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相关论文: Self-accelerated Universe

200 篇论文

We present a cosmological model with a solution that self-accelerates at late-times without signs of ghost instabilities on small scales. The model is a natural extension of the Brans-Dicke (BD) theory including a non-linear derivative…

宇宙学与河外天体物理 · 物理学 2010-01-08 Fabio P Silva , Kazuya Koyama

The acceleration of the expansion of the universe arises from unknown physical processes involving either new fields in high energy physics or modifications of gravitation theory. It is crucial for our understanding to characterize the…

天体物理学 · 物理学 2009-11-10 Eric V. Linder

The cosmological constant, which was introduced by Einstein a century ago to allow for a static universe, experienced a revival two decades ago under the label dark energy as a parameter to model the observed accelerated expansion of the…

综合物理 · 物理学 2019-01-08 Jan O. Stenflo

In a recent paper (Phys. Rev. D95, 103504 (2017)) it is argued that, due to the fluctuations around its mean value, vacuum energy gravitates differently from what previously assumed. As a consequence, the universe would accelerate with a…

广义相对论与量子宇宙学 · 物理学 2018-03-14 Francisco D. Mazzitelli , Leonardo G. Trombetta

The universe appears to be accelerating, but the reason why is a complete mystery. The simplest explanation, a small vacuum energy (cosmological constant), raises three difficult issues: why the vacuum energy is so small, why it is not…

天体物理学 · 物理学 2009-07-09 Sean M. Carroll

Intrinsic properties of the space itself and quantum fluctuations of its geometry are sufficient to provide a mechanism for the acceleration of cosmological expansion (dark energy effect). Applying Bogoliubov-Born-Green-Kirkwood-Yvon…

广义相对论与量子宇宙学 · 物理学 2013-06-27 Leonid Marochnik , Daniel Usikov , Grigory Vereshkov

Acceleration of the universe is obtained from a model of non-relativistic particles with a short-range attractive interaction, at low enough temperature to produce a Bose-Einstein condensate. Conditions are derived for negative-pressure…

天体物理学 · 物理学 2015-05-13 German Izquierdo , Jaime Besprosvany

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 redshift of galaxies is in general explained by the expansion of space. The flat space time theory of gravitation suggests an additional interpretation. In this theory gravitation is explained analogously to Maxwell's theory on a flat…

综合物理 · 物理学 2007-05-31 Walter Petry

We present an exact solution to the equations of massive gravity that displays cosmological constant-like behavior for any spherically symmetric distribution of matter, including arbitrary time dependence. On this solution, the new degrees…

高能物理 - 理论 · 物理学 2012-11-22 Pierre Gratia , Wayne Hu , Mark Wyman

The observation that Type Ia supernovae are fainter than expected given their red shifts has led to the conclusion that the expansion of the universe is accelerating. The widely accepted hypothesis is that this acceleration is caused by a…

宇宙学与河外天体物理 · 物理学 2010-07-09 Rutger Dungan , Harrison B. Prosper

We explain an accelerated expansion of the present universe, suggested from observations of supernovae of type Ia at high redshift, by introducing an anti-frictional force that is self-consistently exerted on the particles of the cosmic…

天体物理学 · 物理学 2008-11-26 Winfried Zimdahl , Dominik J. Schwarz , Alexander B. Balakin , Diego Pavon

Recent observations on the redshift and magnitude of distant supernovae have raised fundamental questions of the cosmological structure and the development of space. Interpretation of the observations with the standard cosmology model…

天体物理学 · 物理学 2007-05-23 Tuomo Suntola , Robert Day

The 2nd law of thermodynamics is used to shed light on present-day puzzles in cosmology. The universal law, given as an equation of motion, describes diverse systems when consuming free energy via various mechanisms to attain stationary…

综合物理 · 物理学 2012-06-20 Arto Annila

Possible effects are considered which would be caused by a hypothetical superstrong interaction of photons or massive bodies with single gravitons of the graviton background. If full cosmological redshift magnitudes are caused by the…

天体物理学 · 物理学 2015-06-24 Michael A. Ivanov

An attempt is made to explain the spiral structure of spiral galaxies through a possible rotation of the Universe. To this end, we write down a possible form of the metric, and we calculate the necessary quantities (Rik, Tik, ...) in order…

天体物理学 · 物理学 2009-04-27 Evangelos Chaliasos

A central theme in cosmology is the perplexing fact that the Universe is undergoing an accelerating expansion. The latter, one of the most important and challenging current problems in cosmology, represents a new imbalance in the governing…

广义相对论与量子宇宙学 · 物理学 2011-09-28 Francisco S. N. Lobo

The Universe is filled with relic neutrinos, remnants from the Leptonic Era. Since the formation of galaxies started, gravitation has modified the Fermi-Dirac momentum distribution of these otherwise decoupled particles. Decelerated…

天体物理学 · 物理学 2007-05-23 Richard Wigmans

We consider a possible connection between matter and cosmological constant $\Lambda$ via the Newtonian cosmic potential of the matter within the expanding particle horizon. Consistent with GR, an increasing potential may drive the metric…

综合物理 · 物理学 2014-05-30 Herman Telkamp

Nearly 4 years ago, two teams of observational astronomers reported that high-redshift Type Ia supernovae are fainter than expected in a decelerating or freely coasting universe. The radical conclusion that the universe has been…

天体物理学 · 物理学 2009-11-07 Alexei V. Filippenko