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相关论文: Tachyon field inspired dark energy and supernovae …

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The background evolution of an accelerated, dark energy dominated universe is aptly described by non-canonical tachyon scalar field models. The accelerated expansion of the universe is determined by the choice of a suitable scalar field…

广义相对论与量子宇宙学 · 物理学 2019-05-10 Avinash Singh , Archana Sangwan , H. K. Jassal

In this work we determine the correspondence between quintessence and tachyon dark energy models with a constant dark energy equation of state parameter, $w_e$. Although the evolution of both the Hubble parameter and the scalar field…

宇宙学与河外天体物理 · 物理学 2015-05-27 P. P. Avelino , L. Losano , J. J. Rodrigues

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

Rolling tachyon field models are among the candidates suggested as explanations for the recent acceleration of the Universe. In these models the field is expected to interact with gauge fields and lead to variations of the fine-structure…

宇宙学与河外天体物理 · 物理学 2016-06-28 C. J. A. P. Martins , F. M. O. Moucherek

There are many different phenomenological models describing the cosmological dark energy and accelerating Universe by choosing adjustable functions. In this paper we consider a specific model of scalar tachyon field which is derived from…

天体物理学 · 物理学 2007-05-23 I. Ya. Aref'eva

Scalar fields aptly describe equation of state of dark energy. The scalar field models were initially proposed to circumvent the fine tuning problem of cosmological constant. However, the model parameters also need a fine tuning of their…

宇宙学与河外天体物理 · 物理学 2018-06-19 Archana Sangwan , Ashutosh Tripathi , H. K. Jassal

In the present work we study a dark energy model in which a non-linear scalar field (tachyon) with a Born-Infeld type of action is responsible for the observed cosmic acceleration. The potential of the tachyon is well-motivated since it…

天体物理学 · 物理学 2007-05-23 G. Panotopoulos

The current paper provides a comprehensive examination of a dark energy cosmological model in the classical regime, in which a generic scalar field is regarded as a dark energy source. Einstein's field equations are solved in model…

广义相对论与量子宇宙学 · 物理学 2022-09-07 Ritika Nagpal , Shibesh Kumar Jas Pacif , Abhishek Parida

Recent progress in theoretical physics suggests that the dark energy in the universe might be resulted from the rolling tachyon field of string theory. Measurements to SNe Ia can be helpful to reconstruct the equation of state of the…

高能物理 - 理论 · 物理学 2009-11-07 Jian-gang Hao , Xin-zhou Li

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

We investigate the case of a homogeneous tachyon field coupled to gravity in a spatially flat Friedman-Robertson-Walker spacetime. Assuming the field evolution to be exponentially decaying with time we solve the field equations and show…

天体物理学 · 物理学 2009-11-11 A. Das , Shashikant Gupta , Tarun Deep Saini , Sayan Kar

Recent observations from the DESI survey have reignited the debate on the true nature of dark energy, challenging the standard model of cosmology. The results suggest a preference for dynamical dark energy rather than a constant. Several…

宇宙学与河外天体物理 · 物理学 2026-04-28 Ramanpreet Singh , Athul CN , H. K. Jassal

In this work we investigate a cosmological model with the tachyon and fermion fields with barotropic equation of state, where pressure $p$, energy density $\rho$ and barotropic index $\gamma$ are related by the relation $p=(\gamma-1)\rho$.…

广义相对论与量子宇宙学 · 物理学 2021-11-10 P. Tsyba , O. Razina , N. Suikimbayeva

We assume that universe is dominated by non-relativistic matter and tachyon field and reconstruct the potential of tachyon field directly from the effective equation of state (EOS) of dark energy. We apply the method to four known…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Ying Shao , Yuanxing Gui

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

The explanation of the accelerated expansion of the Universe poses one of the most fundamental questions in physics and cosmology today. If the acceleration is driven by some form of dark energy, one can try to constrain the parameters…

宇宙学与河外天体物理 · 物理学 2015-06-05 Marek Demianski , Ester Piedipalumbo , Claudio Rubano , Paolo Scudellaro

This paper reports improvements and new results for a well developed theory of tachyons (faster-than-light particles) and follows the suggestion that neutrinos - especially the low energy neutrinos in the Cosmic Neutrino Background - may be…

综合物理 · 物理学 2025-06-23 Charles Schwartz

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

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

In this work we present a new scheme to study the tachyon dark energy model using dynamical systems analysis by considering parametrization of the equation of state(EoS) of the dark energy. Both the canonical and phantom field dynamics are…

广义相对论与量子宇宙学 · 物理学 2023-03-21 Saddam Hussain , Saikat Chakraborty , Nandan Roy , Kaushik Bhattacharya
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