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相关论文: The solution of tachyon inflation in curved univer…

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In this letter, we have assumed that the Universe is filled in tachyonic field with potential, which gives the acceleration of the Universe. For certain choice of potential, we have found the exact solutions of the field equations. We have…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Surajit Chattopadhyay , Ujjal Debnath , Goutami Chattopadhyay

We present a cosmological landscape where the classical closed string tachyon field plays an important role in the framework of a critical bosonic compactification. Our cosmological solutions for a universe with constant curvature describes…

广义相对论与量子宇宙学 · 物理学 2013-01-22 Celia Escamilla-Rivera

We study the possibility to construct an observationally viable scenario where both early Inflation and the recently detected accelerated expansion of the universe can be explained by using a single scalar field associated with the Tachyon.…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Victor H. Cardenas

In this article we study closed inflationary universe models by using a tachyonic field theory. We determine and characterize the existence of an universe with $\Omega > 1$, and which describes a period of inflation. We find that considered…

天体物理学 · 物理学 2008-11-26 Leonardo Balart , Sergio del Campo , Ramon Herrera , Pedro Labrana

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

Loop quantum cosmology (LQC) predicts a nonsingular evolution of the universe through a bounce in the high energy region. We show that this is always true in tachyon matter LQC. Different from the classical Friedman-Robertson-Walker (FRW)…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Hua-Hui Xiong , Jian-Yang Zhu

We study a k-essence field evolving linearly with the cosmic time and the atypical k-essence model on a homogeneous and isotropic flat 3-brane. We show that the k-field is driven by an inverse quadratic polynomial potential. The solutions…

宇宙学与河外天体物理 · 物理学 2010-08-24 Luis P. Chimento , Martín G. Richarte

The dynamics of a tachyon field plus a barotropic fluid is investigated in spatially curved FRW universe. We perform a phase-plane analysis and obtain scaling solutions accompanying with a discussion on their stability. Furthermore, we…

高能物理 - 理论 · 物理学 2010-03-17 Jian-Li Li , Jian-Pin Wu

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

An inflationary universe scenario in the context of tachyon field is studied. This study is done from an ansantz for the effective potential of cosmological perturbations $U(\eta)$. We describe in great detail the analytical solutions of…

广义相对论与量子宇宙学 · 物理学 2016-03-23 Ramon Herrera , Roberto G. Perez

The model of inflation with a single tachyon field generates larger anisotropy and has difficulties in describing the formation of the Universe . In this paper we consider a model with multi tachyon fields and study the assisted…

高能物理 - 唯象学 · 物理学 2009-11-07 Yun-Song Piao , Rong-Gen Cai , Xinmin Zhang , Yuan-Zhong Zhang

In the present work an inflationary tachyon field model of the early universe is considered. Several cosmological effects produced by a particular potential in this tachyonic era are studied, under the approximation of slow-roll inflation.…

广义相对论与量子宇宙学 · 物理学 2015-11-09 Iván E. Sánchez G. , Osvaldo P. Santillan

Cosmological solution to the gravitational field equations in the generalized Randall-Sundrum model for an anisotropic brane with Bianchi I geometry and perfect fluid as matter sources has been considered. The matter on the brane is…

广义相对论与量子宇宙学 · 物理学 2019-12-16 Rikpratik Sengupta , Prasenjit Paul , Bikash Chandra Paul , Saibal Ray

We prove that in the Hartle-Hawking approach to quantum cosmology the existence of an inflationary phase is a general property of minisuperspace models given by a closed Friedmann-Robertson-Walker universe containing a massless scalar field…

广义相对论与量子宇宙学 · 物理学 2010-04-06 Giampiero Esposito , Giovanni Platania

Recently tachyonic field has been depicted as dark energy model to represent the present acceleration of the Universe. In this paper we have considered mixture of tachyonic fluid with a perfect fluid. For this purpose we have considered…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Writambhara Chakraborty , Ujjal Debnath

The emergent model in the context of loop quantum cosmology with a tachyon scalar field is studied. We find that there is a center equilibrium point in the semiclassical region and a saddle point in the classical region. If the potential of…

宇宙学与河外天体物理 · 物理学 2010-05-28 Puxun Wu , Shuang Nan Zhang , Hongwei Yu

We consider issues related to tachyonic inflation with exponential potential. We find exact solution of evolution equations in the slow roll limit in FRW cosmology. We also carry out similar analysis in case of Brane assisted tachyonic…

高能物理 - 理论 · 物理学 2009-11-07 M. Sami , Pravabati Chingangbam , Tabish Qureshi

In this work, I have considered that the universe is filled with normal matter and phantom field (or tachyonic field). If the universe is filled with scalar field, Ellis et al have shown that emergent scenario is possible only for $k=+1$…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Ujjal Debnath

The curvaton reheating in a tachyonic inflationary universe model with an exponential potential is studied. We have found that the energy density in the kinetic epoch, has a complicated dependencies of the scale factor. For different…

广义相对论与量子宇宙学 · 物理学 2009-11-11 C. Campuzano , S. del Campo , R. Herrera

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
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