中文
相关论文

相关论文: Dark Energy predictions from GREA: Background and …

200 篇论文

The acceleration of the universe can be explained either through dark energy or through the modification of gravity on large scales. In this paper we investigate modified gravity models and compare their observable predictions with dark…

天体物理学 · 物理学 2008-11-26 Edmund Bertschinger , Phillip Zukin

The Abnormally Weighting Energy (AWE) hypothesis consists of assuming that the dark sector of cosmology violates the weak equivalence principle (WEP) on cosmological scales, which implies a violation of the strong equivalence principle for…

天体物理学 · 物理学 2008-11-26 A. Fuzfa , J. -M. Alimi

Observations of distant supernovae indicate that the Universe is now in a phase of accelerated expansion the physical cause of which is a mystery. Formally, this requires the inclusion of a term acting as a negative pressure in the…

In this essay, I present an alternative explanation for the cosmic acceleration which appears as a consequence of recent high redshift Supernova data. In the usual interpretation, this cosmic acceleration is explained by the presence of a…

广义相对论与量子宇宙学 · 物理学 2009-10-31 J. -F. Pascual-Sánchez

A phenomenological formalism is presented in which the apparent acceleration of the universe is generated by cosmic structure formation, without resort to Dark Energy, modifications to gravity, or a local void. The observed acceleration…

宇宙学与河外天体物理 · 物理学 2015-06-05 Brett Bochner

General Relativity (GR) is a phenomenologically successful theory that rests on firm foundations, but has not been tested on cosmological scales. The advent of dark energy (and possibly even the requirement of cold dark matter), has…

广义相对论与量子宇宙学 · 物理学 2010-05-12 Constantinos Skordis

In a recent paper \cite{Artymowski:2020zwy} we suggested the possibility that the present acceleration of the Universe is due to thermodynamical behavior of unparticles. The model is free of scalar fields, modified gravity, a Cosmological…

宇宙学与河外天体物理 · 物理学 2022-10-19 Michał Artymowski , Ido Ben-Dayan , Utkarsh Kumar

The acceleration of the expansion of the universe represents one of the major challenges to our current understanding of fundamental physics. In principle, to explain this phenomenon, at least two different routes may be followed: either…

天体物理学 · 物理学 2009-11-10 J. S. Alcaniz , Zong-Hong Zhu

There is now strong evidence that the current energy density of the Universe is dominated by dark energy with an equation of state w<-1/3, which is causing accelerated expansion. The build-up of structure within such Universes is subject to…

天体物理学 · 物理学 2008-11-26 Will J. Percival

The novel idea is that the undergoing accelerated expansion of the universe happens due to infrared quantum gravity modifications at intermediate astrophysical scales of galaxies or galaxy clusters, within the framework of Asymptotically…

广义相对论与量子宇宙学 · 物理学 2021-02-16 Fotios K. Anagnostopoulos , Georgios Kofinas , Vasilios Zarikas

The current standard cosmological model is constructed within the framework of general relativity with a cosmological constant $\Lambda$, which is often associated with dark energy, and phenomenologically explains the accelerated cosmic…

广义相对论与量子宇宙学 · 物理学 2023-06-27 Jiamin Hou , Julian Bautista , Maria Berti , Carolina Cuesta-Lazaro , César Hernández-Aguayo , Tilman Tröster , Jinglan Zheng

The problem of explaining the acceleration of the expansion of the universe and the observational and theoretical difficulties associated with dark matter and dark energy are discussed. The possibility that GR does not correctly describe…

天体物理学 · 物理学 2007-05-23 J. W. Moffat

The gravitational equations were derived in general relativity (GR) using the assumption of their covariance relative to arbitrary transformations of coordinates. It has been repeatedly expressed an opinion over the past century that such…

广义相对论与量子宇宙学 · 物理学 2024-08-07 Alexander P. Sobolev

The standard procedure to explain the accelerated expansion of the Universe is to assume the existence of an exotic component with negative pressure, generically called dark energy. Here, we propose a new accelerating flat cosmology without…

宇宙学与河外天体物理 · 物理学 2025-02-21 P. W. R. Lima , J. A. S. Lima , J. F. Jesus

Below scales of about 100/h Mpc our universe displays a complex inhomogeneous structure dominated by voids, with clusters of galaxies in sheets and filaments. The coincidence that cosmic expansion appears to start accelerating at the epoch…

宇宙学与河外天体物理 · 物理学 2011-02-11 David L. Wiltshire

Modern astrophysical and cosmological models are faced with two severe theoretical difficulties, that can be summarized as the dark energy and the dark matter problems. Relative to the former, it has been stated that cosmology has entered a…

广义相对论与量子宇宙学 · 物理学 2013-08-23 Francisco S. N. Lobo

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

Following the holographic principle, which suggests that the energy density of dark energy may be proportional inversely to the area of the event horizon of the Universe, we have proposed a new energy density of dark energy through the…

广义相对论与量子宇宙学 · 物理学 2023-01-25 H. R. Fazlollahi

One of the biggest mysteries in cosmology is Dark Energy, which is required to explain the accelerated expansion of the universe within the standard model. But maybe one can explain the observations without introducing new physics, by…

宇宙学与河外天体物理 · 物理学 2012-11-09 Christoph Saulder , Steffen Mieske , Werner W. Zeilinger

Extensions of Einstein's General Relativity (GR) can formally be given a GR structure in which additional geometric degrees of freedom are mapped on an effective energy-momentum tensor. The corresponding effective cosmic medium can then be…

宇宙学与河外天体物理 · 物理学 2019-03-11 Winfried Zimdahl , Hermano Velten , William C. Algoner