https://doi.org/10.1140/epjc/s10052-014-3080-3
Regular Article - Theoretical Physics
New holographic reconstruction of scalar-field dark-energy models in the framework of chameleon Brans–Dicke cosmology
1
Pailan College of Management and Technology, Bengal Pailan Park, Kolkata, 700 104, India
2
Department of Physics, University of Trieste, Via Valerio, 2, 34127, Trieste, Italy
3
Department of Theoretical Physics, Yerevan State University, 1 A. Manookian, Yerevan, Armenia
4
Max Planck Institute of Colloids and Interfaces, Potsdam-Golm Science Park, Am Mühlenberg 1 OT Golm, 14476, Potsdam, Germany
* e-mail: surajcha@iucaa.ernet.in
** e-mail: surajitchatto@outlook.com
Received:
12
June
2014
Accepted:
16
September
2014
Published online:
27
September
2014
Motivated by the work of Yang et al. (Mod. Phys. Lett. A 26:191, 2011), we report on a study of the new holographic dark energy (NHDE) model with energy density given by 
in the framework of chameleon Brans–Dicke cosmology. We have studied the correspondence between the quintessence, the DBI-essence, and the tachyon scalar-field models with the NHDE model in the framework of chameleon Brans–Dicke cosmology. Deriving an expression of the Hubble parameter 
and, accordingly, 
in the context of chameleon Brans–Dicke chameleon cosmology, we have reconstructed the potentials and dynamics for these scalar-field models. Furthermore, we have examined the stability for the obtained solutions of the crossing of the phantom divide under a quantum correction of massless conformally invariant fields, and we have seen that the quantum correction could be small when the phantom crossing occurs and the obtained solutions of the phantom crossing could be stable under the quantum correction. It has also been noted that the potential increases as the matter–chameleon coupling gets stronger with the evolution of the universe.
© SIF and Springer-Verlag Berlin Heidelberg, 2014
