Dynamics of coupled phantom and tachyon fields

被引:40
作者
Shahalam, M. [1 ]
Pathak, S. D. [2 ]
Li, Shiyuan [2 ]
Myrzakulov, R. [3 ]
Wang, Anzhong [1 ,4 ]
机构
[1] Zhejiang Univ Technol, Inst Adv Phys & Math, Hangzhou, Zhejiang, Peoples R China
[2] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China
[3] Eurasian Natl Univ, Dept Gen & Theoret Phys, Eurasian Int Ctr Theoret Phys, Astana, Kazakhstan
[4] Baylor Univ, Dept Phys, GCAP CASPER, Waco, TX 76798 USA
来源
EUROPEAN PHYSICAL JOURNAL C | 2017年 / 77卷 / 10期
关键词
PROBE WMAP OBSERVATIONS; COLD DARK-MATTER; COSMOLOGICAL CONSTANT; ACCELERATING UNIVERSE; ENERGY; CONSEQUENCES; QUINTESSENCE; EVOLUTION; EQUATION; LAMBDA;
D O I
10.1140/epjc/s10052-017-5255-1
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this paper, weapply the dynamical analysis to a coupled phantom field with scaling potential taking particular forms of the coupling (linear and combination of linear), and present phase space analysis. We investigate if there exists a late time accelerated scaling attractor that has the ratio of dark energy and dark matter densities of the order one. We observe that the scrutinized couplings cannot alleviate the coincidence problem, however, they acquire stable late time accelerated solutions. We also discuss a coupled tachyon field with inverse square potential assuming linear coupling.
引用
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页数:12
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共 100 条
[61]   The cosmological constant and dark energy [J].
Peebles, PJE ;
Ratra, B .
REVIEWS OF MODERN PHYSICS, 2003, 75 (02) :559-606
[62]  
Percival I., 1999, INTRO DYNAMICS
[63]   Measurements of Ω and Λ from 42 high-redshift supernovae [J].
Perlmutter, S ;
Aldering, G ;
Goldhaber, G ;
Knop, RA ;
Nugent, P ;
Castro, PG ;
Deustua, S ;
Fabbro, S ;
Goobar, A ;
Groom, DE ;
Hook, IM ;
Kim, AG ;
Kim, MY ;
Lee, JC ;
Nunes, NJ ;
Pain, R ;
Pennypacker, CR ;
Quimby, R ;
Lidman, C ;
Ellis, RS ;
Irwin, M ;
McMahon, RG ;
Ruiz-Lapuente, P ;
Walton, N ;
Schaefer, B ;
Boyle, BJ ;
Filippenko, AV ;
Matheson, T ;
Fruchter, AS ;
Panagia, N ;
Newberg, HJM ;
Couch, WJ .
ASTROPHYSICAL JOURNAL, 1999, 517 (02) :565-586
[64]   ON THE INITIAL CONDITIONS FOR SUPER-EXPONENTIAL INFLATION [J].
POLLOCK, MD .
PHYSICS LETTERS B, 1988, 215 (04) :635-641
[65]  
Rasanen S., 2004, ASTROPART PHYS, V0402
[66]   COSMOLOGICAL CONSEQUENCES OF A ROLLING HOMOGENEOUS SCALAR FIELD [J].
RATRA, B ;
PEEBLES, PJE .
PHYSICAL REVIEW D, 1988, 37 (12) :3406-3427
[67]   Phenomenology of Λ-CDM Model: A Possibility of Accelerating Universe with Positive Pressure [J].
Ray, Saibal ;
Khlopov, Maxim ;
Ghosh, Partha Pratim ;
Mukhopadhyay, Utpal .
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2011, 50 (03) :939-951
[68]   Observational evidence from supernovae for an accelerating universe and a cosmological constant [J].
Riess, AG ;
Filippenko, AV ;
Challis, P ;
Clocchiatti, A ;
Diercks, A ;
Garnavich, PM ;
Gilliland, RL ;
Hogan, CJ ;
Jha, S ;
Kirshner, RP ;
Leibundgut, B ;
Phillips, MM ;
Reiss, D ;
Schmidt, BP ;
Schommer, RA ;
Smith, RC ;
Spyromilio, J ;
Stubbs, C ;
Suntzeff, NB ;
Tonry, J .
ASTRONOMICAL JOURNAL, 1998, 116 (03) :1009-1038
[69]   Interacting ghost dark energy models in the higher dimensional cosmology [J].
Sadeghi, J. ;
Khurshudyan, M. ;
Farahani, H. .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2016, 25 (14)
[70]   The case for a positive cosmological Λ-term [J].
Sahni, V ;
Starobinsky, A .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2000, 9 (04) :373-443