Interaction between modified Chaplygin gas and ghost dark energy in the presence of extra dimensions

被引：11

作者：

Khurshudyan, M. ^{[1
]}

Sadeghi, J. ^{[2
]}

Hakobyan, M. ^{[3
,4
]}

Farahani, H. ^{[2
]}

Myrzakulov, R. ^{[5
]}

机构：

[1] Yerevan State Univ, Dept Theoret Phys, Yerevan 0025, Armenia

[2] Mazandaran Univ, Dept Phys, Babol Sar, Iran

[3] AI Alikhanyan Natl Sci Lab, Yerevan, Armenia

[4] Yerevan State Univ, Dept Nucl Phys, Yerevan 0025, Armenia

[5] Eurasian Natl Univ, Eurasian Int Ctr Theoret Phys, Astana 010008, Kazakhstan

来源：

EUROPEAN PHYSICAL JOURNAL PLUS | 2014年 / 129卷 / 06期

关键词：

COSMOLOGICAL CONSTANT; MODEL; VISCOSITY; DENSITY; MATTER;

D O I：

10.1140/epjp/i2014-14119-x

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In this paper, we consider three different models of dark energy in higher-dimensional space-time and discuss some cosmological parameters numerically. The first model is a single-component universe including viscous varying modified Chaplygin gas. In the second model, we consider a two-component universe including viscous varying modified Chaplygin gas and ghost dark energy. In the third model, we consider another two-component universe including viscous modified cosmic Chaplygin gas and ghost dark energy. In the cases of two-component fluids we also consider the possibility of interaction between components.

引用

页数：8

共 50 条

[41] Ghost Dark Energy with Sign-changeable Interaction Term [J].

Zadeh, M. Abdollahi ;

Sheykhi, A. ;

Moradpour, H. .

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2017, 56 (11) :3477-3495

[42] Reconstruction of f(G) gravity with polytropic and Chaplygin gas dark energy models [J].

Azizi, T. ;

Naserinia, P. .

EUROPEAN PHYSICAL JOURNAL PLUS, 2017, 132 (09)

[43] Observational constraints on modified Chaplygin gas in Horava-Lifshitz gravity with dark radiation [J].

Paul, B. C. ;

Thakur, P. ;

Verma, M. M. .

PRAMANA-JOURNAL OF PHYSICS, 2013, 81 (04) :691-718

[44] Interacting modified QCD ghost scalar field models of dark energy [J].

Jawad, Abdul .

ASTROPHYSICS AND SPACE SCIENCE, 2015, 357 (01)

[45] The dark energy interacting with the extended Chaplygin gas in F (R,T) gravity formalism [J].

Abdelhakim Bensaid ;

Rachid Bouamrane .

Indian Journal of Physics, 2019, 93 :1095-1101

[46] Normal oscillation modes and radial stability of neutron stars with a dark-energy core from the Chaplygin gas [J].

Pretel, Juan M. Z. ;

Dutra, Mariana ;

Duarte, Sergio B. .

PHYSICAL REVIEW D, 2024, 109 (02)

[47] Understanding the interaction between dark energy and dark matter [J].

Wang Bin .

HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION, 2007, 31 (09) :874-879

[48] Vestiges of the interaction between dark energy and dark matter [J].

He, Jian-Hua ;

Wang, Bin .

PHYSICS AND MATHEMATICS OF GRAVITATION, 2009, 1122 :292-295

[49] Co-Existence of Modified Chaplygin Gas and Other Dark Energies in the Framework of Fractal Universe [J].

Maity, Sayani ;

Debnath, Ujjal .

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2016, 55 (05) :2668-2681

[50] Fermionic DBI and Chaplygin gas unified models of dark energy and dark matter from f-essence [J].

Momeni, D. ;

Myrzakulov, Y. ;

Tsyba, P. ;

Yesmakhanova, K. ;

Myrzakulov, R. .

3RD ITALIAN-PAKISTANI WORKSHOP ON RELATIVISTIC ASTROPHYSICS (IPWRA2011), 2012, 354

← 1 2 3 4 5 →