Chin. Phys. Lett.  2009, Vol. 26 Issue (10): 109803    DOI: 10.1088/0256-307X/26/10/109803
Original Articles |
A Dark Energy Model with Higher Derivative and Cosmological Evolution
ZHANG Xiao-Fei1, LIU Hui-Hui2
1Department of Physics and Electronic Science, Binzhou College, Shandong 2566002Department of Physics, Henan University of Science and Technology, Luoyang 471003
Cite this article:   
ZHANG Xiao-Fei, LIU Hui-Hui 2009 Chin. Phys. Lett. 26 109803
Download: PDF(250KB)  
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks
Abstract We construct dark energy models which have high derivative terms. In the framework of a single scalar field model with a higher derivative, the equation of state (EOS) w might have some special character in the evolvement, which states that the universe will evolve in some interesting ways. We study the different kinds of dark energy models, and classify them into several genera by their character in the evolvement.
Keywords: 98.80.-k      95.36.+x     
Received: 24 January 2009      Published: 27 September 2009
PACS:  98.80.-k (Cosmology)  
  95.36.+x (Dark energy)  
TRENDMD:   
URL:  
https://cpl.iphy.ac.cn/10.1088/0256-307X/26/10/109803       OR      https://cpl.iphy.ac.cn/Y2009/V26/I10/109803
Service
E-mail this article
E-mail Alert
RSS
Articles by authors
ZHANG Xiao-Fei
LIU Hui-Hui
Related articles from Frontiers Journals
[1] Mubasher Jamil*, D. Momeni** . Evolution of the Brans–Dicke Parameter in Generalized Chameleon Cosmology[J]. Chin. Phys. Lett., 2011, 28(9): 109803
[2] HUANG Zeng-Guang**, FANG Wei, , LU Hui-Qing, . Inflation and Singularity of a Bianchi Type-VII0 Universe with a Dirac Field in the Einstein–Cartan Theory[J]. Chin. Phys. Lett., 2011, 28(8): 109803
[3] Atul Tyagi*, Keerti Sharma . Locally Rotationally Symmetric Bianchi Type-II Magnetized String Cosmological Model with Bulk Viscous Fluid in General Relativity[J]. Chin. Phys. Lett., 2011, 28(8): 109803
[4] Hassan Amirhashchi, Anirudh Pradhan, **, Bijan Saha . An Interacting Two-Fluid Scenario for Dark Energy in an FRW Universe[J]. Chin. Phys. Lett., 2011, 28(3): 109803
[5] HUANG Zeng-Guang**, FANG Wei, LU Hui-Qing, ** . Inflation and Singularity in Einstein–Cartan Theory[J]. Chin. Phys. Lett., 2011, 28(2): 109803
[6] Abdussattar**, S. R. Prajapati** . Friedman–Robertson–Walker Models with Late-Time Acceleration[J]. Chin. Phys. Lett., 2011, 28(2): 109803
[7] CHEN Ju-Hua, **, ZHOU Sheng, WANG Yong-Jiu, . Evolution of Interacting Viscous Dark Energy Model in Einstein Cosmology[J]. Chin. Phys. Lett., 2011, 28(2): 109803
[8] Ujjal Debnath . Modified Chaplygin Gas with Variable G and Λ[J]. Chin. Phys. Lett., 2011, 28(11): 109803
[9] YANG Rong-Jia, QI Jing-Zhao, YANG Bao-Zhu . Restrictions on Purely Kinetic K-Essence[J]. Chin. Phys. Lett., 2011, 28(10): 109803
[10] Koijam Manihar Singh*, Kangujam Priyokumar Singh** . Cosmic String Universes Embedded with Viscosity[J]. Chin. Phys. Lett., 2011, 28(10): 109803
[11] Atul Tyagi, Keerti Sharma. Bianchi Type-V Magnetized String Cosmological Model with Variable Magnetic Permeability for Viscous Fluid distribution[J]. Chin. Phys. Lett., 2010, 27(8): 109803
[12] Atul Tyagi, Keerti Sharma, Payal Jain. Bianchi Type-IX String Cosmological Models for Perfect Fluid Distribution in General Relativity[J]. Chin. Phys. Lett., 2010, 27(7): 109803
[13] YANG Rong-Jia, GAO Xiang-Ting. Observational Constraints on Purely Kinetic k-Essence Dark Energy Models[J]. Chin. Phys. Lett., 2009, 26(8): 109803
[14] LIANG Nan, GAO Chang-Jun, ZHANG Shuang-Nan,. A Two-Field Dilaton Model of Dark Energy[J]. Chin. Phys. Lett., 2009, 26(6): 109803
[15] M. R. Setare. Interacting Holographic Dark Energy in the Scalar Gauss-Bonnet Gravity[J]. Chin. Phys. Lett., 2009, 26(2): 109803
Viewed
Full text


Abstract