Generalized Ghost Pilgrim Scalar Field Models of Dark Energy

被引:18
作者
Jawad, Abdul [1 ]
Debnath, Ujjal [2 ]
Batool, Fazal [3 ]
机构
[1] COMSATS Inst Informat Technol, Dept Math, Lahore 54000, Pakistan
[2] Indian Inst Engn Sci & Technol, Dept Math, Sibpur 711103, Howrah, India
[3] Lahore Leads Univ, Dept Math, Lahore 54590, Pakistan
关键词
generalized ghost Pilgrim dark energy; scalar field models; PROBE WMAP OBSERVATIONS; COSMOLOGICAL CONSTANT; CONSEQUENCES; EVOLUTION; RELEASE; LAMBDA;
D O I
10.1088/0253-6102/64/5/590
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We assume generalized ghost Pilgrim dark energy (GGPDE) model in the presence of cold dark matter in flat FRW universe. With suitable choice of interaction term between GGPDE and cold dark matter, we investigate the nature of equation of state parameter for GGPDE. Also, we investigate the natures of dynamical scalar field models (such as quintessence, tachyon, k-essence, and dilaton dark energy) and concerned potentials through the correspondence phenomenon between GGPDE and these models.
引用
收藏
页码:590 / 596
页数:7
相关论文
共 50 条
[1]   The second data release of the Sloan Digital Sky Survey [J].
Abazajian, K ;
Adelman-McCarthy, JK ;
Agüeros, MA ;
Allam, SS ;
Kurt ;
Anderson, SJ ;
Anderson, SF ;
Annis, J ;
Bahcall, NA ;
Baldry, IK ;
Bastian, S ;
Berlind, A ;
Bernardi, M ;
Blanton, MR ;
Bochanski, JJ ;
Boroski, WN ;
Briggs, JW ;
Brinkmann, J ;
Brunner, RJ ;
Budavári, T ;
Carey, LN ;
Carliles, S ;
Castander, FJ ;
Connolly, AJ ;
Csabai, I ;
Doi, M ;
Dong, F ;
Eisenstein, DJ ;
Evans, ML ;
Fan, XH ;
Finkbeiner, DP ;
Friedman, SD ;
Frieman, JA ;
Fukugita, M ;
Gal, RR ;
Gillespie, B ;
Glazebrook, K ;
Gray, J ;
Grebel, EK ;
Gunn, JE ;
Gurbani, VK ;
Hall, PB ;
Hamabe, M ;
Harris, FH ;
Harris, HC ;
Harvanek, M ;
Heckman, TM ;
Hendry, JS ;
Hennessy, GS ;
Hindsley, RB .
ASTRONOMICAL JOURNAL, 2004, 128 (01) :502-512
[2]   The third data release of the Sloan digital Sky Survey [J].
Abazajian, K ;
Adelman-McCarthy, JK ;
Agüeros, MA ;
Allam, SS ;
Anderson, KSJ ;
Anderson, SF ;
Annis, J ;
Bahcall, NA ;
Baldry, IK ;
Bastian, S ;
Berlind, A ;
Bernardi, M ;
Blanton, MR ;
Bochanski, JJ ;
Boroski, WN ;
Brewington, HJ ;
Briggs, JW ;
Brinkmann, J ;
Brunner, RJ ;
Budavári, T ;
Carey, LN ;
Castander, FJ ;
Connolly, AJ ;
Covey, KR ;
Csabai, I ;
Dalcanton, JJ ;
Doi, M ;
Dong, F ;
Eisenstein, DJ ;
Evans, ML ;
Fan, XH ;
Finkbeiner, DP ;
Friedman, SD ;
Frieman, JA ;
Fukugita, M ;
Gillespie, B ;
Glazebrook, K ;
Gray, J ;
Grebel, EK ;
Gunn, JE ;
Gurbani, VK ;
Hall, PB ;
Hamabe, M ;
Harbeck, D ;
Harris, FH ;
Harris, HC ;
Harvanek, M ;
Hawley, SL ;
Hayes, J ;
Heckman, TM .
ASTRONOMICAL JOURNAL, 2005, 129 (03) :1755-1759
[3]   Dynamical solution to the problem of a small cosmological constant and late-time cosmic acceleration [J].
Armendariz-Picon, C ;
Mukhanov, V ;
Steinhardt, PJ .
PHYSICAL REVIEW LETTERS, 2000, 85 (21) :4438-4441
[4]   k-Inflation [J].
Armendáriz-Picón, C ;
Damour, T ;
Mukhanov, V .
PHYSICS LETTERS B, 1999, 458 (2-3) :209-218
[5]  
Armendariz-Picon C, 2001, PHYS REV D, V63, DOI 10.1103/PhysRevD.63.103510
[6]   More on QCD ghost dark energy [J].
Cai, Rong-Gen ;
Tuo, Zhong-Liang ;
Wu, Ya-Bo ;
Zhao, Yue-Yue .
PHYSICAL REVIEW D, 2012, 86 (02)
[7]   Notes on ghost dark energy [J].
Cai, Rong-Gen ;
Tuo, Zhong-Liang ;
Zhang, Hong-Bo ;
Su, Qiping .
PHYSICAL REVIEW D, 2011, 84 (12)
[8]   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
[9]   Correspondence Between Ricci and Other Dark Energies [J].
Chattopadhyay, Surajit ;
Debnath, Ujjal .
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2011, 50 (02) :315-324
[10]   Kinetically driven quintessence [J].
Chiba, T ;
Okabe, T ;
Yamaguchi, M .
PHYSICAL REVIEW D, 2000, 62 (02) :8