Abstract
We present models, in which phantom energy interacts with two different types of dark energies including variable modified Chaplygin gas (VMCG) and new modified Chaplygin gas (NMCG). We then construct potentials for these cases. It has been shown that the potential of the phantom field decreases from a higher value with the evolution of the Universe.
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Arkani-Hamed, N., et al.: J. High Energy Phys. 0405, 074 (2004)
Babichev, E., et al.: Phys. Rev. Lett. 93, 021102 (2004)
Benaoum, H.B.: hep-th/0205140 (2002)
Bento, M.C., et al.: Phys. Rev. D 66, 043507 (2002)
Bento, M.C., et al.: Phys. Rev. D 73, 043504 (2006)
Bertolami, O., et al.: Phys. Lett. B 564, 165 (2007)
Caldwell, R.R., et al.: Phys. Rev. Lett. 91, 071301 (2003)
Campo, S., et al.: Phys. Rev. D 74, 023501 (2006)
Chattopadhyay, S., Debnath, U.: Gravit. Cosmol. 14, 341 (2008)
Chattopadhyay, S., Debnath, U.: Astrophys. Space Sci. 326, 155 (2010)
Chimento, L.P., Jakubi, A.S.: Phys. Rev. D 67, 087302 (2003)
Copeland, E.J., Sami, M., Tsujikawa, T.: Int. J. Mod. Phys. D 15, 1753 (2006)
Curbelo, R., et al.: Class. Quantum Gravity 23, 1585 (2006)
Debnath, U.: Astrophys. Space Sci. 312, 295 (2007)
Debnath, U., et al.: Class. Quantum Gravity 21, 5609 (2004)
Doglov, A.D.: arXiv:hep-th/0405089 (2004)
Farooq, M.U., Jamil, M., Rashid, M.A.: Int. J. Theor. Phys. 49, 2278 (2010)
Freese, K., Lewis, M.: Phys. Lett. B 540, 1 (2002)
Freese, S., et al.: Nucl. Phys. B 287, 797 (1987)
Frieman, J., et al.: Phys. Rev. Lett. 75, 2077 (1995)
Jamil, M., Rashid, M.A.: Eur. Phys. J. C 58, 111 (2008)
Jamil, M., Rashid, M.A.: Eur. Phys. J. C 60, 141 (2009a)
Jamil, M., Farooq, M.U., Rashid, M.A.: Eur. Phys. J. C 61, 471 (2009b)
Jamil, M., Saridakis, E.N., Setare, M.R.: Phys. Lett. B 679, 172 (2009)
Jamil, M., et al.: Eur. Phys. J. C 61, 471 (2009)
Kamenshchik, A., et al.: Phys. Lett. B 511, 265 (2001)
Li, M., et al.: arXiv:0801.1407 [astro-ph]
Lima, J.A.S., Alacaniz, J.S.: Phys. Lett. B 600, 191 (2004)
Linder, E.V.: New Astron. Rev. 49, 93 (2005)
Mota, D.F.: Astron. Astrophys. 421, 71 (2004)
Nesseris, S., Perivolaropoulos, L.: Phys. Rev. D 70, 123529 (2004)
Panotopoulos, G.: Phys. Rev. D 77, 107303 (2008)
Perlmutter, S., et al.: Astrophys. J. 517, 565 (1999)
Riess, A., et al.: Astron. J. 116, 1009 (1998)
Sadjadi, H.M., Alimohammadi, M.: Phys. Rev. D 74, 103007 (2006)
Sami, M., et al.: Phys. Lett. B 619, 193 (2005)
Sen, A.: J. High Energy Phys. 0207, 065 (2002)
Setare, M.R.: Eur. Phys. J. C 50, 991 (2007a)
Setare, M.R.: Phys. Lett. B 654, 1 (2007b)
Setare, M.R.: Phys. Lett. B 653, 116 (2007c)
Setare, M.R.: Phys. Lett. B 648, 329 (2007d)
Setare, M.R.: Eur. Phys. J. C 52, 689 (2007e)
Setare, M.R., Vagenas, E.C.: arXiv:0704.2070 [hep-th]
Spergel, S., et al.: Astrophys. J. 148, 175 (2003)
Spergel, S., et al.: Astrophys. J. 170, 377 (2007)
Vikman, A.: Phys. Rev. D 71, 023515 (2005)
Wang, B., et al.: Nucl. Phys. B 778, 69 (2007)
Wei, H., Zhang, S.N.: Phys. Lett. B 654, 139 (2007)
Weinberg, S.: Phys. Rev. Lett. 59, 2607 (1987)
Wu, P., Yu, H.: Class. Quantum Gravity 24, 4661 (2007)
Zhang, X.: Commun. Theor. Phys. 44, 762 (2005)
Zhang, X., et al.: J. Cosmol. Astropart. Phys. 0601, 003 (2006a)
Zhang, X., et al.: J. Cosmol. Astropart. Phys. 0106, 003 (2006b)
Zimdahl, W., Pavon, D.: Class. Quantum Grav. 24, 5461 (2007)
Zlatev, I., et al.: Phys. Rev. Lett. 82, 896 (1999)
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Farooq, M.U., Jamil, M. & Debnath, U. Dynamics of interacting phantom and quintessence dark energies. Astrophys Space Sci 334, 243–248 (2011). https://doi.org/10.1007/s10509-011-0721-y
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DOI: https://doi.org/10.1007/s10509-011-0721-y