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Recent astrophysical observations indicate that the universe is composed of a large amount of dark energy (DE) responsible for an accelerated expansion of the universe, along with a sizeable amount of cold dark matter (CDM), responsible for…

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

The present day astrophysical observations indicate that the universe is composed of a large amount of dark energy (DE) responsible for an accelerated expansion of the universe, along with a sizeable amount of cold dark matter (CDM),…

The nature of dark matter (DM) and dark energy (DE) which is supposed to constitute about 95% of the energy density of the universe is still a mystery. There is no shortage of ideas regarding the nature of both. While some candidates for DM…

综合物理 · 物理学 2017-08-25 Kenath Arun , S. B. Gudennavar , C Sivaram

The nature of the main constituents of the mass of the universe is one of the outstanding riddles of cosmology and astro-particle physics. Current models explaining the evolution of the universe, and measurements of the various components…

天体物理学 · 物理学 2017-08-23 Viktor Zacek

Dark energy in the universe is assumed to be vacuum energy. The energy-momentum of vacuum is described by a scale-dependent cosmological constant. The equations of motion imply for the density of matter (dust) the sum of the usual matter…

综合物理 · 物理学 2008-11-09 Walter Petry

[A brief review intended for a general physics colloquium audience.] Astrophysicists now know that 80% of the matter in the universe is `dark matter', composed of neutral and weakly interacting elementary particles that are not part of the…

高能物理 - 唯象学 · 物理学 2008-11-26 Michael E. Peskin

It is generally assumed that the two dark components of the energy density of the universe, a smooth component called dark energy and a fluid of nonrelativistic weakly interacting particles called dark matter, are independent of each other…

天体物理学 · 物理学 2007-05-23 Mark B. Hoffman

Dark Matter (DM) being the vital ingredient in the cosmos, still remains a mystery. Standard assumption is that the collisionless cold dark matter (CCDM) particles are represented by some weakly interacting fundamental fields which can not…

天体物理学 · 物理学 2009-11-11 Ariel Zhitnitsky

In this article, we review a series of recent theoretical results regarding a conventional approach to the dark energy (DE) concept. This approach is distinguished among others for its simplicity and its physical relevance. By compromising…

宇宙学与河外天体物理 · 物理学 2016-04-20 Kostas Kleidis , Nikolaos K. Spyrou

Theoretical results on a conventional approach to the dark energy (DE) concept are reviewed and discussed. According to them, there is absolutely no need for a novel DE component in the Universe, provided that the associated matter-energy…

广义相对论与量子宇宙学 · 物理学 2023-06-19 Kostas Kleidis , Nikolaos K. Spyrou

Dark matter, proposed decades ago as a speculative component of the universe, is now known to be the vital ingredient in the cosmos, eight times more abundant than ordinary matter, one quarter of the total energy density and the component…

天体物理学 · 物理学 2009-09-15 Jeremiah P. Ostriker , Paul J. Steinhardt

Cold Dark Matter (CDM) has become the standard modern theory of cosmological structure formation. Its predictions appear to be in good agreement with data on large scales, and it naturally accounts for many properties of galaxies. But…

天体物理学 · 物理学 2007-05-23 Joel R. Primack

The standard model of particle physics is marvelously successful. However, it is obviously not a complete or final theory. I shall argue here that the structure of the standard model gives some quite concrete, compelling hints regarding…

高能物理 - 唯象学 · 物理学 2009-10-28 Frank Wilczek

The universe is composed of ordinary matter (for example, stars, planets, ourselves), dark matter and dark energy. The estimated percentage of dark matter is about $27\%$ of the entire universe, while $5\%$ is ordinary matter and the…

科普物理 · 物理学 2023-06-05 Alessandra Celletti

We point out that current constraints on dark matter imply only that the majority of dark matter is cold and collisionless. A subdominant fraction of dark matter could have much stronger interactions. In particular, it could interact in a…

高能物理 - 唯象学 · 物理学 2013-08-06 JiJi Fan , Andrey Katz , Lisa Randall , Matthew Reece

Dark matter in the universe seems to be one of the most important puzzles science has to face in this moment. In this essay we point out that dark matter could be a spin-0 fundamental interaction of Nature rather than a simple particle.…

天体物理学 · 物理学 2010-12-09 T. Matos , L. A. Urena-Lopez

The Standard Model of cosmology of the 1980's was based on a remarkable interplay of ideas from particle theory, experiment and astrophysical observations. That model is now dead, and has been replaced by something far more bizarre.…

天体物理学 · 物理学 2007-05-23 Lawrence M. Krauss

There is something unknown in the cosmos. Something big. Which causes the acceleration of the Universe expansion, that is perhaps the most surprising and unexpected discovery of the last decades, and thus represents one of the most pressing…

综合物理 · 物理学 2013-04-18 M. Villata

The Standard Model of cosmology states a surprising composition of the Universe, in which ordinary matter accounts for less than 5%. The remaining 95% are composed of ~70% Dark Energy and ~25% Dark Matter. However, those two components have…

天体物理学 · 物理学 2008-11-14 A. Benoit-Lévy , G. Chardin
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