中文
相关论文

相关论文: Tachyon as a Dark Energy Source

200 篇论文

Here, non-minimally coupled tachyon to gravity is considered as a source of "dark energy". It is demonstrated that with expansion of the universe, tachyon dark energy decays to "dark matter" providing a solution to "cosmic coincidence…

广义相对论与量子宇宙学 · 物理学 2007-05-23 S. K. Srivastaca

A model for the universe on the basis of a self interacting fermionic tachyon field is investigated here. It is shown that, devising a self interaction potential of a proper form, the fermionic tachyon field is capable of producing an…

广义相对论与量子宇宙学 · 物理学 2023-03-29 Salomeh Khoeini-Moghaddam , Farzan Momeni , Fatemeh Yousefabadi

In the past few years, a possibility is investigated, where curvature itself behaves as a source of dark energy. So, it is natural to think whether curvature can produce dark matter too. It is found that, at classical level,…

高能物理 - 理论 · 物理学 2008-01-14 S. K. Srivastava , K. P. Sinha

The fact that the energy densities of dark energy and matter are similar currently, known as the coincidence problem, is one of the main unsolved problems of cosmology. We present here a model in which a spatial curvature of the universe…

天体物理学 · 物理学 2009-11-13 Urbano Franca

Recent attempts to explain the dark matter and energy content of the universe have involved some radical extensions of standard physics, including quintessence, phantom energy, additional space dimensions and variations in the speed of…

天体物理学 · 物理学 2009-11-10 P. C. W. Davies

In a recent paper we showed that a quintessence scalar field plus a dissipative matter fluid can drive late cosmic accelerated expansion and simultaneously solve the coincidence problem [1]. In this brief report we extend this result to the…

天体物理学 · 物理学 2009-11-07 Luis P. Chimento , Alejandro S. Jakubi , Diego Pavon

We present and study a conformally coupled dark energy model, characterised by an interaction between a tachyon field $\phi$, with an inverse square potential $V (\phi)$, and the matter sector. A detailed analysis of the cosmological…

广义相对论与量子宇宙学 · 物理学 2019-09-06 Elsa M. Teixeira , Ana Nunes , Nelson J. Nunes

We study the coincidence problem of late cosmic acceleration by assuming that the present ratio between dark matter and dark energy is a slowly varying function of the scale factor. As dark energy component we consider two different…

天体物理学 · 物理学 2009-11-13 Sergio del campo , Ramon Herrera , Diego Pavon

A tachyon field having a negative squared-mass $-m_t^2$ can be described in terms of massless fields degenerating infinitely with respect to helicities. This picture for tachyons does not contradict causality. It is seen that the tachyon…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Tsunehiro Kobayashi

The so called `cosmic coincidence' problem seems to suggest a coupling between dark energy and dark matter. A possibility could be given by dark matter particles with masses depending exponentially on the scalar field associated to dark…

高能物理 - 唯象学 · 物理学 2007-05-23 Massimo Pietroni

Recently it has been argued that a possible source for the dark energy may arise due to the contribution to the vacuum energy of the QCD ghost in a time-dependent background. In this paper we establish a connection between interacting ghost…

高能物理 - 理论 · 物理学 2012-04-10 A. Sheykhi , M. Sadegh Movahed , E. Ebrahimi

I discuss the possibility that dark energy is a scalar field whose quanta are extremely light and very weakly interacting superluminal particles, i.e. tachyons, with purely imaginary mass $m = i\Gamma$ with $\Gamma$ real.

综合物理 · 物理学 2018-11-09 Michael Albrow

Astrophysical observations are pointing out huge amounts of dark matter and dark energy needed to explain the observed large scale structures and cosmic accelerating expansion. Up to now, no experimental evidence has been found, at…

天体物理学 · 物理学 2009-11-11 S. Capozziello , V. F. Cardone , A. Troisi

A curvature self-interaction of the cosmic gas is shown to mimic a cosmological constant or other forms of dark energy, such as a rolling tachyon condensate or a Chaplygin gas. Any given Hubble rate and deceleration parameter can be traced…

天体物理学 · 物理学 2016-08-30 Alexander B. Balakin , Diego Pavon , Dominik J. Schwarz , Winfried Zimdahl

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…

高能物理 - 唯象学 · 物理学 2023-07-04 Miguel Hoyuelos , Pablo Sisterna

A late accelerated expansion of the Universe is obtained from non-relativistic particles with a short-range attractive interaction, and low enough temperature to produce a Bose-Einstein condensate; by considering coupled dark-energy…

宇宙学与河外天体物理 · 物理学 2016-05-13 Jaime Besprosvany , German Izquierdo

The introduction of an interaction for dark energy to the standard cosmology offers a potential solution to the cosmic coincidence problem. We examine the conditions on the dark energy density that must be satisfied for this scenario to be…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Micheal S. Berger , Hamed Shojaei

The string inspired tachyon field can serve as a candidate of dark energy. Its equation of state parameter $w$ varies from 0 to -1. In case of tachyon field potential $V(\phi)\to 0$ slower(faster) than $1/\phi^2$ at infinity, dark…

宇宙学与河外天体物理 · 物理学 2009-06-30 Amna Ali , M. Sami , A. A. Sen

Dark energy and dark matter are the dominant sources in the evolution of the late universe. They are currently only indirectly detected via their gravitational effects, and there could be a coupling between them without violating…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Christian G. Boehmer , Gabriela Caldera-Cabral , Ruth Lazkoz , Roy Maartens

A physical mechanism that produces three energy components is proposed as the common origin of dark energy and dark matter. The first two have equations of state W ~ 0 and act like dark matter, while the last has W ~ -1 at low redshifts…

广义相对论与量子宇宙学 · 物理学 2012-12-12 I. Gontijo
‹ 上一页 1 2 3 10 下一页 ›