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相关论文: Cosmic acceleration from effective forces?

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The current accelerated expansion of our universe could be due to an unknown energy component with negative pressure (dark energy) or a modification to general relativity (modified gravity). On the other hand, recently warm dark matter…

宇宙学与河外天体物理 · 物理学 2025-03-28 Hao Wei , Jing Liu , Zu-Cheng Chen , Xiao-Peng Yan

The discovery that the expansion of the universe is accelerating in time is a major discovery which still awaits adequate explanation. It is generally agreed that this implies a cosmic repulsion as a result of the existence of a…

综合物理 · 物理学 2008-11-26 R. F. O'Connell

In this paper we present an alternative explanation to the acceleration of the universe and the dark energy problems in terms of the Friedmann Thermodynamics. This model has the capability of making definite predictions in-line with the…

天体物理学 · 物理学 2007-05-23 Selcuk Bayin

Phenomena currently attributed to Dark Matter (DM) and Dark Energy (DE) are merely a result of the interplay between gravitational energy density, caused by the contraction of space by matter, and space dilation, caused by the energy…

天体物理学 · 物理学 2008-10-23 Shlomo Barak , Elia M. Leibowitz

A new cosmic scenario with gravitationally induced particle creation is proposed. In this model the Universe evolves from an early to a late time de Sitter era, with the recent accelerating phase driven only by the negative creation…

广义相对论与量子宇宙学 · 物理学 2015-06-22 J. A. S. Lima , L. L. Graef , D. Pavón , S. Basilakos

Geometrothermodynamics is a geometric theory which combines thermodynamics with contact and Riemannian geometry. In this work we use the formalism of geometrothermodynamics to infer cosmological models which predict the observed speed up.…

广义相对论与量子宇宙学 · 物理学 2025-11-12 Alessandro Bravetti , Orlando Luongo

In this work, I develop an alternative explanation for the acceleration of the cosmic expansion, which seems to be a result of recent high redshift Supernova data. In the current interpretation, this cosmic acceleration is explained by…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. -F. Pascual-Sánchez

General relativity can be reconciled with quantum field theory without quantising the geometry only if the metric evolves stochastically. In this article, we explore the consequences of such a proposal at early cosmological times. We find…

广义相对论与量子宇宙学 · 物理学 2026-05-29 Jonathan Oppenheim , Emanuele Panella , Andrew Pontzen

In the past decade or so observations of supernovae, Large Scale Structures (LSS), and the Cosmic Microwave Background (CMB) have confirmed the presence of what is called dark energy - the cause of accelerating expansion of the Universe.…

宇宙学与河外天体物理 · 物理学 2012-08-14 Houri Ziaeepour

In this paper, we examine dynamical friction at galactic scales within the framework of coupled dark energy. This model posits dark energy as coupled quintessence, which maintains a minimal coupling to gravity but interacts non-minimally…

星系天体物理 · 物理学 2025-02-18 Nasrin Nari , Mahmood Roshan

The Einstein equation in a semi-classical approximation is applied to a spherical region of the universe, with the stress-energy tensor consisting of the mass density and pressure of the LambdaCDM cosmological model plus an additional…

广义相对论与量子宇宙学 · 物理学 2024-12-11 Emilio Santos

A new model of accelerating expansion of the universe is presented. A de Sitter solution in vacuum and a exact solution with the dust mater source are obtained. A new explanation of the acceleration of the cosmic expansion is given. In is…

综合物理 · 物理学 2013-01-16 G. Y. Chee

In this (second) part of the work we present the results of numerical and qualitative analysis, based on a new model of the Archimedean-type interaction between dark matter and dark energy. The Archimedean-type force is linear in the…

广义相对论与量子宇宙学 · 物理学 2011-02-28 Alexander B. Balakin , Vladimir V. Bochkarev

In this paper we introduce the fractional dark energy model, in which the accelerated expansion of the Universe is driven by a nonrelativistic gas (composed by either fermions or bosons) with a noncanonical kinetic term. The kinetic energy…

宇宙学与河外天体物理 · 物理学 2021-04-20 Ricardo G. Landim

We investigate the clustering properties of a dynamical dark energy component. In a cosmic mix of a pressureless fluid and a light scalar field, we follow the linear evolution of spherical matter perturbations. We find that the scalar field…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Sourish Dutta , Irit Maor

There is now strong evidence that the main contribution to the cosmic energy density is not due to matter, but to another component with negative pressure. Its nature is still unknown: it could be the vacuum energy, manifesting itself as a…

天体物理学 · 物理学 2007-05-23 Alberto Cappi

The Lambda-Cold Dark Matter (LCDM) model agrees with most of the cosmological observations, but has some hindrances from observed data at smaller scales such as galaxies. Recently, Berezhiani and Khoury (2015) proposed a new theory…

广义相对论与量子宇宙学 · 物理学 2020-07-22 Shreya Banerjee , Sayantani Bera , David F. Mota

A possible slowing down of the cosmic expansion is investigated through a cosmographic approach. By expanding the luminosity distance to fourth order and fitting the SN Ia data from the most recent compilations (Union, Constitution and…

宇宙学与河外天体物理 · 物理学 2015-03-17 Antonio C. C. Guimarães , José Ademir S. Lima

The accelerating expansion of the universe is the most surprising cosmological discovery in many decades. In this short review, we briefly summarize theories for the origin of cosmic acceleration and the observational methods being used to…

宇宙学与河外天体物理 · 物理学 2014-01-03 Michael J. Mortonson , David H. Weinberg , Martin White

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