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相关论文: Tachyon as a Dark Energy Source

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A minus sign is inserted, for good reason, into the formula for the Energy-Momentum Tensor for tachyons. This leads to remarkable theoretical consequences and a plausible explanation for the phenomenon called Dark Energy in the cosmos.

综合物理 · 物理学 2017-07-10 Charles Schwartz

We study physics concerning the cosmological constant problem in the framework of effective field theory and suggest that a dominant part of dark energy can originate from gravitational corrections of vacuum energy, under the assumption…

高能物理 - 理论 · 物理学 2017-02-24 Yugo Abe , Masaatsu Horikoshi , Yoshiharu Kawamura

A consistent theory of free tachyons has shown how tachyon neutrinos can explain major cosmological phenomena, Dark Energy and Dark Matter. Now we investigate how tachyon neutrinos might interact with other particles: the weak interactions.…

综合物理 · 物理学 2023-07-26 Charles Schwartz

This paper deals with dark and phantom energy in the tachyon and sub-quantum models for dark energy. We obtain that the simplest condition for such a regime to occur in these scenarios is that the scalar field be Wick rotated to imaginary…

高能物理 - 理论 · 物理学 2007-05-23 Pedro F. Gonzalez-Diaz

Usually considered highly speculative, tachyons can be treated via straightforward Einsteinian dynamics. Kinetic theory and thermodynamics for a gas of ``dark'' tachyons are readily constructed. Such a gas exhibits density and pressure…

广义相对论与量子宇宙学 · 物理学 2022-06-15 James M. Starke , Ian H. Redmount

We study cosmological effects of homogeneous tachyon field as dark energy. We concentrate on two different scalar field potentials, the inverse square potential and the exponential potential. These models have a unique feature that the…

天体物理学 · 物理学 2008-11-26 H. K. Jassal

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

It is obtained that dark energy emerges from higher-derivative gravity with anon-linear terms proportional to $R^2$ and $R^3$ with $R$ being the Ricci scalar curvature. Interestingly, it is found that the universe begins with acceleration,…

天体物理学 · 物理学 2008-11-26 S. K. Srivastava

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…

We perform a full investigation on dynamics of a new dark energy model in which the four-derivative of a non-canonical scalar field (tachyon) is non-minimally coupled to the vector torsion. Our analysis is done in the framework of…

广义相对论与量子宇宙学 · 物理学 2015-06-23 Behnaz Fazlpour , Ali Banijamali

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

The consideration of dark energy's quanta, required also by thermodynamics, introduces its chemical potential into the cosmological equations. Isolating its main contribution, we obtain solutions with dark energy decaying to matter or…

天体物理学 · 物理学 2008-11-26 J. Besprosvany

Although the cosmic concordance cosmology is quite successful in fitting data, fine tuning and coincidence problems apparently weaken it. We review several possibilities to ease its problems, by considering various kinds of dynamical Dark…

天体物理学 · 物理学 2008-11-26 S. A. Bonometto , R. Mainini , L. P. L. Colombo

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

Most of the models leading to a current state of cosmic accelerated expansion fail to address the coincidence problem, i.e., that the dark energy density and the energy density of the matter fluid are of the same order precisely today. We…

天体物理学 · 物理学 2007-05-23 Diego Pavon , Luis P. Chimento , Alejandro S. Jakubi

We consider the prospects for dark matter/energy unification in k-essence type theories. General mappings are established between the k-essence scalar field, the hydrodynamic and braneworld descriptions. We develop an extension of the…

广义相对论与量子宇宙学 · 物理学 2009-08-11 Neven Bilic , Gary B. Tupper , Raoul D. Viollier

Any non-gravitational coupling between dark matter and dark energy modifies the cosmological dynamics. Interactions in the dark sector are considered to be relevant to address the coincidence problem. Moreover, in various models the…

宇宙学与河外天体物理 · 物理学 2015-06-04 W. Zimdahl

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…

天体物理学 · 物理学 2009-11-10 Pedro F. Gonzalez-Diaz

Motivated by recent work of one of us [1], we generalize this work to agegraphic tachyon models of dark energy with entropy correction terms arising from loop quantum gravity. We establish a connection between the entropy-corrected…

综合物理 · 物理学 2011-01-25 Mubasher Jamil , Ahmad Sheykhi

We investigate several varying-mass dark-matter particle models in the framework of phantom cosmology. We examine whether there exist late-time cosmological solutions, corresponding to an accelerating universe and possessing dark energy and…

广义相对论与量子宇宙学 · 物理学 2014-11-18 Genly Leon , Emmanuel N. Saridakis