×

Holographic DBI-essence dark energy via power-law solution of the scale factor. (English) Zbl 1282.83063

Summary: The present work reports a Holographic reconstruction of Dirac-Born-Infeld (DBI)-essence Dark Energy (DE) in a flat FRW universe. The scale factor \(a(t)\) is chosen in power law form. We have reconstructed the scalar field and potential and subsequently the equation of state (EoS) parameter \(\omega\) of the DBI-essence DE. The corresponding plots show increasing scalar field, decaying tension and decaying potential. The reconstructed EoS parameter stays below \(-1\), showing a phantom-like behavior. The stability of the reconstructed DBI-essence DE is investigated through squared speed of sound \(v_s^2\): its negative sign reveals that the holographically reconstructed DBI-essence is classically unstable.

MSC:

83F05 Relativistic cosmology
Full Text: DOI

References:

[1] Spergel, D. N.; etal., No article title, Astrophys. J. Suppl. Ser., 148, 175 (2003) · doi:10.1086/377226
[2] Perlmutter, S.; etal., No article title, Astrophys. J., 517, 565 (1999) · Zbl 1368.85002 · doi:10.1086/307221
[3] Komatsu, E.; Smith, K. M.; Dunkley, J.; Bennett, C. L.; etal., No article title, Astrophys. J. Suppl. Ser., 192, 18 (2011) · doi:10.1088/0067-0049/192/2/18
[4] Cardone, V.F., Radicella, N., Camera, S.: arXiv:1204.5294 [astro-ph.CO]
[5] Frieman, J. A.; Turner, M. S.; Huterer, D., No article title, Annu. Rev. Astron. Astrophys., 46, 385 (2008) · doi:10.1146/annurev.astro.46.060407.145243
[6] Copeland, E. J.; Sami, M.; Tsujikawa, S., No article title, Int. J. Mod. Phys. D, 15, 1753 (2006) · Zbl 1203.83061 · doi:10.1142/S021827180600942X
[7] Padmanabhan, T., No article title, Phys. Rep., 380, 235 (2003) · Zbl 1027.83544 · doi:10.1016/S0370-1573(03)00120-0
[8] Bamba, K.; Capozziello, S.; Nojiri, S.; Odintsov, S. D., No article title, Astrophys. Space Sci., 342, 155 (2012) · Zbl 1314.83037 · doi:10.1007/s10509-012-1181-8
[9] Setare, M. R., No article title, Phys. Lett. B, 653, 116 (2007) · Zbl 1246.83273 · doi:10.1016/j.physletb.2007.08.011
[10] Horava, P.; Minic, D., No article title, Phys. Rev. Lett., 85, 1610 (2000) · Zbl 1369.83106 · doi:10.1103/PhysRevLett.85.1610
[11] Thomas, S. D., No article title, Phys. Rev. Lett., 89 (2002) · Zbl 1267.83044 · doi:10.1103/PhysRevLett.89.081301
[12] Li, M., No article title, Phys. Lett. B, 603, 1 (2004) · doi:10.1016/j.physletb.2004.10.014
[13] Fay, S.; Tavakol, R., No article title, Phys. Rev. D, 74 (2006) · doi:10.1103/PhysRevD.74.083513
[14] Jamil, M.; Farooq, M. U., No article title, Int. J. Theor. Phys., 49, 42 (2010) · Zbl 1186.83123 · doi:10.1007/s10773-009-0176-x
[15] Jamil, M.; Farooq, M. U.; Rashid, M. A., No article title, Eur. Phys. J. C, 61, 471 (2009) · doi:10.1140/epjc/s10052-009-1021-3
[16] Martin, J.; Yamaguchi, M., No article title, Phys. Rev. D, 77 (2008) · doi:10.1103/PhysRevD.77.123508
[17] Setare, M. R., No article title, Phys. Lett. B, 644, 99 (2007) · Zbl 1248.83178 · doi:10.1016/j.physletb.2006.11.033
[18] Setare, M. R., No article title, Phys. Lett. B, 648, 329 (2007) · Zbl 1248.83179 · doi:10.1016/j.physletb.2007.03.025
[19] Setare, M. R., No article title, Phys. Lett. B, 654, 1 (2007) · doi:10.1016/j.physletb.2007.08.038
[20] Jamil, M.; Farooq, M. U., No article title, Int. J. Theor. Phys., 49, 42 (2010) · Zbl 1186.83123 · doi:10.1007/s10773-009-0176-x
[21] Farooq, M. U.; Jamil, M.; Rashid, M. A., No article title, Int. J. Theor. Phys., 49, 2334 (2010) · Zbl 1201.83048 · doi:10.1007/s10773-010-0420-4
[22] Sheykhi, A.; Jamil, M., No article title, Phys. Lett. B, 694, 284 (2011) · doi:10.1016/j.physletb.2010.10.019
[23] Karami, K.; Khaledian, M. S.; Jamil, M., No article title, Phys. Scr., 83 (2011) · Zbl 1221.83044 · doi:10.1088/0031-8949/83/02/025901
[24] Sheykhi, A.; Karami, K.; Jamil, M.; Kazemi, E.; Haddad, M., No article title, Int. J. Theor. Phys., 51, 1663 (2012) · Zbl 1252.83124 · doi:10.1007/s10773-011-1043-0
[25] Pasqua, A.; Jamil, M.; Myrzakulov, R.; Majeed, B., No article title, Phys. Scr., 86 (2012) · Zbl 1263.83193 · doi:10.1088/0031-8949/86/04/045004
[26] Chattopadhyay, S.; Debnath, U., No article title, Int. J. Theor. Phys., 49, 1465 (2010) · Zbl 1197.83061 · doi:10.1007/s10773-010-0328-z
[27] Setare, M. R., No article title, Int. J. Mod. Phys. D, 12, 2219 (2008) · Zbl 1180.83108 · doi:10.1142/S0218271808013819
[28] Setare, M. R., No article title, Phys. Rev. D, 18, 419 (2008)
[29] Myung, Y. S., No article title, Phys. Lett. B, 652, 223 (2007) · Zbl 1248.83170 · doi:10.1016/j.physletb.2007.07.033
[30] Kim, K. Y.; Lee, H. W.; Myung, Y. S., No article title, Phys. Lett. B, 660, 118 (2008) · doi:10.1016/j.physletb.2007.12.045
[31] Sharif, M.; Jawad, A., No article title, Eur. Phys. J. C, 72, 2097 (2012) · doi:10.1140/epjc/s10052-012-2097-8
[32] Jawad, A.; Pasqua, A.; Chattopadhyay, S., No article title, Astrophys. Space Sci., 344, 489 (2013) · doi:10.1007/s10509-012-1345-6
[33] Barrow, J. D.; Tsagas, C. G., No article title, Class. Quantum Gravity, 22, 1563 (2005) · Zbl 1072.83030 · doi:10.1088/0264-9381/22/9/006
[34] Jawad, A.; Chattopadhyay, S.; Pasqua, A., No article title, Astrophys. Space Sci. (2013) · doi:10.1007/s10509-013-1428-z
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.