Co-existence of modified Chaplygin gas and other dark energies in the framework of fractal universe. (English) Zbl 1338.83220
Summary: In this work, we consider a non-flat universe in the framework of fractal cosmology. We have investigated the co-existence of different kinds of dark energy models such as tachyonic field, DBI-essence, hessence, k-essence, dilaton, quintessence with the modified Chaplygin gas (MCG) in fractal universe and obtained the statefinder parameters. The natures of the scalar fields and the concerned potentials have been analyzed by the correspondence scenario in the fractal universe.
MSC:
| 83F05 | Relativistic cosmology |
References:
| [1] | Perlmutter, S.; etal., No article title, Astrophys. J., 517, 565 (1999) · Zbl 1368.85002 · doi:10.1086/307221 |
| [2] | Riess, AG; etal., No article title, Astron. J., 116, 1009 (1998) · doi:10.1086/300499 |
| [3] | Sen, A., No article title, JHEP, 0207, 065 (2002) · doi:10.1088/1126-6708/2002/07/065 |
| [4] | Wei, H.; Cai, RG; Zhang, DF, No article title, Class. Quantum Grav., 22, 3189 (2005) · Zbl 1075.83574 · doi:10.1088/0264-9381/22/16/005 |
| [5] | Lu, H.Q., et al.: arXiv:0409309 [hep-th] |
| [6] | Martin, J.; Yamaguchi, M., No article title, Phys. Rev. D, 77, 103508 (2008) · doi:10.1103/PhysRevD.77.103508 |
| [7] | Armendariz-Picon, C.; etal., No article title, Phys. Rev. D, 63, 103510 (2001) · doi:10.1103/PhysRevD.63.103510 |
| [8] | Peebles, PJE; Ratra, B., No article title, Astrophys. J., 325, l17 (1988) · doi:10.1086/185100 |
| [9] | Caldwell, RR; Dave, R.; Steinhardt, PJ, No article title, Phys. Rev. Lett., 80, 1582 (1998) · Zbl 1371.83193 · doi:10.1103/PhysRevLett.80.1582 |
| [10] | Calcagni, G., No article title, JHEP, 1003, 120 (2010) · Zbl 1271.83032 · doi:10.1007/JHEP03(2010)120 |
| [11] | Setare, MR, No article title, Phys. Lett. B, 648, 329-332 (2007) · Zbl 1248.83179 · doi:10.1016/j.physletb.2007.03.025 |
| [12] | Setare, MR, No article title, Phys. Lett. B, 653, 116-121 (2007) · Zbl 1246.83273 · doi:10.1016/j.physletb.2007.08.011 |
| [13] | Setare, MR, No article title, Phys. Lett. B, 654, 1-6 (2007) · doi:10.1016/j.physletb.2007.08.038 |
| [14] | Setare, MR, No article title, Eur. Phys. J.C, 52, 689-692 (2007) · doi:10.1140/epjc/s10052-007-0405-5 |
| [15] | Setare, MR, No article title, Int. J. Mod. Phys. D, 18, 419-427 (2009) · Zbl 1173.83319 · doi:10.1142/S0218271809014558 |
| [16] | Karami, K., et al.: arXiv:1201.6233v1 [physics.gen-ph] |
| [17] | Lemets, O.A., et al.: arXiv:1202.3457v3 [astro-ph.CO] |
| [18] | Sheykhi, A., et al.: arXiv:1212.2137v3 [physics.gen-ph] |
| [19] | Chattopadhyay, S.; Pasqua, A.; Roy, S., No article title, ISRN High Energy Phys., 2013, 251498 (2013) · Zbl 1362.83028 |
| [20] | Debnath, U.; Banerjee, A.; Chakraborty, S., No article title, Class. Quantum Grav., 21, 5609 (2004) · Zbl 1065.83063 · doi:10.1088/0264-9381/21/23/019 |
| [21] | Gumjudpai, B.; Ward, J., No article title, Phys. Rev. D, 80, 023528 (2009) · doi:10.1103/PhysRevD.80.023528 |
| [22] | Copeland, EJ; Sami, M.; Tsujikawa, S., No article title, Int. J. Mod. Phys. D, 15, 1753 (2006) · Zbl 1203.83061 · doi:10.1142/S021827180600942X |
| [23] | Armendáriz-Picón, C.; Damour, T.; Mukhanov, V., No article title, Phys. Lett. B, 458, 209 (1999) · Zbl 0992.83096 · doi:10.1016/S0370-2693(99)00603-6 |
| [24] | Chiba, T.; Okabe, T.; Yamaguchi, M., No article title, Phys. Rev. D, 62, 023511 (2000) · doi:10.1103/PhysRevD.62.023511 |
| [25] | Gasperini, M.; etal., No article title, Phys. Rev. D, 65, 023508 (2002) · doi:10.1103/PhysRevD.65.023508 |
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