Abstract
Om diagnostic can differentiate between different models of dark energy without the accurate current value of matter density. We apply this geometric diagnostic to dilaton dark energy (DDE) model and differentiate DDE model from LCDM. We also investigate the influence of coupled parameter α on the evolutive behavior of Om with respect to redshift z. According to the numerical result of Om, we get the current value of equation of state ω σ0=−0.952 which fits the WMAP5+BAO+SN very well.
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Acatrinei, C., Sochichiu, C.: Mod. Phys. Lett. A 18, 31 (2003)
Albrecht, A., Skordis, C.: Phys. Rev. Lett. 84, 2076 (2000)
Alexander, S.H.: Phys. Rev. D 65, 0203507 (2002)
Amendola, L., Quartin, M., Tsujikawa, S., Waga, I.: Phys. Rev. D 74, 023525 (2006a)
Amendola, L., Tsujikawa, S., Sami, M.: Phys. Lett. B 632, 155 (2006b)
Armendariz-Picon, C., Damour, T., Mukhanov, V.: Phys. Lett. B 458, 209 (1999)
Armendáriz-Picón, C., Mukhanov, V., Steinhardt, P.J.: Phys. Rev. Lett. 85, 4438 (2000)
Armendáriz-Picón, C., Mukhanov, V., Steinhardt, P.J.: Phys. Rev. D 63, 103510 (2001)
Bagla, J.S., Jassal, H.K., Padmamabhan, T.: Phys. Rev. D 67, 063504 (2003)
Bahcall, N.A., et al.: Science 284, 1481 (1999)
Bennett, C.L., et al.: Astrophys. Phys. Lett. 148, 1 (2003)
Chiba, T.: Phys. Rev. D 66, 063514 (2002)
Chiba, T., Okabe, T., Yamaguchi, M.: Phys. Rev. D 62, 023511 (2000)
Chimento, L.P.: Phys. Rev. D 69, 123517 (2004)
Cho, Y.M.: Phys. Rev. Lett. 68, 3133 (1992)
Copeland, E.J., Sami, M., Tsujikawa, S.: arXiv:hep-th/0603057v3 (2006)
Damour, T., Nordtvedt, K.: Phys. Rev. Lett. 70, 2217 (1993)
Elizalde, E., Nojiri, S., Odintsov, S.D.: arXiv:hep-th/0405034 (2004)
Fairbairn, M., Tytgat, M.H.: Phys. Lett. B 546, 1 (2002)
Fang, W., Lu, H.Q., Huang, Z.G., Zhang, K.F.: Int. J. Mod. Phys. D 15, 199 (2006)
Feinstein, A.: Phys. Rev. D 66, 063511 (2002)
Feng, B.: arXiv:astro-ph/0602156 (2006)
Frolov, A., Kofman, L., Starobinsky, A.: Phys. Lett. B 545, 8 (2002)
Gong, Y.G., Wang, B., Zhang, Y.Z.: Phys. Rev. D 72, 043510 (2005)
Guo, Z.K., Piao, Y.S., Zhang, X.M., Zhang, Y.Z.: Phys. Lett. B 608, 177 (2005)
Gupta, R.C., Pradhan, A.: Int. J. Theor. Phys. 49, 821 (2010)
Hinshaw, G., et al.: arXiv:0803.0732 (2008)
Huang, Q.G., Li, M.: J. Cosmol. Astropart. Phys. 0408, 013 (2004)
Huang, Q.G., Li, M.: J. Cosmol. Astropart. Phys. 0503, 001 (2005)
Huang, Z.G., Lu, H.Q.: Int. J. Mod. Phys. D 15, 1501 (2006)
Huang, Z.G., Lu, H.Q., Fang, W.: Class. Quantum Gravity 23, 6215 (2006). arXiv:hep-th/0604160
Huang, Z.G., Li, X.H., Sun, Q.Q.: Astrophys. Space Sci. 310, 53 (2007a). arXiv:hep-th/0610019
Huang, Z.G., Lu, H.Q., Fang, W.: Int. J. Mod. Phys. D 16, 1109 (2007b). arXiv:hep-th/0610018
Huang, Z.G., Song, X.M., Lu, H.Q., Fang, W.: Astrophys. Space Sci. 315, 179 (2008)
Ito, M.: Europhys. Lett. 71, 712–715 (2005)
Ke, K., Li, M.: Phys. Lett. B 606, 173–176 (2005)
Kofman, L., Linde, A., J. High Energy Phys. 0207, 004 (2004)
Kowalski, M., et al.: arXiv:0804.4142 (astro-ph) (2008)
Li, M.: Phys. Lett. B 603, 1 (2004). arXiv:hep-th/0403127
Lu, H.Q.: Int. J. Mod. Phys. D 14, 355 (2005)
Lu, J.B., Xu, L.X., Gui, Y.X., Chang, B.R.: arXiv:0812.2074 (astro-ph) (2008)
Malquarti, M., Copeland, E.J., Liddle, A.R., Trodden, M.: Phys. Rev. D 67, 123503 (2003)
Melchiorri, A., Mersini, L., Odman, C.J., Trodden, M.: Phys. Rev. D 68, 043509 (2003)
Nojiri, S., Odintsov, S.D.: Phys. Lett. B 639, 144 (2006)
Nolta, M.R., et al.: arXiv:0803.0593 (2008)
Padmanabhan, T., Choudhury, T.R.: Phys. Rev. D 66, 081301 (2002)
Perlmutter, S., et al.: Astrophys. J. 517, 565 (1999)
Riess, A.G., et al.: Astron. J. 116, 1009 (1998)
Riess, A.G., et al.: Astrophys. J. 607, 665 (2004)
Sahni, V., Shafieloo, A., Starobinsky, A.A.: Phys. Rev. D 78, 103502 (2008). arXiv:0807.3548 (astro-ph)
Sen, A.: J. High Energy Phys. 0204, 048 (2002)
Sherrer, R.J.: Phys. Rev. Lett. 93, 011301 (2004)
Singh, P., Sami, M., Dadhich, N.: Phys. Rev. D 68, 023522 (2003)
Skordis, C., Albrecht, A.: Phys. Rev. D 66, 043523 (2002)
Tegmark, M., et al.: Phys. Rev. D 69, 103510 (2004)
Tong, M.L., Zhang, Y.: Phys. Rev. D 80, 023503 (2009). arXiv:0906.3646 (gr-qc)
Wei, H., Cai, R.G., Zeng, D.F.: Class. Quantum Gravity 22, 3189 (2005)
Wetterich, C.: Nucl. Phys. B 302, 668 (1998)
Zhang, X.: Int. J. Mod. Phys. D 14, 1597–1606 (2005)
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Huang, Z.G., Lu, H.Q. & Zhang, K. Om diagnostic for dilaton dark energy. Astrophys Space Sci 331, 331–335 (2011). https://doi.org/10.1007/s10509-010-0437-4
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DOI: https://doi.org/10.1007/s10509-010-0437-4