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相关论文: Tachyons, Scalar Fields and Cosmology

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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

We study the dynamics of the scalar tensor cosmological model in the presence of tachyon field. In an alternative approach, in two exponential and power law form of the scalar field functions in the model, field equations are solved by…

广义相对论与量子宇宙学 · 物理学 2011-11-22 H. Farajollahi , A. Salehi , A. Shahabi

The cosmological effects of the tachyon rolling down to its ground state are discussed by coupling a simple effective field theory for the tachyon field to Einstein gravity. As the tachyon rolls down to the minimum of its potential the…

高能物理 - 理论 · 物理学 2009-10-07 G. W. Gibbons

We apply a very simple procedure to construct non-singular cosmological models for flat Friedmann universes filled with minimally coupled scalar fields or by tachyon Born-Infeld-type fields. Remarkably, for the minimally coupled scalar…

广义相对论与量子宇宙学 · 物理学 2024-03-14 Alexander Kamenshchik , Polina Petriakova

We study the general properties of attractors in a cosmological model with tachyonic potential and a scalar field non-minimally coupled to matter. A general analytic formulation is given to derive fixed points with a discussion on their…

广义相对论与量子宇宙学 · 物理学 2011-07-08 H. Farajollahi , A. Salehi

We study inflation, perturbations, non-gaussinity and late-time cosmological dynamics of a tachyon field both minimally and non-minimally coupled to gravity. By analyzing the parameters space of the model, the viability of the model in…

广义相对论与量子宇宙学 · 物理学 2015-06-16 Kourosh Nozari , Narges Rshidi

In this paper we investigate a tachyon field model in cosmology, provided its interaction with the quintessence or phantom fields.The model takes into account this interaction beyond the usual approach, in which the interaction is…

广义相对论与量子宇宙学 · 物理学 2012-05-25 V. K. Shchigolev , M. P. Rotova

It is often the case that scalar fields are produced in the early Universe in the form of coherent oscillation. These scalar fields may have huge abundances and affect the evolution of the Universe. In particular, if the lifetime is long…

高能物理 - 唯象学 · 物理学 2013-02-20 Masahiro Kawasaki , Naoya Kitajima , Kazunori Nakayama

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

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 develop a technique for the reconstruction of the potential for a scalar field or a tachyon field, reproducing a given cosmological evolution in a closed and open isotropic cosmological models. Such potentials are explicitly written down…

广义相对论与量子宇宙学 · 物理学 2015-06-03 Alexander Y. Kamenshchik , Serena Manti

The bouncing cosmology provides a successful solution of the cosmological singularity problem. In this paper, we study the bouncing behavior of a single scalar field model with tachyon field non-minimally coupled to itself, its derivative…

广义相对论与量子宇宙学 · 物理学 2015-06-03 A. Banijamali , B. Fazlpour

In this work we investigate the duality linking standard and tachyon scalar field cosmologies. We determine the transformation between standard and tachyon scalar fields and between their associated potentials, corresponding to the same…

宇宙学与河外天体物理 · 物理学 2010-11-11 P. P. Avelino , D. Bazeia , L. Losano , J. C. R. E. Oliveira , A. B. Pavan

We study a tachyon model with non-minimal derivative coupling to gravity in the Friedmann-Robertson-Walker flat cosmology. We propose the special re-definition of the tachyon field which allows us to represent tachyon field equation…

广义相对论与量子宇宙学 · 物理学 2012-09-13 V. K. Shchigolev , M. P. Rotova

We show how the scalar field, a candidate of quintessence, in a proposed model of the scalar-tensor theories of gravity provides a way to understand a small but nonzero cosmological constant as indicated by recent observations. A particular…

广义相对论与量子宇宙学 · 物理学 2009-09-25 Yasunori Fujii

The solution to the current extending Universe problem, and the description of all stages of evolution compels scientists to consider various cosmological models. Scalar - tensor models are rather simple and also allow us to clearly define…

广义相对论与量子宇宙学 · 物理学 2015-06-23 K. E. Osetrin , A. N. Makarenko , Yu. A. Rybalov

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 study dynamics of generalized tachyon scalar field in the framework of teleparallel gravity. This model is an extension of tachyonic teleparallel dark energy model which has been proposed in [26]. In contrast with tachyonic teleparallel…

广义相对论与量子宇宙学 · 物理学 2014-08-04 Behnaz Fazlpour , Ali Banijamali

Scalar fields in the early Universe are mostly discussed in two limits: either in equilibrium or completely decoupled. In this work we discuss scenarios where there are scalar fields that are not in equilibrium, but for which the coupling…

高能物理 - 唯象学 · 物理学 2025-07-30 V. Knapp-Perez , Gopolang Mohlabeng , Michael Ratz , Tim M. P. Tait

We compare the existing observational data on type Ia Supernovae with the evolutions of the universe predicted by a one-parameter family of tachyon models which we have introduced recently in paper \cite{we-tach}. Among the set of the…

广义相对论与量子宇宙学 · 物理学 2009-04-22 Z. Keresztes , L. Á. Gergely , V. Gorini , U. Moschella , A. Yu. Kamenshchik
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