Abstract
In this work we have proposed a non-canonical model of exponential harmonic field as dark energy in FRW universe. In this context, we have studied the inflationnary parameters in presence of power law potential. The analysis showed that observational data have been confirmed for quadratic and cubic potentials. In addition, deceleration parameter have been examined by associating to that dark energy, gas of Chaplygin as dark matter; three types of parametrisation have been considered in this case. The behaviors of deceleration parameter show transition from positive values to negative values, which would show that recent accelerated phase of the universe was preceded by a deceleration phase.
Similar content being viewed by others
References
Abazajian, M., et al. 2004, Astron. J. 128, 502
Adelman-McCarthy, J. K., et al. 2008, Astrophys. J. Suppl. Ser. 175, 297
Allen, S. W., et al. 2004, Mon. Not. Roy. Astron. Soc. 353, 457
Armendariz-Picon, C., Damour, T., Mukhanov, V. 1999, Phys. Lett. B 458, 209
Armendariz-Picon, C., Lim, E. A. 2005, JCAP 0508, 007
Astier, P., et al. 2006, Astron. Astrophys. 447, 31
Barboza, E. M., Alcaniz, J. S. 2008, Phys. Lett. B 666, 415
Bennett, C. L., et al. 2003, Astrophys. J. Supp. Ser. 148, 1
Bertacca, D., Matarrese, S., Pietroni, M. 2007, Mod. Phys. Lett. A 22, 2893
Bertacca, D., Bartolo, N. Matarrese, S. 2008, JCAP 0805, 005
Bilic, N, Tupper, G. B., Viollier, R. D. 2002, Phys. Lett. B 535, 17
Bose, N., Majumdar, A. S. 2009, Phys. Rev. D 80, 103508
Cai, Y. F, Saridakis, E. N., Setare M. R., Xia, J. Q. 2010, Phys. Rept. 493, 1
Caldwell, R. R. 2002, Phys. Lett. B 545, 23
Campo, S., Herrera, R., Toloza, A. 2009, Phys. Rev. D 79, 083507
Chevallier, M. Polarski, D. 2001, Int. J. Mod. Phys. D 10, 213
Chiba, T., Okabe, T., Yamaguchi, M. 2000, Phys. Rev. D 62, 023511
Chimento, L. P. 2004, Phys. Rev. D 69, 123517
Choudhury, S. et al. 2016, [arXiv:1511.05734]
De-Santiago, J., Cervantes-Cota, J. L. 2011, Phys. Rev. D 83, 063502
Dutta, S., Saridakis, E. N., Scherrer, R. J. 2009, Phys. Rev. D 79, 103005
Fairbairn, M., Tytgat, M. H. G. 2002, Phys. Lett. B 546, 1
Garriga, J., Mukhanov, V. F. 1999, Phys. Lett. B 458, 219
Gupta, G., Saridakis, E. N., Sen, A. A. 2009, Phys. Rev. D 79, 123013
Guo, Z. K. , Piao, Y. S., Zhang, X. M., Zhang, Y. Z. 2005, Phys. Lett. B 608, 177
Huey, G., et al. 2001 [arXiv:astro-ph/0104006]
Huterer, D., Turner, M. S. 1999, Phys. Rev. D 60, 081301
Jassal, H. K., Bagla J. S., Padmanabhan, T., 2005, Mon. Not. Roy. Astron. Soc. 356, L11
Johri, V. B. 2004, arXiv:astro-ph/0409161
Kanfon, D. A., Fuzfa, A. & Lambert, D. 2002, J. Phys. A: Math. Gen. 35, 7629–7639
Kanfon, D. A., Mavoa, F. 2018, J. Astrophys. Astro, 39, 62
Komatsu, E., et al. 2009, Astrophys. J. Suppl. 180, 330
Linder, E. V., 2003, Phys. Rev. Lett. 90, 091301
Maartens, R. et al., 2000 [arXiv:hep-th/9912464]
Magana J., et al. 2014, JCAP 017, 1410
Mamon, A. A., et al., 2015 [arXiv:1503.06280]
Mukhanov, V., Vikman, A. 2006, JCAP 0602, 004
Olivares, G., et al. 2008, Phys. Rev. D 77, 063513
Padmanabhan, T. 2003, Phys. Rep. 380, 235
Ade, P. A. R, et al. 2014, Astron. Astrophys. 571, A16
Perlmutter, S., et al. 1999, Astrophys. J. 517, 565
Peebles, P. J. E., Ratra, B. 2003, Rev. Mod. Phys. 75, 559
Ratra, B., Peebles, P. J. E. , 1988, Phys. Rev. D 37, 3406
Riess, A. G. et al. 1998, Astron. J. 116, 1009
Scherrer, R. J. 2004, Phys. Rev. Lett. 93, 011301
Seljak, U. et al. 2005, Phys. Rev. D 71, 103515
Sen, A. 2005, Phys. Scripta, T117, 70
Spergel, D. N., et al. 2003, Astrophys. J. Suppl. Ser. 148, 175
Steer, D. A., Vernizzi, F. 2004, Phys. Rev. D 70, 043527
Steinhardt, P. J. et al., 1999 Phys. Rev. Lett., 59, 123504
Sudipta, D. et al. 2018 [arXiv:1805.07148]
Tegmark, M. et al. 2004, Phys. Rev. D 69, 103501
Unnikrishnan, S. et al. 2012, JCAP 1208 018
Unnikrishnan, S. et al. 2008, Phys. Rev. D 78, 063007
Zimdahl, W. 2011, arXiv:1204.5892
Zimdahl, W. et al. 2003, arXiv:astro-ph/0404122
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Kanfon, A.D., Mavoa, F. Parameterization of non-canonical model of the exponential harmonic field. J Astrophys Astron 40, 18 (2019). https://doi.org/10.1007/s12036-019-9580-7
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s12036-019-9580-7