from ground and space telescopes are questioning the established paradigm, the so-called Lambda Cold Dark Matter model. The particle nature of Dark Matter is severely…

宇宙学与河外天体物理 · 物理学 2026-04-15 Juan Garcia-Bellido

To explain the currently observed accelerated expansion of the universe, a large number of different theoretical models are presently being discussed. In one way or another, all of these contain `new physics', though at different levels.…

天体物理学 · 物理学 2015-06-24 Christian Beck

An impressive amount of different astrophysical data converges towards the picture of a spatially flat universe undergoing a today phase of accelerated expansion. The nature of the dark energy dominating the energy content of the universe…

天体物理学 · 物理学 2009-11-10 S. Capozziello , V. F. Cardone , M. Funaro , S. Andreon

The most studied way to explain the current accelerated expansion of the universe is to assume the existence of dark energy; a new component that fill the universe, does not clumps, currently dominates the evolution, and has a negative…

宇宙学与河外天体物理 · 物理学 2015-06-11 Victor H. Cardenas

One of the principal discoveries in modern cosmology is that standard model particles (including baryons, leptons and photons) together comprise only 5% of the mass-energy budget of the Universe. The remaining 95% consists of dark energy…

宇宙学与河外天体物理 · 物理学 2014-03-04 Andrew Pontzen , Fabio Governato

Dark energy is one of the mysteries of modern science. It is unlike any known form of matter or energy and has been detected so far only by its gravitational effect of repulsion. Owing to its effects being discernible only at very very…

宇宙学与河外天体物理 · 物理学 2009-08-25 Aruna Kesavan

Despite two decades of tremendous experimental and theoretical progress, the riddle of the accelerated expansion of the Universe remains to be solved. On the experimental side, our understanding of the possibilities and limitations of the…

The problem of dark energy can be roughly stated as the proposition and validation of a cosmological model that can explain the phenomenon of the accelerated expansion of the Universe. This problem is an open discussion topic in modern…

广义相对论与量子宇宙学 · 物理学 2014-12-19 Genly Leon

Dark matter, the major component of the matter content of the Universe, played a significant role at early stages during structure formation. But at present the Universe is dark energy dominated as well as accelerating. Here, the presence…

天体物理学 · 物理学 2013-09-17 Saibal Ray , Utpal Mukhopadhyay , Farook Rahaman , Ruby Sarkar

Observations provide increasingly strong evidence that the universe is accelerating. This revolutionary advance in cosmological observations confronts theoretical cosmology with a tremendous challenge, which it has so far failed to meet.…

天体物理学 · 物理学 2008-11-26 Ruth Durrer , Roy Maartens

A six parameter cosmological model, involving a vacuum energy density that is extremely tiny compared to fundamental particle physics scales, describes a large body of increasingly accurate astronomical data. In a first part of this brief…

高能物理 - 唯象学 · 物理学 2009-11-11 Norbert Straumann

In this work we explore a model of the universe in which dark energy is modelled explicitely with both a dynamical quintessence field (with a double exponential self-interaction potential) and a cosmological constant. For a given region of…

天体物理学 · 物理学 2007-05-23 Rolando Cardenas , Tame Gonzalez , Osmel Martin , Israel Quiros

Mounting observational data confirm that about 73% of the energy density consists of dark energy which is responsible for the current accelerated expansion of the Universe. We present observational evidences and dark energy projects. We…

宇宙学与河外天体物理 · 物理学 2012-12-20 Jaewon Yoo , Yuki Watanabe

Keeping in mind the current picture of an accelerating and flat Universe, some specific dynamical models of the cosmological term $\Lambda$ have been selected for investigating the nature of dark energy. Connecting the free parameters of…

天体物理学 · 物理学 2008-11-26 Saibal Ray , Utpal Mukhopadhyay , Xin-He Meng

The standard model of cosmology relies on the existence of two components, "dark matter" and "dark energy", which dominate the expansion of the Universe. There is no direct proof of their existence, and their nature is still unknown. Many…

宇宙学与河外天体物理 · 物理学 2014-11-20 Alexandre Arbey

The expansion of the universe has been accepted by scientists for more than a century. However, since the 1990s, observations have suggested that the universe is expanding at an accelerating rate. Although the source of this acceleration is…

泛函分析 · 数学 2017-11-13 Issa Mohamadi

The discovery ten years ago that the expansion of the Universe is accelerating put in place the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark energy. Yet the underlying cause of…

宇宙学与河外天体物理 · 物理学 2009-04-17 Joshua A. Frieman