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We show that loop quantum gravity suffers from a potential problem with non-locality, coming from a mismatch between micro-locality, as defined by the combinatorial structures of their microscopic states, and macro-locality, defined by the…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Fotini Markopoulou , Lee Smolin

In this thesis we are interested in the problem of dark energy in cosmology. In particular, we consider the possibility that this effect is due to an infrared non-local modification of the theory of General Relativity. Inspired by massive…

广义相对论与量子宇宙学 · 物理学 2016-04-26 Ermis Mitsou

A novel idea is proposed for a natural solution of the dark energy and its cosmic coincidence problem. The existence of local antigravity sources, associated with astrophysical matter configurations distributed throughout the universe, can…

广义相对论与量子宇宙学 · 物理学 2018-07-04 Georgios Kofinas , Vasilios Zarikas

The accelerating expansion of universe can be described by the non-zero cosmological constant or the dark energy. However, the origin of the dark energy remains a mystery of modern physics. The local Lorentz invariance is the most exact…

广义相对论与量子宇宙学 · 物理学 2018-10-16 Jiayin Shen , Xun Xue

The Schr\"odinger-Newton equation is a proposed model to explain the localization of macroscopic particles by suppressing quantum dispersion with the particle's own gravitational attraction. On cosmic scales, however, dark energy also acts…

广义相对论与量子宇宙学 · 物理学 2020-04-01 Kelvin , Kelvin Onggadinata , Matthew J. Lake , Tomasz Paterek

We argue that discreteness at the Planck scale (naturally expected to arise from quantum gravity) might manifest in the form of minute violations of energy-momentum conservation of the matter degrees of freedom when described in terms of…

广义相对论与量子宇宙学 · 物理学 2019-06-12 Alejandro Perez , Daniel Sudarsky

A mildly inhomogeneous universe with a cosmological constant may look like it contains evolving dark energy. We show that could be the case by modelling the inhomogeneities and their effects in three different ways: as clumped matter…

宇宙学与河外天体物理 · 物理学 2026-01-29 Yonadav Barry Ginat , Pedro G. Ferreira

The fact that the energy densities of dark energy and matter are similar currently, known as the coincidence problem, is one of the main unsolved problems of cosmology. We present here a model in which a spatial curvature of the universe…

天体物理学 · 物理学 2009-11-13 Urbano Franca

In this paper, we give a conceptual explanation of dark energy as a small negative residual scalar curvature present even in empty spacetime. This curvature ultimately results from postulating a discrete spacetime geometry, very closely…

数学物理 · 物理学 2012-08-16 Aaron Trout

While observational cosmology has recently progressed fast, it revealed a serious dilemma called dark energy: an unknown source of exotic energy with negative pressure driving a current accelerating phase of the universe. All attempts so…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Martin Bojowald

In this letter, we consider the possibility of reconciling metric theories of gravitation with violation of the conservation of energy-momentum. Under some circumstances, this can be achieved in the context of unimodular gravity, and it…

广义相对论与量子宇宙学 · 物理学 2017-01-18 Thibaut Josset , Alejandro Perez , Daniel Sudarsky

The unexpected discovery of the accelerated cosmic expansion in 1998 has filled the Universe with the embarrassing presence of an unidentified "dark energy", or cosmological constant, devoid of any physical meaning. While this standard…

宇宙学与河外天体物理 · 物理学 2013-02-14 M. Villata

We review the evidence for recently accelerating cosmological expansion or "dark energy", either a negative pressure constituent in General Relativity (Dark Energy) or modified gravity (Dark Gravity), without any Dark Energy constituent. If…

天体物理学 · 物理学 2007-05-23 Sidney Bludman

We give a well-motivated explanation for the origin of dark energy, claiming that it arises from a small residual negative scalar-curvature present even in empty spacetime. The vacuum has this residual curvature because spacetime is…

数学物理 · 物理学 2012-08-16 Aaron D. Trout

The observed cosmic acceleration was attributed to an exotic dark energy in the framework of classical general relativity. The dark energy behaves very similar with vacuum energy in quantum mechanics. However, once the quantum effects are…

综合物理 · 物理学 2015-06-17 M. J. Luo

We explore the theoretical possibility that dark energy density is derived from the vacuum particle pairs together with the quantum fluctuation of space-time. By assuming the vacuum particle pairs fall into the horizon boundary of the…

广义相对论与量子宇宙学 · 物理学 2023-07-24 Long Huang , Xiao feng Yang , Xiang Liu

The presence of dark energy in the Universe is inferred directly and indirectly from a large body of observational evidence. The simplest and most theoretically appealing possibility is the vacuum energy density (cosmological constant).…

天体物理学 · 物理学 2008-11-26 J. S. Alcaniz

Dark energy is an elusive concept, which has been introduced two decades ago in order to make the acceleration of the universe a comprehensible phenomenon. However, the nature of this energy is far from being understood, both from a…

高能物理 - 唯象学 · 物理学 2023-07-04 Miguel Hoyuelos , Pablo Sisterna

It is shown that quantum vacuum fluctuations give rise to a curvature of space-time of the order appropriate to explain the observed accelerated expansion of the universe. The fact that the fluctuations produce curvature, even if the…

广义相对论与量子宇宙学 · 物理学 2011-03-21 Emilio Santos

It has been suggested that the Dark Energy Coincidence Problem could be interpreted as a possible link between the cosmological constant and a massive graviton. We show that by using that link and models for the graviton mass a dark energy…

广义相对论与量子宇宙学 · 物理学 2009-11-11 M. Tajmar
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