H. Hossienkhani, V. Fayaz, S. A. A. Terohid, N. Azimi, Z. Zarei, M. Ganji, “Anisotropic cosmology with a dilaton field coupled to ghost dark energy”, TMF, 194:3 (2018), 481–509; Theoret. and Math. Phys., 194:3 (2018), 415

Teoreticheskaya i Matematicheskaya Fizika

RUS ENG

JOURNALS PEOPLE ORGANISATIONS CONFERENCES SEMINARS VIDEO LIBRARY PACKAGE AMSBIB

JavaScript is disabled in your browser. Please switch it on to enable full functionality of the website

	General information
	Latest issue
	Archive
	Impact factor
	Guidelines for authors
	License agreement
	Submit a manuscript

	Search papers
	Search references

	RSS
	Latest issue
	Current issues
	Archive issues
	What is RSS

TMF:
Year:
Volume:
Issue:
Page:
	Find

Personal entry:
Login:
Password:
	Save password
	Enter
	Forgotten password?
	Register

Teoreticheskaya i Matematicheskaya Fizika, 2018, Volume 194, Number 3, Pages 481–509
DOI: https://doi.org/10.4213/tmf9323 (Mi tmf9323)

This article is cited in 7 scientific papers (total in 7 papers)

Anisotropic cosmology with a dilaton field coupled to ghost dark energy

H. Hossienkhani^a, V. Fayaz^a, S. A. A. Terohid^a, N. Azimi^b, Z. Zarei^a, M. Ganji^a

^a Department of Physics, Hamedan Branch, Islamic Azad University, Hamedan, Iran
^b Department of Mathematics, Hamedan Branch, Islamic Azad University, Hamedan, Iran

Full-text PDF (1167 kB) Citations (7)

References:

PDF

HTML

DOI: https://doi.org/10.4213/tmf9323

Abstract: We study a dilaton scalar field coupled to ghost dark energy in an anisotropic universe. The evolution of dark energy, which dominates the universe, can be completely described by a single dilaton scalar field. This connection allows reconstructing the kinetic energy and also the dynamics of the dilaton scalar field according to the evolution of the energy density. Using the latest observational data, we obtain bounds on the ghost dark energy models and also on generalized dark matter and dark energy. For this, we investigate how the expansion history

$H(z)$ is determined by observational quantities. We calculate the evolution of density perturbations in the linear regime for both ghost and generalized ghost dark energy and compare the results with

$\Lambda$ CDM models. We discuss the justification of the generalized second law of thermodynamics in a Bianchi type-I universe. The obtained model is stable for large time intervals but is unstable at small times.

Keywords: anisotropic universe, ghost dark energy, generalized ghost dark energy, dilaton scalar field, generalized second law of thermodynamics, perturbation theory.

Received: 16.12.2016
Revised: 29.03.2017

English version:
Theoretical and Mathematical Physics, 2018, Volume 194, Issue 3, Pages 415–438
DOI: https://doi.org/10.1134/S0040577918030091

Bibliographic databases:

Document Type: Article

PACS: 95.36.+x, 95.35.+d, 98.80.-k

Language: Russian

Citation: H. Hossienkhani, V. Fayaz, S. A. A. Terohid, N. Azimi, Z. Zarei, M. Ganji, “Anisotropic cosmology with a dilaton field coupled to ghost dark energy”, TMF, 194:3 (2018), 481–509; Theoret. and Math. Phys., 194:3 (2018), 415–438

Citation in format AMSBIB

\Bibitem{HosFayTer18}

\by H.~Hossienkhani, V.~Fayaz, S.~A.~A.~Terohid, N.~Azimi, Z.~Zarei, M.~Ganji

\paper Anisotropic cosmology with a~dilaton field coupled to ghost dark

energy

\jour TMF

\yr 2018

\vol 194

\issue 3

\pages 481--509

\mathnet{http://mi.mathnet.ru/tmf9323}

\crossref{https://doi.org/10.4213/tmf9323}

\mathscinet{http://mathscinet.ams.org/mathscinet-getitem?mr=3769238}

\elib{https://elibrary.ru/item.asp?id=32641418}

\transl

\jour Theoret. and Math. Phys.

\yr 2018

\vol 194

\issue 3

\pages 415--438

\crossref{https://doi.org/10.1134/S0040577918030091}

\isi{https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=Publons&SrcAuth=Publons_CEL&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=000429233100009}

\scopus{https://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-85044945936}

Linking options:

https://www.mathnet.ru/eng/tmf9323

https://doi.org/10.4213/tmf9323

https://www.mathnet.ru/eng/tmf/v194/i3/p481

This publication is cited in the following 7 articles:

H. Hossienkhani, F. Mahmoodi, V. Fayaz, S. A. A. Terohid, N. Azimi, Z. Zarei, “Phantom cosmologies from the simplest parameterization of the DE model using observational data in a BI type universe”, Chinese Phys. C, 47:11 (2023), 115104
A. Najafi, H. Hossienkhani, “Using Pantheon and Hubble parameter data to constrain the Ricci dark energy in a Bianchi I Universe”, Commun. Theor. Phys., 74:6 (2022), 065401
H. Hossienkhani, N. Azimi, H. Yousefi, “Constraints on the Ricci dark energy cosmologies in Bianchi type i model”, Int. J. Geom. Methods Mod. Phys., 18:06 (2021), 2150095
S. A. A. Terohid, H. Hossienkhani, “Anisotropy effects and observational data on the constraints of evolution dark energy models”, Commun. Theor. Phys., 71:1 (2019), 79–90
S. D. Katore, D. V. Kapse, “Dynamical behavior of coupled magnetized dark energy in lyra's geometry”, Astrophysics, 62:3 (2019), 415–433
H. Hossienkhani, H. Yousefi, N. Azimi, “Testing anisotropy and comparison of various supernova data constraints on dark energy model”, Mod. Phys. Lett. A, 34:34 (2019), 1950276
H. Hossienkhani, H. Yousefi, N. Azimi, “Effect of low anisotropy on cosmological models by using supernova data”, New Astronomy, 68 (2019), 65

Citing articles in Google Scholar: Russian citations, English citations
Related articles in Google Scholar: Russian articles, English articles

Statistics & downloads:
Abstract page:	351
Full-text PDF :	113
References:	46
First page:	6

Registration to the website

Logotypes