Inflation with holographic dark energy
Inflation with holographic dark energy
复制标题
全息暗能量的暴胀
DOI：
10.1016/j.nuclphysb.2007.04.007
复制
发表时间：
2007-07-09
影响因子：
2.8
通讯作者：
Wang, Yi
中科院分区：
文献类型：
--
作者：
Chen, Bin;Li, Miao;Wang, Yi
我们研究了全息暗能量对暴胀范式的修正。我们详细研究了暴胀宇宙中全息暗能量的演化，并对全息暗能量对原始标量功率谱的修正进行了模型无关的分析。事实证明，校正通常会使光谱更红。为了与实验数据一致，再加热温度必须有一个上限。我们还讨论了不同的红外截止点所引起的校正。(c) 2007 Elsevier B.V.版权所有
We investigate the corrections of the holographic dark energy to inflation paradigm. We study the evolution of the holographic dark energy in the inflationary universe in detail, and carry out a model - independent analysis on the holographic dark energy corrections to the primordial scalar power spectrum. It turns out that the corrections generically make the spectrum redder. To be consistent with the experimental data, there must be a upper bound on the reheating temperature. We also discuss the corrections due to different choices of the infrared cutoff. (c) 2007 Elsevier B.V. All rights reserved.