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相关论文: Cosmological model with fermion and tachyon fields…

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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

In this work we study the dynamical generation of a fermion mass induced by a constant and uniform external magnetic field in an Abelian gauge model with a Yukawa term. We show that the Yukawa coupling not only enhances the dynamical…

高能物理 - 理论 · 物理学 2009-10-31 Efrain J. Ferrer , Vivian de la Incera

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

Recent results from the Dark Energy Spectroscopic Instrument (DESI) provide evidence for a dynamical dark-energy component, whose equation of state appears to have recently crossed the phantom divide. In this Letter, we present an…

宇宙学与河外天体物理 · 物理学 2026-05-20 E. Abdalla , O. P. F. Piedra , A. A. Escobal , A. M. Vicente , F. B. Abdalla , B. Wang , A. Marins

This paper consider an universe dominated by baryonic matter, radiation and a nonminimally coupled massive scalar field under the action of a symmetry breaking potential. Inflation occurs naturally with appropriated slow-roll values. The…

宇宙学与河外天体物理 · 物理学 2021-11-02 S. H. Pereira

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

In this work we extend the first order formalism for cosmological models that present an interaction between a fermionic and a scalar field. Cosmological exact solutions describing universes filled with interacting dark energy and dark…

广义相对论与量子宇宙学 · 物理学 2012-11-22 A. B. Pavan , Elisa G. M. Ferreira , Sandro M. R. Micheletti , J. C. C. de Souza , E. Abdalla

Inflation has long been the accepted paradigm for understanding the early universe. Most models of inflation have a scalar field acting as the inflaton particle which decays after inflation during a process called reheating into standard…

广义相对论与量子宇宙学 · 物理学 2018-11-30 Abhass Kumar

A new formulation of perturbation theory for a description of the Dirac and scalar fields (the Yukawa model) is suggested. As the main approximation the self-consistent field model is chosen, which allows in a certain degree to account for…

综合物理 · 物理学 2016-06-01 Yu. M. Poluektov

Yukawa interactions can mediate relatively long-range attractive forces between fermions in the early universe. Such a globally attractive interaction creates an instability that can result in the growth of structure in the affected species…

宇宙学与河外天体物理 · 物理学 2023-09-18 Ruth Durrer , Alexander Kusenko

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

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

We argue that, when coupled to Einstein's theory of gravity, the Yukawa theory may solve the cosmological constant problem in the following sense: The radiative corrections of fermions generate an effective potential for the scalar field,…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Tomislav Prokopec

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 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 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

By solving the gap equation in the quenched, ladder approximation for an Abelian gauge model with Yukawa interaction in the presence of a constant magnetic field, we show that the Yukawa interactions enhance the dynamical generation of…

高能物理 - 唯象学 · 物理学 2009-10-31 Efrain J. Ferrer , Vivian de la Incera

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

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

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