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相关论文: Cosmology with decaying tachyon matter

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We present a detailed study of cosmological effects of homogeneous tachyon matter coexisting with non-relativistic matter and radiation, concentrating on the inverse square potential and the exponential potential for the tachyonic scalar…

天体物理学 · 物理学 2011-05-05 J. S. Bagla , H. K. Jassal , T. Padmanabhan

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

This paper presents an investigation of cosmological dynamics of tachyon fluid coupled to varyingmass dark matter particles in the background of spatially flat FLRW universe. The mechanism of varying mass particles scenario assumes the mass…

广义相对论与量子宇宙学 · 物理学 2025-07-22 Goutam Mandal , Sudip Mishra , Abdulla Al Mamon , Sujay Kr. Biswas

In this work a tachyonization of the $\Lambda$CDM model for a spatially flat Friedmann-Robertson-Walker space-time is proposed. A tachyon field and a cosmological constant are considered as the sources of the gravitational field. Starting…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Luis P. Chimento , Mónica Forte , Gilberto M. Kremer , Marlos O. Ribas

We propose a holographic tachyon model of dark energy with interaction between the components of the dark sector. The correspondence between the tachyon field and the holographic dark energy densities allows the reconstruction of the…

广义相对论与量子宇宙学 · 物理学 2010-11-25 Alberto Rozas-Fernández , David Brizuela , Norman Cruz

In this paper, we study the phase space analysis of locally rotationally symmetric Bianchi type I universe model by taking interactions between dark matter and scalar field models. We define normalized dimensionless variables to develop an…

广义相对论与量子宇宙学 · 物理学 2019-08-07 M. Sharif , Saadia Mumtaz

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

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

In this work we study the cosmological evolution of a dark energy model with two scalar fields, i.e. the tachyon and the phantom tachyon. This model enables the equation of state $w$ to change from $w>-1$ to $w<-1$ in the evolution of the…

天体物理学 · 物理学 2009-12-04 Shang-Gang Shi , Yun-Song Piao , Cong-Feng Qiao

The possibility of explanation of accelerated expansion of the Universe by tachyonic scalar fields which homogeneously fill the world is discussed. The dependences of potential and kinetic term on scale factor are deduced for the case of…

宇宙学与河外天体物理 · 物理学 2014-01-14 Bohdan Novosyadlyj

In this work we present a model of dark matter based on scalar-tensor theory of gravity. With this scalar field dark matter model we study the non-linear evolution of the large scale structures in the universe. The equations that govern the…

宇宙学与河外天体物理 · 物理学 2015-06-03 Mario A. Rodriguez-Meza

We discuss the coupling between dark energy and matter by considering a homogeneous tachyonic scalar field as a candidate for dark energy. We obtained the functional form of scale factor by assuming that the coupling strength depends…

广义相对论与量子宇宙学 · 物理学 2021-01-27 A Kundu , S D Pathak , V K Ojha

The existence of dark energy is essential to explain the cosmic accelerated expansion. We consider a homogenous interacting tachyonic scalar field as a possible candidate for the dynamical dark energy. The interaction between the tachyonic…

广义相对论与量子宇宙学 · 物理学 2023-05-02 V K Ojha , Adithya A Rao , S D Pathak

A tachyon field having a negative squared-mass $-m_t^2$ can be described in terms of massless fields degenerating infinitely with respect to the helicity. The degeneracy leads symmetry breakings of space-time. This picture for the tachyon…

广义相对论与量子宇宙学 · 物理学 2010-02-01 Tsunehiro Kobayashi

Recently, the tachyon cosmology has been represented as dark energy model to support the current acceleration of the universe without phantom crossing. In this paper, we study the dynamics of the tachyon cosmology in which the field plays…

广义相对论与量子宇宙学 · 物理学 2015-05-27 H. Farajollahi , A. Ravanpak , G. F. Fadakar

We investigate the cosmological dynamics of a homogeneous scalar field non-minimally coupled to torsion gravity, which also interacts with cold dark matter through energy and momentum transfer. The matter and radiation perfect fluids are…

广义相对论与量子宇宙学 · 物理学 2025-02-05 Carlos Rodriguez-Benites , Manuel Gonzalez-Espinoza , Giovanni Otalora , Manuel Alva-Morales

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

We study the cosmological evolution of a tachyon scalar field T with a Dirac- Born- Infeld type lagrangian and potential V (T) coupled to a canonically normalized scalar field with an arbitrary but factorizeable interaction potential B…

高能物理 - 唯象学 · 物理学 2010-11-11 U. Filobello , A. de la Macorra

We present a detailed analysis of the phase-space for the field equations in scalar field cosmology with a chameleon cosmology in a spatially flat Friedmann--Lema\^{\i}tre--Robertson--Walker spacetime. For the matter source we assume that…

广义相对论与量子宇宙学 · 物理学 2023-06-07 Andronikos Paliathanasis

A Friedmann-Robertson-Walker cosmological model dominated by tachyonic -- faster-than-light -- dark matter can exhibit features similar to those of a standard dark energy/dark matter or $Lambda$CDM model. It can undergo expansion which…

广义相对论与量子宇宙学 · 物理学 2022-08-19 Audrey Claire Martin , Ian H. Redmount
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