Abstract
We propose in this paper an interacting holographic dark energy (IHDE) model in chameleon–tachyon cosmology by interaction between the components of the dark sectors. In the formalism, the interaction term emerges from the scalar field coupling matter Lagrangian in the model rather than being inserted into the formalism as an external source for the interaction. The correspondence between the tachyon field and the holographic dark energy (HDE) densities allows to reconstruct the tachyon scalar field and its potential in a flat FRW universe. The model can show the accelerated expansion of the universe and satisfies the observational data.
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References
Amanullah, R., et al.: Astrophys. J. 716, 712–738 (2010)
Bagla, J.S., Jassal, H.K., Padmanabhan, T.: Phys. Rev. D 67, 063504 (2003)
Cohen, A.G., Kaplan, D.B., Nelson, A.E.: Phys. Rev. Lett. 82, 4971 (1999)
Copeland, E.J., Garousi, M.R., Sami, M., Tsujikawa, S.: Phys. Rev. D 71, 043003 (2005)
Farajollahi, H., Ravanpak, A., Fadakar, G.F.: Mod. Phys. Lett. A 26(15), 1125–1135 (2011a)
Farajollahi, H., Salehi, A., Tayebi, F., Ravanpak, A.: J. Cosmol. Astropart. Phys. 05, 017 (2011b)
Granda, L.N.: Int. J. Mod. Phys. D 18, 1749–1764 (2009)
Hsu, S.D.H.: Phys. Lett. B 594, 13 (2004)
Mohseni Sadjadi, H.: J. Cosmol. Astropart. Phys. 0702, 026 (2007)
Myung, Y.S.: Phys. Lett. B 610, 18 (2005)
Riess, A.G., et al.: J. Astron. 116, 1009 (1998)
Sahni, V., Starobinsky, A.A.: Int. J. Mod. Phys. D 9, 373 (2000)
Sandro Micheletti, M.R.: J. Cosmol. Astropart. Phys. 1005, 009 (2010)
Setare, M.R.: Phys. Lett. B 642, 421–425 (2006b)
Setare, M.R.: Phys. Lett. B 642, 1–4 (2006a)
Setare, M.R.: Phys. Lett. B 653, 116–121 (2007a)
Setare, M.R.: J. Cosmol. Astropart. Phys. 0701, 023 (2007b)
Setare, M.R., Vagenas Elias, C.: Int. J. Mod. Phys. D 18, 147–157 (2009)
Susskind, L.: J. Math. Phys. 36, 6377 (1995)
Wang, B., Gong, Y.G., Abdalla, E.: Phys. Lett. B 624, 141 (2005)
Wu, Q., Gong, Y., Wang, A., Alcaniz, J.S.: Phys. Lett. B 659, 34 (2008)
Zhang, X.: Int. J. Mod. Phys. D 14, 1597 (2005)
Zhang, X.: Phys. Lett. B 648, 1 (2007)
Zhang, X., Wu, F.Q.: Phys. Rev. D 72, 043524 (2005)
Zhang, J., Zhang, X., Liu, H.: Phys. Lett. B 651, 84 (2007)
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Farajollahi, H., Ravanpak, A. & Fadakar, G.F. Holographic dark energy in chameleon tachyon cosmology. Astrophys Space Sci 336, 461–467 (2011). https://doi.org/10.1007/s10509-011-0779-6
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DOI: https://doi.org/10.1007/s10509-011-0779-6