中文
相关论文

相关论文: Dark Matter as Dark Energy

200 篇论文

In recent work we have extended the theory that dark matter is composed of primordial black hole (PBHs) to extremely high masses and made an assumption that the holographic entropy bound is saturated. Astrophysicists have recently suggested…

综合物理 · 物理学 2022-10-26 Paul H. Frampton

Following the idea of the induced matter theory, for a non-vacuum five-dimensional version of general relativity, we propose a model in which the induced terms emerging from the extra dimension in our four-dimensional space-time, supposed…

广义相对论与量子宇宙学 · 物理学 2018-07-27 Amir F. Bahrehbakhsh

Recent astronomical observations of distant supernovae light-curves suggest that the expansion of the universe has recently begun to accelerate. Acceleration is created by an anti-gravitational repulsive stress, like that produced by a…

天体物理学 · 物理学 2009-10-31 John Barrow , Rachel Bean , Joao Magueijo

The data indicating existence of different forms of dark matter in the universe as well as the role of this matter in structure formation are briefly reviewed. It is argued that vacuum energy gives a dominant contribution into the total…

天体物理学 · 物理学 2007-05-23 A. D. Dolgov

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

Theoretical results on a conventional approach to the dark energy (DE) concept are reviewed and discussed. According to them, there is absolutely no need for a novel DE component in the Universe, provided that the associated matter-energy…

广义相对论与量子宇宙学 · 物理学 2023-06-19 Kostas Kleidis , Nikolaos K. Spyrou

Vacuum energy is a simple model for dark energy driving an accelerated expansion of the universe. If the vacuum energy is inhomogeneous in spacetime then it must be interacting. We present the general equations for a spacetime-dependent…

宇宙学与河外天体物理 · 物理学 2014-07-01 Josue De-Santiago , David Wands , Yuting Wang

In the present work, an alternative interpretation of the source of accelerated expansion of the Universe is suggested. A probable candidate is the interaction between the quantum spin of a moving particle and the torsion of space-time,…

广义相对论与量子宇宙学 · 物理学 2016-11-15 M. I. Wanas

The nonbaryonic dark matter of the Universe is assumed to consist of new stable particles. A specific case is possible, when new stable particles bear ordinary electric charge and bind in heavy "atoms" by ordinary Coulomb interaction. Such…

宇宙学与河外天体物理 · 物理学 2015-03-17 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

We consider a supersymmetric model of dark energy coupled to cold dark matter: the supersymmetron. In the absence of cold dark matter, the supersymmetron converges to a supersymmetric minimum with a vanishing cosmological constant. When…

高能物理 - 唯象学 · 物理学 2015-05-30 Philippe Brax , Anne-Christine Davis

The expansion of the universe has been accepted by scientists for more than a century. However, since the 1990s, observations have suggested that the universe is expanding at an accelerating rate. Although the source of this acceleration is…

泛函分析 · 数学 2017-11-13 Issa Mohamadi

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

Observations seem to indicate that our universe is presently accelerating due to the presence of dark energy. Quintessence represents a possible way to model the dark energy. In these proceedings, we briefly review its main properties.

天体物理学 · 物理学 2007-05-23 Philippe Brax , Jerome Martin

We show that an interaction between dark matter and dark energy generically results in an effective dark energy equation of state of w<-1. This arises because the interaction alters the redshift-dependence of the matter density. An observer…

天体物理学 · 物理学 2010-03-26 Subinoy Das , Pier Stefano Corasaniti , Justin Khoury

Recent observational evidences of accelerating phase of the universe strongly demand that the dominating matter in the universe is in the form of dark energy. In this work, we study the evolution of the apparent and event horizons for…

广义相对论与量子宇宙学 · 物理学 2015-05-28 Ritabrata Biswas , Nairwita Mazumder , Subenoy Chakraborty

A dual component made of non-relativistic particles and a scalar field, exchanging energy, naturally falls onto an attractor solution, making them a (sub)dominant part of the cosmic energy during the radiation dominated era, provided that…

宇宙学与河外天体物理 · 物理学 2012-08-15 Silvio A. Bonometto , Giandomenico Sassi , Giuseppe La Vacca

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

Based on the results from numerous astrophysics experiments, it is currently believed that the majority of matter in the Universe is in some unknown form, known as dark matter. In the past it has been common to model dark matter as a…

高能物理 - 唯象学 · 物理学 2008-12-25 Chris Bird

The universe has evolved to be a filamentary web of galaxies and large inter-galactic zones of space without matter. The Euclidian nature of the universe indicates that it is not a 3D manifold within space with an extra spatial dimension.…

宇宙学与河外天体物理 · 物理学 2010-03-29 Shlomo Barak , Elia M. Leibowitz

It is shown that the vacuum condensate induced by many phenomena behaves as a perfect fluid which, under particular conditions, has zero or negative pressure. In particular, the condensates of thermal states, of fields in curved space and…

高能物理 - 理论 · 物理学 2016-10-28 Antonio Capolupo