Abstract.
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.
Similar content being viewed by others
References
M. Jamil, U. Debnath, Int. J. Theor. Phys. 50, 1602 (2011)
M. Jamil, F. Rahaman, M. Kalam, Eur. Phys. J. C 60, 149 (2009)
B. Ratra, P. Peebles, Phys. Rev. D 37, 3406 (1988)
I. Zlatev, L.-M. Wang, P.J. Steinhardt, Phys. Rev. Lett. 82, 896 (1999)
Z.-K. Guo, N. Ohta, Y.-Z. Zhang, Mod. Phys. Lett. A 22, 883 (2007)
S. Dutta, E.N. Saridakis, R.J. Scherrer, Phys. Rev. D 79, 103005 (2009)
E.N. Saridakis, S.V. Sushkov, Phys. Rev. D 81, 083510 (2010)
M. Khurshudyan, E. Chubaryan, B. Pourhassan, Int. J. Theor. Phys. (2014) DOI:10.1007/s10773-014-2036-6
R.R. Caldwell, M. Kamionkowski, N.N. Weinberg, Phys. Rev. Lett. 91, 071301 (2003)
S. Nojiri, S.D. Odintsov, Phys. Lett. B 562, 147 (2003)
P. Singh, M. Sami, N. Dadhich, Phys. Rev. D 68, 023522 (2003)
M. Setare, E. Saridakis, JCAP 03, 002 (2009)
S. Capozziello, S. Nojiri, S. Odintsov, Phys. Lett. B 632, 597 (2006)
Y.-F. Cai, T. Qiu, Y.-S. Piao, M. Li, X. Zhang, JHEP 10, 071 (2007)
E.N. Saridakis, J.M. Weller, Phys. Rev. D 81, 123523 (2010)
M. Setare, E. Saridakis, Int. J. Mod. Phys. D 18, 549 (2009)
Y.-F. Cai, E.N. Saridakis, M.R. Setare, J.-Q. Xia, Phys. Rep. 493, 1 (2010)
T. Qiu, Mod. Phys. Lett. A 25, 909 (2010)
Q.-G. Huang, M. Li, JCAP 08, 013 (2004)
M. Ito, Europhys. Lett. 71, 712 (2005)
H. Li, Z.-K. Guo, Y.-Z. Zhang, Int. J. Mod. Phys. D 15, 869 (2006)
E. Saridakis, JCAP 04, 020 (2008)
M.R. Setare, Phys. Lett. B 648, 329 (2007)
J. Sadeghi, B. Pourhassan, Z.A. Moghaddam, Int. J. Theor. Phys. 53, 125 (2014)
M.R. Setare, Phys. Lett. B 654, 1 (2007)
H. Wei, R.-G. Cai, Eur. Phys. J. C 59, 99 (2009)
L. Xu, J. Lu, Y. Wang, Eur. Phys. J. C 72, 1883 (2012)
H. Saadat, B. Pourhassan, Int. J. Theor. Phys. 53, 1168 (2014)
Xiang-Hua Zhai et al., Int. J. Mod. Phys. D 15, 1151 (2006)
Y.D. Xu et al., Astrophys. Space Sci. 337, 493 (2012)
Ali.R. Amani, B. Pourhassan, Int. J. Theor. Phys. 52, 1309 (2013)
H. Saadat, B. Pourhassan, Int. J. Theor. Phys. 52, 3712 (2013)
M. Khurshudyan, E.O Kahya, A. Pasqua, B. Pourhassan, arXiv:1401.6630 [gr-qc]
M. Khurshudyan, Cent. Eur. J. Phys. 12, 348 (2014)
U. Debnath, A. Banerjee, S. Chakraborty, Class. Quantum Grav. 21, 5609 (2004)
J. Sadeghi, M. Khurshudyan, B. Pourhassan, H. Farahani, Int. J. Theor. Phys. 53, 911 (2014)
H. Saadat, B. Pourhassan, Astrophys. Space Sci. 343, 783 (2013)
J. Naji, B. Pourhassan, A.R. Amani, Int. J. Mod. Phys. D 23, 1450020 (2013)
J. Sadeghi, M. Khurshudyan, B. Pourhassan, H. Farahani, Int. J. Theor. Phys. 53, 911 (2014)
H. Saadat, B. Pourhassan, Astrophys. Space Sci. 344, 237 (2013)
J. Sadeghi, H. Farahani, Astrophys. Space Sci. 347, 209 (2013)
B. Pourhassan, Int. J. Mod. Phys. D 22, 1350061 (2013)
F.R. Urban, A.R. Zhitnitsky, Phys. Rev. D 80, 063001 (2009)
R.-G. Cai, Z.-L. Tuo, H.-B. Zhang, Q. Su, Phys. Rev. D 84, 123501 (2011)
E. Ebrahimi, A. Sheykhi, Int. J. Mod. Phys. D 20, 2369 (2011)
C.-J. Feng, X.-Z. Li, P. Xi, JHEP 05, 046 (2012)
C.-J. Feng, X.-Z. Li, X.-Y. Shen, Phys. Rev. D 87, 023006 (2013)
J. Sadeghi, M. Khurshudyan, A. Movsisyan, H. Farahan, JCAP 12, 031 (2013)
A.R. Amani, B. Pourhassan, Int. J. Theor. Phys. 51, 49 (2012)
M. Khurshudyan, B. Pourhassan, E.O. Kahya, Int. J. Geom. Methods Mod. Phys. 11, 1450061 (2014)
S. Chakraborty, U. Debnath, M. Jamil, Can. J. Phys. 90, 365 (2012)
Author information
Authors and Affiliations
Corresponding authors
Rights and permissions
About this article
Cite this article
Khurshudyan, M., Sadeghi, J., Hakobyan, M. et al. Interaction between modified Chaplygin gas and ghost dark energy in the presence of extra dimensions. Eur. Phys. J. Plus 129, 119 (2014). https://doi.org/10.1140/epjp/i2014-14119-x
Received:
Revised:
Accepted:
Published:
DOI: https://doi.org/10.1140/epjp/i2014-14119-x