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The phenomenon of dark energy and its manifestations are studied in a spherically symmetric universe considering the Brans-Dicke scalar tensor theory. In the first model the dark energy behaves like a phantom type and in such a universe the…

General Relativity and Quantum Cosmology · Physics 2019-03-29 Koijam Manihar Singh , Gauranga C. Samanta

The physical process leading to the acceleration of the expansion of the universe is unknown. It may involve new high energy physics or extensions to gravitation. Calling this generically dark energy, we examine the consistencies and…

Astrophysics · Physics 2009-11-10 Eric V. Linder

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…

Functional Analysis · Mathematics 2017-11-13 Issa Mohamadi

A class of dynamical dark energy models is constructed through an extended version of fermion fields corresponding to phantom dark ghost spinors, which are spin one half with mass dimension one. We find that if these spinors interact with…

General Relativity and Quantum Cosmology · Physics 2017-05-09 Yu-Chiao Chang , Mariam Bouhmadi-López , Pisin Chen

We discuss the possibility that the existence of dark energy may be due to the presence of a spin zero field $\phi(x)$, either elementary or composite. In the presence of other matter field, the transformation $\phi(x)\to \phi(x) +$…

Astrophysics · Physics 2009-11-10 T. D. Lee

The hypothesis is rapidly gaining popularity that the dark energy pervading our universe is extra-repulsive ($-p>\rho$). The density of such a substance(usually called phantom energy) grows with the cosmological expansion and may become…

Astrophysics · Physics 2010-02-01 Anton Baushev

A class of dynamical dark energy models, dubbed Spinor Quintom, can be constructed by a spinor field $\psi$ with a nontraditional potential. We find that, if choosing suitable potential, this model is able to allow the equation-of-state to…

High Energy Physics - Theory · Physics 2008-11-26 Yi-Fu Cai , Jing Wang

There is compelling evidence that the Universe is undergoing a late phase of accelerated expansion. One of the simplest explanations for this behaviour is the presence of dark energy. A plethora of microphysical models for dark energy have…

Cosmology and Nongalactic Astrophysics · Physics 2024-10-25 William J. Wolf , Pedro G. Ferreira

A dark energy component is responsible for the present stage of acceleration of our universe. If no fine tuning is assumed on the dark energy potential then it will end up dominating the universe at late times and the universe will not stop…

Astrophysics · Physics 2008-11-26 A. de la Macorra

The cosmic acceleration is one of the most significant cosmological discoveries over the last century. Following the more accurate data a more dramatic result appears: the recent analysis of the observation data (especially from SNe Ia)…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-17 Hongsheng Zhang

Phantom energy which violates the dominant-energy condition and is not excluded by current constraints on the equation of state may be dominating the evolution of the universe now. It has been pointed out that in such a case the fate of the…

Astrophysics · Physics 2009-11-07 Pedro F. Gonzalez-Diaz

If dark energy is a form of quintessence driven by a scalar field $\phi$ evolving down a monotonically decreasing potential $V(\phi)$ that passes sufficiently below zero, the universe is destined to undergo a series of smooth transitions.…

Cosmology and Nongalactic Astrophysics · Physics 2022-05-05 Cosmin Andrei , Anna Ijjas , Paul J. Steinhardt

We consider the oscillating dark energy with periodic equation of state in two equivalent formulations: ideal fluid or scalar-tensor theory. It is shown that such dark energy suggests the natural way for the unification of early-time…

High Energy Physics - Theory · Physics 2009-09-17 Shin'ichi Nojiri , Sergei D. Odintsov

We present cosmic solutions corresponding to universes filled with dark and phantom energy, all having a negative cosmological constant. All such solutions contain infinite singularities, successively and equally distributed along time,…

General Relativity and Quantum Cosmology · Physics 2010-11-02 Salvador Robles-Perez , Prado Martin-Moruno , Alberto Rozas-Fernandez , Pedro F. Gonzalez-Diaz

This paper deals with a cosmological model in which the universe is filled with tachyon dark energy in order to describe current and future accelerating expansion. We obtain that the simplest condition for the regime of phantom energy to…

Astrophysics · Physics 2009-11-10 Pedro F. Gonzalez-Diaz

This paper is devoted to some simple approach based on general physics tools to describe the physical properties of a hypothetical particle which can be the source of dark energy in the Universe known as phantom. Phantom is characterized by…

General Relativity and Quantum Cosmology · Physics 2015-09-15 Mariusz P. Dabrowski

Dark energy appears to be the dominant component of the physical Universe, yet there is no persuasive theoretical explanation for its existence or magnitude. The acceleration of the Universe is, along with dark matter, the observed…

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…

High Energy Physics - Phenomenology · Physics 2023-07-04 Miguel Hoyuelos , Pablo Sisterna

Dark energy with the usually used equation of state $p=w\rho$, where $w=const<0$ is hydrodynamically unstable. To overcome this drawback we consider the cosmology of a perfect fluid with a linear equation of state of a more general form…

Astrophysics · Physics 2009-11-06 E. Babichev , V. Dokuchaev , Yu. Eroshenko

To explain the acceleration of the cosmological expansion researchers have considered an unusual form of mass-energy generically called dark energy. Dark energy has a ratio of pressure over mass density which obeys $w=p/\rho <-1/3$. This…

High Energy Physics - Theory · Physics 2008-12-19 Max Chaves , Douglas Singleton
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