中文
相关论文

相关论文: Explain cosmic acceleration? First, correct Einste…

200 篇论文

The acceleration of the universe is described as a dynamical effect of the extrinsic curvature of space-time. By extending previous results, the extrinsic curvature is regarded as an independent spin-2 field, determined by a set of…

宇宙学与河外天体物理 · 物理学 2009-05-27 M. D. Maia , A. J. S. Capistrano , J. S. Alcaniz , E. M. Monte

Modern astrophysical and cosmological models are plagued with two severe theoretical difficulties, namely, the dark energy and the dark matter problems. Relative to the former, high-precision observational data have confirmed with startling…

广义相对论与量子宇宙学 · 物理学 2015-05-05 Francisco S. N. Lobo

There is general agreement that the universe began with an "explosion" of matter and energy at a "singularity", the "Big Bang". This paper analyses the mechanics of that beginning and two alternative theories related to it: - The…

综合物理 · 物理学 2007-05-23 Roger Ellman

A refined version of a recently introduced method for analysing the dynamics of an inhomogeneous irrotational dust universe is presented. A fully non-perturbative numerical computation of the time dependence of volume in this framework…

宇宙学与河外天体物理 · 物理学 2014-10-01 Harald Skarke

As an explanation for the acceleration of the universe, we propose dark matter with self-interactions characterized by a negative pressure; there is no vacuum energy whatsoever in this Cardassian model. These self-interactions may arise due…

高能物理 - 唯象学 · 物理学 2007-05-23 Paolo Gondolo , Katherine Freese

We show that, due to the nonlinear nature of gravity, fluctuations in spacetime curvature generate additional gravitational attraction. This fluctuation-induced extra attraction was overlooked in the conventional understanding of the…

广义相对论与量子宇宙学 · 物理学 2024-01-09 Qingdi Wang

We have observed the acceleration of the expansion of the universe. To explain this phenomenon, we usually introduce the dark energy (DE) which has a negative pressure or we need to modify the Einstein's equation to produce a term which is…

宇宙学与河外天体物理 · 物理学 2011-11-04 Dong-Biao Kang

Homogeneous cosmological solutions are obtained in five dimensional space time assuming equations of state $ p = k\rho $ and $ p_{5}= \gamma\rho$ where p is the isotropic 3 - pressure and $p_{5}$, that for the fifth dimension. Using…

广义相对论与量子宇宙学 · 物理学 2009-11-11 D. Panigrahi , Y. Z. Zhang , S. Chatterjee

We have assumed that in a physical universe a blackhole is created some where. We conjecture that this blackhole will then separate itself from the physical universe and will build up an extra dimensional entity associated with the physical…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. M. Harunar Rashid , Arshad Momen , A. L. Choudhury

Gravitational repulsion is an inherent aspect of the Schwarzschild solution of the Einstein-Hilbert field equations of general relativity. We show that this circumstance means that it is possible to gravitationally accelerate particles to…

高能天体物理现象 · 物理学 2018-02-26 Charles H. McGruder

We suggest the possibility that the mysterious dark energy component driving the acceleration of the Universe is the leading term, in the de Sitter temperature, of the free energy density of space-time seen as a quantum gravity coherent…

广义相对论与量子宇宙学 · 物理学 2014-04-03 Luciano Vanzo

The principles of General Relativity allow for a non-vanishing cosmological constant, which can possibly be interpreted at least partially in terms of quantum-fluctuations of matter fields. Depending on sign and magnitude it can cause…

天体物理学 · 物理学 2007-05-23 Domenico Giulini , Norbert Straumann

Cosmic acceleration is widely believed to require either a source of negative pressure (i.e., dark energy), or a modification of gravity, which necessarily implies new degrees of freedom beyond those of Einstein gravity. In this paper we…

高能物理 - 理论 · 物理学 2017-06-28 Lasha Berezhiani , Justin Khoury , Junpu Wang

Cosmic backreaction as an additional source of the expansion of the universe has been a debate topic since the discovery of cosmic acceleration. The major concern is whether the self interaction of small-scale nonlinear structures would…

宇宙学与河外天体物理 · 物理学 2019-07-10 Zhiqi Huang , Han Gao , Haoting Xu

A solution to Einstein's field equations via the Friedman equations is shown to produce a cosmological model that is in exact agreement with the measurements made by the dark energy astronomers. All the essential physical parameters are…

综合物理 · 物理学 2012-06-26 James G. Gilson

The origin of negative pressure fluid (the dark energy) is investigated in the quantum model of the homogeneous, isotropic and closed universe filled with a uniform scalar field and a perfect fluid which defines a reference frame. The…

广义相对论与量子宇宙学 · 物理学 2008-12-19 V. E. Kuzmichev , V. V. Kuzmichev

We show that in imaginary time quantum metric fluctuations of empty space form a self-consistent de Sitter gravitational instanton that can be thought of as describing tunneling from "nothing" into de Sitter space of real time (no…

广义相对论与量子宇宙学 · 物理学 2015-06-04 Leonid Marochnik

Einstein's Field Equations have proven applicable across many scales, from black holes to cosmology. Even the mysterious Cosmological Constant found a physical interpretation in the so-called ``dark energy'' causing the accelerated cosmic…

广义相对论与量子宇宙学 · 物理学 2024-05-15 Jenny Wagner

We investigate the gravitational property of the quantum vacuum by treating its large energy density predicted by quantum field theory seriously and assuming that it does gravitate to obey the equivalence principle of general relativity. We…

广义相对论与量子宇宙学 · 物理学 2019-04-22 Qingdi Wang , Zhen Zhu , William G. Unruh

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