Abstract
Applying the parametrization of dark energy density, we can construct directly independent-model potentials. In Born-Infeld type phantom dark energy model, we consider four special parametrization equation of state parameter. The evolutive behavior of dark energy density with respect to red-shift z, potentials with respect to φ and z are shown mathematically. Moreover, we investigate the effect of parameter η upon the evolution of the constructed potential with respect to z. These results show that the evolutive behavior of constructed Born-Infeld type dark energy model is quite different from those of the other models.
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Alam, U., Sahni, V., Saini, T.D., Starobinsky, A.A.: Mon. Not. R. Astron. Soc. 354, 275 (2004)
Amendola, L., Quartin, M., Tsujikawa, S., Waga, I.: Phys. Rev. D 74, 023525 (2006)
Armendáriz-Picón, C., Mukhanov, V., Steinhardt, P.J.: Phys. Rev. Lett 85, 4438 (2000)
Bagla, J.S., Jassal, H.K., Padmamabhan, T.: Phys. Rev. D 67, 063504 (2003)
Born, M., Infeld, Z.: Proc. R. Soc. A 144, 425 (1934)
Capozziello, S., Nojiri, S., Odintsov, S.D.: Phys. Lett. B 632, 597 (2006a)
Capozziello, S., Nojiri, S., Odintsov, S.D., Troisi, A.: Phys. Lett. B 639, 135 (2006b)
Carroll, S.M.: Living Rev. Rel. 4, 1 (2001)
Chevallier, M., Polarski, D.: Intl. J. Mod. Phys. D 10, 213 (2001)
Chiba, T., Okabe, T., Yamaguchi, M.: Phys. Rev. D 62, 023511 (2002)
Cooray, A.R., Huterer, D.: Astrophys. J. 513, L95 (1999)
Copeland, E.J., Sami, M., Tsujikawa, S.: arXiv:hep-th/0603057 (2006)
de Bernardis, P., et al.: astro-ph/0105296 (2002)
Fang, W., Lu, H.Q., Huang, Z.G., Zhang, K.F.: Intl. J. Mod. Phys. D 15, 199 (2006)
Fang, W., Lu, H.Q., Huang, Z.G.: arXiv:hep-th/0606032 (2007)
Garousi, M.R.: Nucl. Phys. B 584, 284 (2000)
Gerke, B.F., Efstathiou, G.: Mon. Not. R. Astron. Soc. 335, 33 (2002)
Gibbons, G.W.: Phys. Lett. B 537, 1 (2002)
Gibbons, G.W., Herdeiro, C.A.R.: Phys. Rev. D 63, 064006 (2001)
Guo, Z.K., Ohta, N., Zhang, Y.Z.: Phys. Rev. D 72, 023504 (2005)
Guo, Z.K., Ohta, N., Zhang, Y.Z.: Mod. Phys. Lett. A 22, 883 (2007). arXiv:astro-ph/0603109
Hannestad, S., Mortsell, E.: Phys. Rev. D 66, 063508 (2002a)
Hannestad, S., Mortsell, E.: Phys. Rev. D 66, 063508 (2002b)
Hinshaw, G., et al.: Astrophys. J. Suppl. 180, 225 (2009)
Huang, Z.G., Sun, Q.Q., Fang, W., Lu, H.Q.: Mod. Phys. Lett. A. 22, 3073 (2008). arXiv:hep-th/0612176
Jassal, H., Bagla, J., Padmanabhan, T.: astro-ph/0506748 (2005)
Kofman, L., Linde, A.: J. High Energy Phys. 0207, 004 (2002)
Li, M.: Phys. Lett. B 603, 1 (2004). arXiv:hep-th/0403127
Linder, E.V.: Phys. Rev. Lett. 90, 091301 (2003)
Lu, H.Q.: Intl. J. Mod. Phys. D 14, 355 (2005)
Melchiori, A., Mersini-Houghton, L., Odman, C.J., Trodden, M.: Phys. Rev. D 68, 043509 (2003a)
Melchiorri, A., Mersini, L., Odman, C.J., Trodden, M.: Phys. Rev. D 68, 043509 (2003b)
Nojiri, S., Odintsov, S.D., Sasaki, M.: Phys. Rev. D 70, 043539 (2004)
Nolta, M.R., et al.: Astrophys. J. Suppl. 180, 296 (2009)
Padmanabhan, T.: Phys. Reports 380, 235 (2003)
Padmanabhan, T., Choudhury, T.R.: Phys. Rev. D 66, 081301 (2002)
Padmanabhan, T., Choudhury, T.R.: Mon. Not. R. Astron. Soc. 344, 823 (2003)
Peebles, P.J.E., Ratra, B.: Rev. Mod. Phys. 75, 559 (2003)
Percival, W.J., et al.: Mon. Not. R. Astron. Soc. 337, 1068 (2002)
Piao, Y.S., Cai, R.G., Zhang, X.M., Zhang, Y.Z.: Phys. Rev. D 66, 121301 (2002)
Riess, A.G.: Astron. J. 116, 1009 (1998)
Sahni, V., Starobinsky, A.: Intl. J. Mod. Phys. D 9, 373 (2000)
Sen, A.: J. High Energy Phys. 0204, 048 (2002)
Sherrer, R.J.: Phys. Rev. Lett. 93, 011301 (2004)
Tegmark, M., et al.: Phys. Rev. D 69, 103510 (2004)
Weinberg, S.: Rev. Mod. Phys. 61, 1 (1989)
Wetterich, C.: Nucl. Phys. B 302, 668 (1998)
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Huang, Z.G., Lu, H.Q. & Fang, W. Parametrization of Born-Infeld type phantom dark energy model. Astrophys Space Sci 324, 55 (2009). https://doi.org/10.1007/s10509-009-0139-y
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DOI: https://doi.org/10.1007/s10509-009-0139-y