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相关论文: More on Emergent Dark Energy from Unparticles

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{\it The universe is expanding} is known (through Galaxy observations) since 1929 through Hubble's discovery ($V = H D$). Recently in 1999, it is found (through Supernovae observations) that the universe is not simply expanding but is…

综合物理 · 物理学 2010-10-20 R. C. Gupta , Anirudh Pradhan

We are at a specific period of modern cosmology, during which the large increase of the amount of data leads to the idea that the determination of cosmological parameters has been achieved with a rather good precision. There is a large…

天体物理学 · 物理学 2017-08-23 A. Blanchard

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

Motivated by the apparent discrepancy between Cosmic Microwave Background measurements of the Hubble constant and measurements from Type-Ia supernovae, we construct a model for Dark Energy with equation of state $w = p / \rho < -1$,…

宇宙学与河外天体物理 · 物理学 2018-10-31 Gabriela Barenboim , William H. Kinney , Michael J. P. Morse

The recent astronomical measurements of distant supernovae as well as other observations indicate that our universe is presently accelerating. There are different proposals for the explanation of this acceleration, such as the cosmological…

天体物理学 · 物理学 2008-11-26 Marek Szydlowski , Wlodzimierz Godlowski

A new bound dark energy, BDE, cosmology has been proposed where the dark energy is the binding energy between light meson fields that condense a few tens of years after the big bang. It is reported that the correct dark energy density…

宇宙学与河外天体物理 · 物理学 2019-11-06 Rodger I. Thompson

If general relativity is the correct theory of physics on large scales, then there is a differential equation that relates the Hubble expansion function, inferred from measurements of angular diameter distance and luminosity distance, to…

天体物理学 · 物理学 2011-02-01 Mustapha Ishak , Amol Upadhye , David N. Spergel

In the late 1990's, observations of 93 Type Ia supernovae were analysed in the framework of the FLRW cosmology assuming these to be `standard(isable) candles'. It was thus inferred that the Hubble expansion rate is accelerating as if driven…

宇宙学与河外天体物理 · 物理学 2021-09-13 Roya Mohayaee , Mohamed Rameez , Subir Sarkar

Decaying Dark Energy models modify the background evolution of the most common observables, such as the Hubble function, the luminosity distance and the Cosmic Microwave Background temperature-redshift scaling relation. We use the most…

宇宙学与河外天体物理 · 物理学 2018-09-05 Ivan de Martino

The cause for the observed acceleration in the expansion of the universe is unknown, and referred to as "dark energy" for convenience. Dark energy could be an unknown energy component, or a modification of Einstein's general relativity.…

宇宙学与河外天体物理 · 物理学 2015-06-03 Yun Wang

Several models have been proposed to explain the dark energy that is causing universe expansion to accelerate. Here the acceleration predicted by the Holographic Dark Information Energy (HDIE) model is compared to the acceleration that…

宇宙学与河外天体物理 · 物理学 2015-06-04 Michael Paul Gough

No. It is simply not plausible that cosmic acceleration could arise within the context of general relativity from a back-reaction effect of inhomogeneities in our universe, without the presence of a cosmological constant or ``dark energy.''…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Akihiro Ishibashi , Robert M. Wald

We study a cosmological model featuring evolutionary dark energy, according to the idea that the creation of its constituents arises from the gravitational field of the expanding universe, whose non-equilibrium physics is described by a…

宇宙学与河外天体物理 · 物理学 2025-12-01 Iolanda Navone , Maria Giovanna Dainotti , Elisa Fazzari , Giovanni Montani , Naoto Maki , Kazunori Kohri

It is argued that cosmological models that feature a flow of energy from dark energy to dark matter may solve the coincidence problem of late acceleration (i.e., "why the energy densities of both components are of the same order precisely…

广义相对论与量子宇宙学 · 物理学 2009-02-06 Sergio del Campo , Ramon Herrera , Diego Pavon

Cosmology is living through fascinating times, where new observations from ground and space telescopes are questioning the established paradigm, the so-called Lambda Cold Dark Matter model. The particle nature of Dark Matter is severely…

宇宙学与河外天体物理 · 物理学 2026-04-15 Juan Garcia-Bellido

Based on dramatic observations of the CMB with WMAP and of Type Ia supernovae with the Hubble Space Telescope and ground-based facilities, it is now generally believed that the Universe's expansion is accelerating. Within the context of…

天体物理学 · 物理学 2007-11-30 Fulvio Melia

We propose that dark energy in the form of a scalar field could effectively couple to dark matter inhomogeneities. Through this coupling energy could be transferred to/from the scalar field, which could possibly enter an accelerated regime.…

宇宙学与河外天体物理 · 物理学 2016-04-25 Valerio Marra

The paper deals with a spatially homogeneous and anisotropic universe filled with perfect fluid and dark energy components. The two sources are assumed to interact minimally together with a special law of variation for the average Hubble's…

综合物理 · 物理学 2014-08-27 Suresh Kumar , Anil Kumar Yadav

In this article, we review a series of recent theoretical results regarding a conventional approach to the dark energy (DE) concept. This approach is distinguished among others for its simplicity and its physical relevance. By compromising…

宇宙学与河外天体物理 · 物理学 2016-04-20 Kostas Kleidis , Nikolaos K. Spyrou

By using an unmodified Einstein gravity theory it is shown that all of the speeding-up effects taking place in the current universe are entirely due to the quantum effects associated with the background radiation or to the combination of…

天体物理学 · 物理学 2009-11-11 Pedro F. Gonzalez-Diaz , Alberto Rozas-Fernandez