2008, Vol. 25(2): 798-801    DOI:
Dynamical Evolution of Modified Chaplygin Gas
FU Ming-Hui，WU Ya-Bo, HE Jing
Department of Physics, Liaoning Normal University, Dalian 116029
收稿日期 2007-09-02  修回日期 1900-01-01
Supporting info

[1] Riess A G et al 1998 Astron. J. 116 1009

[2] Bennett C L et al 2003 Astrophys. J. Suppl.
148 1

[3] Tegmark M et al 2004 Phys. Rev. D 69 103501


[4] Wood-Vasey W M et al 2007 Astrophys. J. 82
v1


[5] Upadhye A et al 2005 Phys. Rev. D 72 063501


[6] Wu Y B et al 2007 Mod. Phys. Lett. A 22 783


[7] Wu Y B et al 2007 Gen. Relat. and Grav. 39
653

[8] Wei H and Zhang $S$ N 2007 Phys. Lett. B 644
7
[9] Riess A G et al 2004 Astrophys. J. 607 665

[10] Akaike H 1974 IEEE Trans. Auto. Control 19
716

[11] Schwarz G 1978 Ann. Statist. 5 461

[12] Zimdahl W, Pavon D and Chimento L P 2001 Phys. Lett.
B 521 133


[13] Liddle A R and Lyth D H 2000 Cosmological Inflation
and Large-Scale Structure (London: Cambridge University Press) chap
4 p 80

[14] Sen A A, Cardone V F, Capozziello $S$ and Troisi A
astro-ph/0511313

[15] Lahav O et al 2002 Mon. Not. Roy. Astron. Soc.
333 961

[16] Verde L, Kamionkowski M, Mohr J J and Benson A J 2001
Mon. Not. Roy. Astron. Soc. 321 L7

[17] Silveira V and Waga I 1994 Phys. Rev. D 50
4890

[18] Wang L and Steinhardt P J 1998 Astrophys. J.
508 483