Inflation in de Sitter spacetime and CMB large scale anomaly

被引:4
|
作者
Zhao Dong [1 ]
Li Ming-Hua [2 ]
Wang Ping [1 ]
Chang Zhe [1 ]
机构
[1] Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China
[2] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou 510275, Guangdong, Peoples R China
基金
中国国家自然科学基金;
关键词
de Sitter spacetime; dark energy; inflation; anisotropy; PROBE WMAP OBSERVATIONS;
D O I
10.1088/1674-1137/39/9/095101
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The influence of cosmological constant-type dark energy in the early universe is investigated. This is accommodated by a new dispersion relation in de Sitter spacetime. We perform a global fit to explore the cosmological parameter space by using the CosmoMC package with the recently released Planck TT and WMAP polarization datasets. Using the results from the global fit, we compute a new CMB temperature temperature (TT) spectrum. The obtained TT spectrum has lower power compared with that based on the ACDM model at large scales.
引用
收藏
页数:4
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