Chamelionic generalized Brans-Dicke cosmology

被引:0
作者
R. A. El-nabulsi
机构
[1] Key Laboratory of Numerical Simulation of Sichuan Province,College of Mathematics and Information Science
[2] Neijiang Normal University,undefined
来源
The European Physical Journal Plus | / 127卷
关键词
Vertical Axis; Dark Energy; Deceleration Parameter; Weak Energy Condition; Phantom Energy;
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摘要
We discuss the late-time dynamics of a chameleonic generalized Brans-Dicke cosmology with the power law chameleonic function f (φ) ∝ φn, where n is a real parameter motivated from string theories by conjecturing that the four-dimensional Hubble parameter varies with a scale factor like φ = ξam, where (ξ, m) are real parameters. For some critical values of m, n and the Brans-Dicke parameter, it was observed that the universe is free from the initial singularity. Both singularity-free and singular cosmological scenarios are discussed. Several cosmological tests like the physical cosmological distances and the statefinder parameters are discussed.
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[1]  
Sahni V.(2004)undefined Lect. Notes Phys. 653 141-undefined
[2]  
Sahni V.(2000)undefined PRAMANA J. Phys. 55 43-undefined
[3]  
Sahni V.(2002)undefined Class. Quantum Grav. 19 3435-undefined
[4]  
Riess A.G.(1998)undefined Astron. J. 116 1009-undefined
[5]  
Perlmutter S.(1999)undefined Astrophys. J. 517 565-undefined
[6]  
de Bernardis P.(2000)undefined Nature 377 600-undefined
[7]  
Alcaniz J.S.(2004)undefined Phys. Rev. D 69 083521-undefined
[8]  
Caldwell R.(2003)undefined Phys. Rev. Lett. 91 071301-undefined
[9]  
Kamionkowski M.(1999)undefined Phys. Lett. B 468 45-undefined
[10]  
Weinberg N.(2002)undefined Phys. Rev. D 66 063514-undefined