Abstract
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 ω 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.
Similar content being viewed by others
References
Spergel, D.N., et al.: Astrophys. J. Suppl. Ser. 148, 175 (2003)
Perlmutter, S., et al.: Astrophys. J. 517, 565 (1999)
Komatsu, E., Smith, K.M., Dunkley, J., Bennett, C.L., et al.: Astrophys. J. Suppl. Ser. 192, 18 (2011)
Cardone, V.F., Radicella, N., Camera, S.: arXiv:1204.5294 [astro-ph.CO]
Frieman, J.A., Turner, M.S., Huterer, D.: Annu. Rev. Astron. Astrophys. 46, 385 (2008)
Copeland, E.J., Sami, M., Tsujikawa, S.: Int. J. Mod. Phys. D 15, 1753 (2006)
Padmanabhan, T.: Phys. Rep. 380, 235 (2003)
Bamba, K., Capozziello, S., Nojiri, S., Odintsov, S.D.: Astrophys. Space Sci. 342, 155 (2012)
Setare, M.R.: Phys. Lett. B 653, 116 (2007)
Horava, P., Minic, D.: Phys. Rev. Lett. 85, 1610 (2000)
Thomas, S.D.: Phys. Rev. Lett. 89, 081301 (2002)
Li, M.: Phys. Lett. B 603, 1 (2004)
Fay, S., Tavakol, R.: Phys. Rev. D 74, 083513 (2006)
Jamil, M., Farooq, M.U.: Int. J. Theor. Phys. 49, 42 (2010)
Jamil, M., Farooq, M.U., Rashid, M.A.: Eur. Phys. J. C 61, 471 (2009)
Martin, J., Yamaguchi, M.: Phys. Rev. D 77, 123508 (2008)
Setare, M.R.: Phys. Lett. B 644, 99 (2007)
Setare, M.R.: Phys. Lett. B 648, 329 (2007)
Setare, M.R.: Phys. Lett. B 654, 1 (2007)
Jamil, M., Farooq, M.U.: Int. J. Theor. Phys. 49, 42 (2010)
Farooq, M.U., Jamil, M., Rashid, M.A.: Int. J. Theor. Phys. 49, 2334 (2010)
Sheykhi, A., Jamil, M.: Phys. Lett. B 694, 284 (2011)
Karami, K., Khaledian, M.S., Jamil, M.: Phys. Scr. 83, 025901 (2011)
Sheykhi, A., Karami, K., Jamil, M., Kazemi, E., Haddad, M.: Int. J. Theor. Phys. 51, 1663 (2012)
Pasqua, A., Jamil, M., Myrzakulov, R., Majeed, B.: Phys. Scr. 86, 045004 (2012)
Chattopadhyay, S., Debnath, U.: Int. J. Theor. Phys. 49, 1465 (2010)
Setare, M.R.: Int. J. Mod. Phys. D 12, 2219 (2008)
Setare, M.R.: Phys. Rev. D 18, 419 (2008)
Myung, Y.S.: Phys. Lett. B 652, 223 (2007)
Kim, K.Y., Lee, H.W., Myung, Y.S.: Phys. Lett. B 660, 118 (2008)
Sharif, M., Jawad, A.: Eur. Phys. J. C 72, 2097 (2012)
Jawad, A., Pasqua, A., Chattopadhyay, S.: Astrophys. Space Sci. 344, 489 (2013)
Barrow, J.D., Tsagas, C.G.: Class. Quantum Gravity 22, 1563 (2005)
Jawad, A., Chattopadhyay, S., Pasqua, A.: Astrophys. Space Sci. (2013, online first). doi:10.1007/s10509-013-1428-z
Acknowledgements
The constructive suggestions from the reviewers are thankfully acknowledged. The first author acknowledges the facilities provided by the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune, India, during his visit under Visiting Associateship programme in December, 2012. The financial support from the Department of Science and Technology, Govt. of India under project grant no. SR/FTP/PS-167/2011 is duly acknowledged by the first author.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Chattopadhyay, S., Pasqua, A. Holographic DBI-Essence Dark Energy via Power-Law Solution of the Scale Factor. Int J Theor Phys 52, 3945–3952 (2013). https://doi.org/10.1007/s10773-013-1705-1
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10773-013-1705-1