Invisible QCD as Dark Energy

被引:2
|
作者
Addazi, Andrea [1 ,2 ]
Alexander, Stephon [3 ]
Marciano, Antonino [4 ,5 ,6 ]
机构
[1] Sichuan Univ, Coll Phys Sci & Technol, Ctr Theoret Phys, Chengdu 610065, Peoples R China
[2] INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy
[3] Brown Univ, Dept Phys, Providence, RI 02912 USA
[4] Fudan Univ, Ctr Field Theory & Particle Phys, Shanghai 200433, Peoples R China
[5] Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China
[6] INFN, Lab Nazl Frascati, 54 Via Enrico Fermi, I-00044 Rome, Italy
关键词
dark energy; non-Abelian gauge theory; condensate; OBSERVATIONAL EVIDENCE; DYNAMICAL MODEL; ANALOGY;
D O I
10.3390/universe6060075
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We account for the late time acceleration of the Universe by extending the Quantum Chromodynamics (QCD) color to a SU(3) invisible sector (IQCD). If the Invisible Chiral symmetry is broken in the early universe, a condensate of dark pions (dpions) and dark gluons (dgluons) forms. The condensate naturally forms due to strong dynamics similar to the Nambu-Jona-Lasinio mechanism. As the Universe evolves from early times to present times the interaction energy between the dgluon and dpion condensate dominates with a negative pressure equation of state and causes late time acceleration. We conclude with a stability analysis of the coupled perturbations of the dark pions and dark gluons.
引用
收藏
页数:10
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