Abstract
In this paper, we propose the non-linear Born–Infeld scalar field and canonical scalar field dark energy models with the potential \(\frac{\lambda }{4}( {\phi ^2 - \sigma ^2 })^2 + V_0\), which admits late time de Sitter attractor solution. The attractor solution corresponds to an equation of state ω_φ → − 1 and a cosmic density parameter Ω_φ → 1, which are important features for a dark energy model that can meet the current observations. dark energy; canonical scalar field, non-linear Born–Infeld type scalar field, attractor solution.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Alverson, N. W. H. et al. (2002). Astronomical Journal 568, 38.
Barreiro, T., Copeland, E. J., and Nunes, N. J. (2000). Physical Review D 61, 127301.
Bennett, C. L. et al. (2003). {astro-ph/0302207}.
Born, M. and Infeld, Z. (1934). Proceedings of the Royal Society of London, Series A 144, 425.
Caldwell, R. R. (2002). Physics Letters B 545, 23.
Caldwell, R. R., Dave, R., and Steinhardt, P. J. (1998). Physical Review Letters 80, 1582
Carroll, S. M., Hoffman, M., and Trodden, M. (2003). Physical Review D 68, 023509.
Coble, K., Dodelson, S., and Frieman, J. (1997). Physical Review D 55, 1851.
De Oliveira, H. P. (1995). Journal of Mathematical Physics 36, 2988.
Fang, W., et al. (2006). International Journal of Modern Physics D 15, 199.
Hao, J. G. and Li, X. Z. (2003a). Physical Physical D 67, 107303.
Hao, J.-G. and Li, X.-Z. (2003b). Physical Review D 68, 083514.
Heisenberg, W. (1946). Zeitschrift fur Physik 126, 519.
Heisenberg, W. (1952). Zeitschrift fur Physik 133, 79.
Lu, H. Q. (2005). International Journal of Modern Physics D 14, 355.
Netterfield, C. B. et al. (2002). Astrophysical Journal 571, 604.
Padmanabhan, T. (2003). Physics Reports 380, 235
Peebles, P. J. E. and Ratra, B. (2003). Reviews of Modern Physics 75, 559
Perlmuter, S. et al. (1999). Astrophysical Journal 517, 565.
Ratra, B. and Peebles, P. J. (1988). Physical Review D 37, 3406.
Riess, A. G. et al. (1998). Astronomical Journal 116, 1009.
Singh, P., Sami, M., and Dadhich, N. (2003). Physical Review D 68, 023522.
Taniuti, T. (1958). Progress of Theoretical Physics (kyoto) Supplement l9, 69.
Tonry, J. L. et al. (2003). astro-ph/0305008.
Zlatev, I., Wang, L., and Steinhardt, P. J. (1999). Physical Review Letters 82, 896.
Author information
Authors and Affiliations
Corresponding author
Additional information
PACS number(s):98.80.-k; 98.80.Cq; 98.80.Es.
Rights and permissions
About this article
Cite this article
Ke-Feng, Z., Wei, F. & Hui-Qing, L. Dark Energy Model with Canonical Scalar Field and Non-Linear Born–Infeld Type Scalar Field. Int J Theor Phys 45, 1296–1307 (2006). https://doi.org/10.1007/s10773-006-9147-7
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10773-006-9147-7