The ω =-1 crossing of the quintom model with slowly-varying potentials

被引:28
作者
Alimohammadi, M. [1 ]
Sadjadi, H. Mohseni [1 ]
机构
[1] Univ Tehran, Dept Phys, N Karegar Ave, Tehran, Iran
关键词
D O I
10.1016/j.physletb.2007.03.014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Considering the quintom model with arbitrary potential, it is shown that there always exists a solution which evolves from omega > -1 region to omega < -1 region. The problem is restricted to the slowly varying potentials, i.e. the slow-roll approximation. It is seen that the rate of this phase transition only depends on the energy density of matter at transition time, which itself is equal to the kinetic part of quintom energy density at that time. The perturbative solutions of the fields are also obtained. (C) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:113 / 118
页数:6
相关论文
共 43 条
[1]   Attractor solutions for general hessence dark energy [J].
Alimohammadi, M ;
Sadjadi, HM .
PHYSICAL REVIEW D, 2006, 73 (08)
[2]   Crossing w=-1 in Gauss-Bonnet brane world with induced gravity [J].
Cai, RG ;
Zhang, HS ;
Wang, AZ .
COMMUNICATIONS IN THEORETICAL PHYSICS, 2005, 44 (05) :948-954
[3]   A phantom menace? Cosmological consequences of a dark energy component with super-negative equation of state [J].
Caldwell, RR .
PHYSICS LETTERS B, 2002, 545 (1-2) :23-29
[4]   Phantom energy:: Dark energy with w&lt;-1 causes a cosmic doomsday -: art. no. 071301 [J].
Caldwell, RR ;
Kamionkowski, M ;
Weinberg, NN .
PHYSICAL REVIEW LETTERS, 2003, 91 (07)
[5]   Cosmological imprint of an energy component with general equation of state [J].
Caldwell, RR ;
Dave, R ;
Steinhardt, PJ .
PHYSICAL REVIEW LETTERS, 1998, 80 (08) :1582-1585
[6]   The Cosmological Constant [J].
Carroll S.M. .
Living Reviews in Relativity, 2001, 4 (1)
[7]   Can the dark energy equation-of-state parameter w be less than-1? -: art. no. 023509 [J].
Carroll, SM ;
Hoffman, M ;
Trodden, M .
PHYSICAL REVIEW D, 2003, 68 (02)
[8]   The phantom menaced: Constraints on low-energy effective ghosts [J].
Cline, JM ;
Jeon, S ;
Moore, GD .
PHYSICAL REVIEW D, 2004, 70 (04) :4
[9]   Loop corrections to scalar quintessence potentials -: art. no. 043519 [J].
Doran, M ;
Jäckel, J .
PHYSICAL REVIEW D, 2002, 66 (04)
[10]   Late-time cosmology in a (phantom) scalar-tensor theory: Dark energy and the cosmic speed-up [J].
Elizalde, E ;
Nojiri, S ;
Odintsov, SD .
PHYSICAL REVIEW D, 2004, 70 (04) :20