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相关论文: Cosmology with decaying tachyon matter

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Spatially averaged inhomogeneous cosmologies in classical general relativity can be written in the form of effective Friedmann equations with sources that include backreaction terms. In this paper we propose to describe these backreaction…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Thomas Buchert , Julien Larena , Jean-Michel Alimi

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

In this study we explore the cosmological behavior of a non-minimally coupled scalar field that is linked to torsion gravity. We demonstrate the Sorkin-Schutz formalism with general power law teleparallel torsion coupling. The autonomous…

广义相对论与量子宇宙学 · 物理学 2025-04-08 S. A. Kadam

The impact of a fast decaying component of mass-energy, that decreases faster than radiation with the increase of the scale factor, on the evolution of the universe is studied using a hydrodynamic approach. Proceeding from the Hamiltonian…

广义相对论与量子宇宙学 · 物理学 2024-12-10 V. E. Kuzmichev , V. V. Kuzmichev

The prevailing cosmological model with the lambda-term, in which the space is flat, is studied (section 1). The corresponding age of the Universe (t0) is calculated (assuming a Hubble constant consistent with the measurements of the Hubble…

天体物理学 · 物理学 2009-09-29 Evangelos Chaliasos

We get the same degeneracy relation between $w_0$ and $w_a$ for the tachyon fields as for quintessence and phantom fields. Our results show that the dynamics of scalar fields with different origins becomes indistinguishable when the…

广义相对论与量子宇宙学 · 物理学 2013-09-10 Ximing Chen , Yungui Gong

The work deals with homogeneous and isotropic, flat FRW model of the universe which is filled up with non-interacting dark matter and dark energy to compatible with recent observational evidences. By choosing the dark energy in the form of…

广义相对论与量子宇宙学 · 物理学 2013-05-09 Nilanjana Mahata , Subenoy Chakraborty

In this paper we propose a new dark energy model in the teleparallel alternative of general relativity, by considering a generalized non--minimal coupling of a tachyonic scalar field with the teleparallel boundary term. Within the framework…

广义相对论与量子宇宙学 · 物理学 2019-04-15 Sebastian Bahamonde , Mihai Marciu , Jackson Levi Said

The observed dark energy in the universe might give particles inertial mass. We investigate one realization of this idea, that the dark energy field might be a decayed scalar component of a supermultiplet field in the early universe that…

天体物理学 · 物理学 2007-05-23 Robert J. Nemiroff , Bijunath Patla

A cosmological model that aims at solving the coincidence problem should show that dark energy and dark matter follow the same scaling solution from some time onward. At the same time, the model should contain a sufficiently long…

天体物理学 · 物理学 2009-11-11 Luca Amendola , Miguel Quartin , Shinji Tsujikawa , Ioav Waga

We study the Brans-Dicke model in the presence of an axion. The dynamical equations are solved when the fields are space independent and the metric is spatially flat. It is found that at late time the scale factor undergoes decelerated…

高能物理 - 理论 · 物理学 2009-10-30 Sudipta Mukherji

We propose that dark energy in the form of a scalar field could effectively couple to dark matter inhomogeneities. Through this coupling energy could be transferred to/from the scalar field, which could possibly enter an accelerated regime.…

宇宙学与河外天体物理 · 物理学 2016-04-25 Valerio Marra

The dynamical behavior of tachyon field with an inverse potential is investigated in loop quantum cosmology. It reveals that the late time behavior of tachyon field with this potential leads to a power-law expansion. In addition, an…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Fei Huang , Kui Xiao , Jian-Yang Zhu

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

It is investigated the cosmological dynamics of scalar-torsion $f(T,\phi)$ gravity as a dark energy model, where $T$ is the torsion scalar of teleparallel gravity and $\phi$ is a canonical scalar field. In this context, we are concerned…

广义相对论与量子宇宙学 · 物理学 2021-06-16 Manuel Gonzalez-Espinoza , Giovanni Otalora

In this work, we have considered a model of the flat FRW universe filled with cold dark matter and Chameleon field where the scale function is taken as, (i) Intermediate Expansion and (ii) Logamediate Expansion. In the both cases we find…

广义相对论与量子宇宙学 · 物理学 2011-09-30 Piyali Bagchi Khatua , Ujjal Debnath

The idea that coherent oscillations of a scalar field, oscillating over a time period that is much shorter than the cosmological timescale, can exhibit cold dark matter (CDM) like behavior was previously established. In our work we first…

广义相对论与量子宇宙学 · 物理学 2025-12-24 Priyanka Saha , Dipanjan Dey , Kaushik Bhattacharya

Cosmological scaling solutions, which give rise to a scalar-field density proportional to a background fluid density during radiation and matter eras, are attractive to alleviate the energy scale problem of dark energy. In the presence of…

广义相对论与量子宇宙学 · 物理学 2010-03-25 Junko Ohashi , Shinji Tsujikawa

Recently it has been argued that a possible source for the dark energy may arise due to the contribution to the vacuum energy of the QCD ghost in a time-dependent background. In this paper we establish a connection between interacting ghost…

高能物理 - 理论 · 物理学 2012-04-10 A. Sheykhi , M. Sadegh Movahed , E. Ebrahimi

This work deals with $F(T)$ gravity models driven by real scalar fields with usual and phantom dynamics. We illustrate the results with examples of current interest, and we find some analytical solutions for scale factors and scalar fields.…

广义相对论与量子宇宙学 · 物理学 2010-06-22 K. K. Yerzhanov , Sh. R. Myrzakul , I. I. Kulnazarov , R. Myrzakulov
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