Abstract
We have studied the evolution of cosmological parameters by considering exponential harmonic field with collisional matter. A comparison has been made with the behavior of these parameters in the presence of ordinary matter and the model \(\Lambda CDM\). We have also compared the evolution of these parameters with the ones obtained in the modified gravity f(R) and f(R, T) theory case. The results are in line with those of the modified gravity so that the harmonic exponential field can be used to explain why the Universe has gone from the deceleration phase to the acceleration phase.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Ara M. 1999, Kodai Math. J., 22, 243.
Ara M. 1991, Mathematics Subject Classification, Primary 58E20.
Ara M. 1991, Mathematics Subject Classification, Primary 58E05.
Ara M. 2001, Hiroshima Math. J., 31, 171.
Aubourg E. et al. 2015, arXiv:1411.1074V3.
Baffou E. H., Houndjo M. J. S., Rodrigues M. E., Kpadonou A. V., Tossa J. 2016, arXiv:1504.05496V2 [gr-qc].
Bernal J. L., Bellomo N., Raccanelli A., Verde L. 2017, arXiv:1709.07465V2.
Bezares-Roder Nils M., Nandan H., Dehnen H. 2007, arXiv:gr-qc/0609125.
Bezares-Roder Nils M., Nandan H., Dehnen H. 2010, arXiv:0912.4039V3.
Eells J., Lemaire L. 1978, Bull. London Math. Soc., 10, 1.
Eells J., Lemaire L. 1964, Am. J. Math., 86, 109.
Fock V. 1959, The theory of space, time and gravitation, Pergamon Press, London, pp. 81–83 and 91–94.
Freese K., Lewis M. 2002, Phys. Lett., B540.
Gondolo P., Freese K. 2002, arXiv:hep-ph/0211397.
Harko T., Lobo N. S. F., Saridakis N. E., Tsoukalass M. 2016, arXiv:1609.01503V1.
Hughes T., Kato T., Marsden J. 1977, Arch. Ration. Anal., 63, 273.
Hirschman T., Schimming R. 1988, Astro. Nachr., 309, 5.
Kanfon D. A., Fuzfa A., Lambert D. 2002, J. Phys. A: Math. Gen., 35, 7629.
Kanfon D. A., Lambert D. 2012, J. Mod. Phys 3, 1727.
Kleidis K., Spyrou N. K. 2011, Astron. Astrophys., 529, A26.
Lidsey J. E., Wands D., Copeland E. J. 1998, arXiv:hep-th/9909061.
Nozari K. 2014, preprint arXiv:1306.5853v1.
Oikonomou V. K., Karagiannakis N., Park M. 2014, arXiv:1411.3199 [gr-qc].
Oikonomou V. K., Karagiannakis N. 2014, arXiv:1408.5353.
Riess A. G. et al. 1998, ApJ, 116, 1009.
Riess A. G. et al. 2004, ApJ, 607, 665.
Riess A. G. et al. 2007, ApJ, 659, 98.
Springel V., Frank C. S., White S. M. D. 2006, Nature (London), 440, 1137.
Xu Y. D., Huang Z. G. 2012, Astrophys. Space Sci., 342, 493.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Kanfon, A.D., Mavoa, F. Cosmological implications of exponential harmonic field with collisional matter. J Astrophys Astron 39, 62 (2018). https://doi.org/10.1007/s12036-018-9550-5
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s12036-018-9550-5