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相关论文: More on Emergent Dark Energy from Unparticles

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The Hubble tension and the unknown origin of dark energy motivate the exploration of alternative mechanisms for late-time cosmic acceleration. We investigate gravitationally induced particle creation (PC) as a non-equilibrium process that…

宇宙学与河外天体物理 · 物理学 2026-04-28 Tiziano Schiavone , Mariaveronica De Angelis , Luis A. Escamilla , Giovanni Montani , Eleonora Di Valentino

General relativistic entropic acceleration theory may explain the present cosmic acceleration from first principles without the need of introducing a cosmological constant. Following the covariant formulation of non-equilibrium phenomena in…

广义相对论与量子宇宙学 · 物理学 2021-10-20 Juan Garcia-Bellido , Llorenc Espinosa-Portales

In the last dozens of years different data sets revealed the accelerated expansion of the Universe which is driven by the so called dark energy, that now dominates the total amount of matter-energy in the Universe. In a recent paper Glavan,…

宇宙学与河外天体物理 · 物理学 2019-06-27 Marek Demianski , Ester Piedipalumbo

Constantly accumulating observational data continue to confirm that about 70% of the energy density today consists of dark energy responsible for the accelerated expansion of the Universe. We present recent observational bounds on dark…

宇宙学与河外天体物理 · 物理学 2013-11-12 Shinji Tsujikawa

The current observations are usually explained by an accelerating expansion of the present universe. However, with the present quality of the supernovae Ia data, the allowed parameter space is wide enough to accommodate the decelerating…

天体物理学 · 物理学 2009-11-07 R. G. Vishwakarma

In this paper we review a part of the approaches that have been considered to explain the extraordinary discovery of the late time acceleration of the Universe. We discuss the arguments that have led physicists and astronomers to accept…

宇宙学与河外天体物理 · 物理学 2010-12-13 Domenico Sapone

We present a model of the expanding Universe that begins in a zero energy vacuum state. The Universe results from the spontaneous breaking of the electroweak symmetry, wherein the vacuum with positive expectation energy produces the dark…

综合物理 · 物理学 2021-04-29 R. N. Henriksen

A large number of recent observational data strongly suggest that we live in a flat, accelerating Universe composed of $\sim$ 1/3 of matter (baryonic + dark) and $\sim$ 2/3 of an exotic component with large negative pressure, usually named…

天体物理学 · 物理学 2015-06-24 J. A. S. Lima

We propose a cosmological model that makes a significant step toward solving the coincidence problem of the near similarity at the present of the dark energy and dark matter components. Our cosmology has the following properties: a) among…

天体物理学 · 物理学 2008-11-26 Luca Amendola , Domenico Tocchini-Valentini

It has been proposed that the accelerated expansion of the universe can be explained by the merging of our universe with baby universes, resulting in dark energy with a phantom-like equation of state. However, the evidence in favor of it…

宇宙学与河外天体物理 · 物理学 2025-06-18 Varun Muralidharan , James M. Cline

In the present work we discuss a third alternative to explain the latest observational data concerning the accelerating Universe and its different stages. The particle creation mechanism in the framework of non-equilibrium thermodynamics is…

广义相对论与量子宇宙学 · 物理学 2016-05-17 Subenoy Chakraborty , Supriya Pan , Subhajit Saha

Explanations of the late-time cosmic acceleration within the framework of general relativity are plagued by difficulties. General relativistic models are mostly based on a dark energy field with fine-tuned, unnatural properties. There is a…

天体物理学 · 物理学 2010-04-22 Ruth Durrer , Roy Maartens

Observations conducted over the last few decades show that the expansion of the Universe is accelerating. In the standard model of cosmology, this accelerated expansion is attributed to a dark energy in the form of a cosmological constant.…

宇宙学与河外天体物理 · 物理学 2021-04-22 Joseph Ryan

Late-time cosmic acceleration is one of the most interesting unsolved puzzles in modern cosmology. The explanation most accepted nowadays, dark energy, raises questions about its own nature, e.g. what exactly is dark energy, and…

宇宙学与河外天体物理 · 物理学 2019-04-26 Williams J. M. Ribeiro

Recently, new arguments (astro-ph/0501152, hep-th/0503117) for how corrections from super-Hubble modes can explain the present-day acceleration of the universe have appeared in the literature. However, in this letter, we argue that, to…

天体物理学 · 物理学 2009-11-10 Ghazal Geshnizjani , Daniel J. H. Chung , Niayesh Afshordi

The traditional "explanation" for the observed acceleration of the universe is the existence of a positive cosmological constant. However, this can hardly be a truly convincing explanation, as an expanding universe is not expected to have a…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Joan Sola

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

We examine a dark energy model where a scalar unparticle degree of freedom plays the role of quintessence. In particular, we study a model where the unparticle degree of freedom has a standard kinetic term and a simple mass potential, the…

宇宙学与河外天体物理 · 物理学 2009-11-06 De-Chang Dai , Sourish Dutta , Dejan Stojkovic

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

Over the past decade, the disparity between the value of the cosmic expansion rate directly determined from measurements of distance and redshift or instead from the standard $\Lambda$CDM cosmological model calibrated by measurements from…

宇宙学与河外天体物理 · 物理学 2022-11-10 Marc Kamionkowski , Adam G. Riess