Cosmology with a variable generalized Chaplygin gas

被引:46
作者
Lu, Jianbo [1 ]
机构
[1] Dalian Univ Technol, Sch Phys & Optoelect Technol, Dalian 116024, Peoples R China
关键词
Variable generalized Chaplygin gas (VGCG); Unification of dark matter and dark energy; ACCELERATING UNIVERSE; CONSTRAINTS; SUPERNOVAE;
D O I
10.1016/j.physletb.2009.09.027
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate observational constraint on the variable generalized Chaplygin gas (VGCG) model as the unification of dark matter and dark energy by using the Union supernovae sample and the baryon acoustic oscillations data. Based on the best fit parameters for VGCG model it is shown that the current value of equation of state for dark energy is W-0de = -1.08 < -1, and the universe will not end up with big rip in the future. In addition, we also discuss the evolution of several quantities in VGCG cosmology such as deceleration parameter, fractional density parameters, growth index and sound speed. Finally, the statefinder diagnostic is performed to discriminate the VGCG with other models. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码:404 / 410
页数:7
相关论文
共 36 条
[11]  
GUN ZK, ARXIVASTROPH0509790
[12]   Cosmology with a variable Chaplygin gas [J].
Guo, Zong-Kuan ;
Zhang, Yuan-Zhong .
PHYSICS LETTERS B, 2007, 645 (04) :326-329
[13]   BVRI light curves for 29 type Ia supernovae [J].
Hamuy, M ;
Phillips, MM ;
Suntzeff, NB ;
Schommer, RA ;
Maza, J ;
Antezana, R ;
Wischnjewsky, M ;
Valladares, G ;
Muena, C ;
Gonzalez, LE ;
Aviles, R ;
Wells, LA ;
Smith, RC ;
Navarrete, M ;
Covarrubias, R ;
Williger, GM ;
Walker, AR ;
Layden, AC ;
Elias, JH ;
Baldwin, JA ;
Hernandez, M ;
Tirado, H ;
Ugarte, P ;
Elston, R ;
Saavedra, N ;
Barrientos, F ;
Costa, E ;
Lira, P ;
Ruiz, MT ;
Anguita, C ;
Gomez, X ;
Ortiz, P ;
DellaValle, M ;
Danziger, J ;
Storm, J ;
Kim, YC ;
Bailyn, C ;
Rubenstein, EP ;
Tucker, D ;
Cersosimo, S ;
Mendez, RA ;
Siciliano, L ;
Sherry, W ;
Chaboyer, B ;
Koopmann, RA ;
Geisler, D ;
Sarajedini, A ;
Dey, A ;
Tyson, N ;
Rich, RM .
ASTRONOMICAL JOURNAL, 1996, 112 (06) :2408-2437
[14]   An alternative to quintessence [J].
Kamenshchik, A ;
Moschella, U ;
Pasquier, V .
PHYSICS LETTERS B, 2001, 511 (2-4) :265-268
[15]  
KOMATSU E, ARXIVASTROPH08030547, P23514
[16]  
LI M, ARXIVASTROPH09040928
[17]   Constraints on accelerating universe using ESSENCE and Gold supernovae data combined with other cosmological probes [J].
Lu, Jianbo ;
Xu, Lixin ;
Liu, Molin ;
Gui, Yuanxing .
EUROPEAN PHYSICAL JOURNAL C, 2008, 58 (02) :311-324
[18]   Comparison of the legacy and gold type Ia supernovae dataset constraints on dark energy models [J].
Nesseris, S ;
Perivolaropoulos, L .
PHYSICAL REVIEW D, 2005, 72 (12)
[19]  
NESSERIS S, 2007, JCAP, V701, DOI [10.1088/1475-7516/2007/01/018, DOI 10.1088/1475-7516/2007/01/018]
[20]   Constraints on linear negative potentials in quintessence and phantom models from recent supernova data [J].
Perivolaropoulos, L .
PHYSICAL REVIEW D, 2005, 71 (06) :1-7