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相关论文: A Unifying Theory of Dark Energy and Dark Matter: …

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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

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

In the standard cosmological model, the Universe consists mainly of two invisible substances: vacuum energy with constant mass-density rho_v=\Lambda/(8pi G) (where Lambda is a `cosmological constant' originally proposed by Einstein and G is…

宇宙学与河外天体物理 · 物理学 2015-06-18 Matthew G. Walker , Abraham Loeb

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

A recent study by Farnes (2018) proposed an alternative cosmological model in which both dark matter and dark energy are replaced with a single fluid of negative mass. This paper presents a critical review of that model. A number of…

宇宙学与河外天体物理 · 物理学 2019-06-05 Hector Socas-Navarro

Physics invites the idea that space contains energy whose gravitational effect approximates that of Einstein's cosmological constant, Lambda; nowadays the concept is termed dark energy or quintessence. Physics also suggests the dark energy…

天体物理学 · 物理学 2008-11-26 P. J. E. Peebles , Bharat Ratra

A model for gravitational collapse where the event horizon is a quantum critical phase transition is extended to provide an explanation for the origin of the observable universe, where the expanding universe that we observe today was…

广义相对论与量子宇宙学 · 物理学 2016-02-09 George Chapline , James Barbieri

Motivated by results implying that the constituents of dark matter (DM) might be collisional, we consider a cosmological (toy-) model, in which the DM itself possesses some sort of thermodynamic properties. In this case, not only can the…

广义相对论与量子宇宙学 · 物理学 2015-03-19 Kostas Kleidis , Nicholas K. Spyrou

To explain the acceleration of the cosmological expansion researchers have considered an unusual form of mass-energy generically called dark energy. Dark energy has a ratio of pressure over mass density which obeys $w=p/\rho <-1/3$. This…

高能物理 - 理论 · 物理学 2008-12-19 Max Chaves , Douglas Singleton

The traditional "explanation" for the observed acceleration of the universe is the existence of a positive cosmological constant. However, this can hardly be a truly convincing explanation, as an expanding universe is not expected to have a…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Joan Sola

The existence of dark matter and dark energy in cosmology is implied by various observations, however, they are still unclear because they have not been directly detected. In this Letter, an unified model of dark energy and dark matter that…

宇宙学与河外天体物理 · 物理学 2016-10-27 Jiro Matsumoto

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 Cosmological Constant Lambda, a concept introduced by Einstein in 1917, has been with us ever since in different variants and incarnations, including the broader concept of Dark Energy. Current observations are consistent with a value…

科普物理 · 物理学 2020-12-30 Ofer Lahav

The observed excess of gravitational forces in galaxies and galactic clusters is usually referred as the existence of "dark matter particles" of unknown origin. An alternative explanation of the dark matter effect is presented here by…

宇宙学与河外天体物理 · 物理学 2011-10-04 Arkady Z. Dolginov

This paper deals with the cancellation mechanism, which identifies the energy density of space-time expansion in an empty universe with the zero-point energy density and avoids the scale discrepancy with the observed energy density…

综合物理 · 物理学 2018-06-12 Christian Henke

More than sixty years ago Zwicky made the case that the great clusters of galaxies are held together by the gravitational force of unseen (dark) matter. Today, the case is stronger and more precise: Dark, nonbaryonic matter accounts for 30%…

天体物理学 · 物理学 2016-11-23 Michael S. Turner

A new kind of accelerating flat model with no dark energy that is fully dominated by cold dark matter (CDM) is investigated. The number of CDM particles is not conserved and the present accelerating stage is a consequence of the negative…

天体物理学 · 物理学 2014-11-18 J. A. S. Lima , F. E. Silva , R. C. Santos

A disk-shaped universe (encompassing the observable universe) rotating globally with an angular speed equal to the Hubble constant is postulated. It is shown that dark energy and dark matter are cosmic inertial effects resulting from such a…

综合物理 · 物理学 2016-06-03 Serkan Zorba

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

Within the standard cosmological scenario the Universe is found to be filled by obscure components (dark matter and dark energy) for ~95% of its energy budget. In particular, almost all the matter content in the Universe is given by dark…

宇宙学与河外天体物理 · 物理学 2015-06-04 Crescenzo Tortora , Philippe Jetzer , Nicola R. Napolitano
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