Inflation with holographic dark energy

Bin Chen; Miao Li; Yi Wang

doi:10.1016/j.nuclphysb.2007.04.007

Inflation with holographic dark energy

Bin Chen, Miao Li, Yi Wang^*

^*Corresponding author for this work

Research output: Contribution to journal › Journal Article › peer-review

74 Citations (Scopus)

Abstract

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.

Original language	English
Pages (from-to)	256-267
Number of pages	12
Journal	Nuclear Physics B
Volume	774
Issue number	1-3
DOIs	https://doi.org/10.1016/j.nuclphysb.2007.04.007
Publication status	Published - 9 Jul 2007
Externally published	Yes

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10.1016/j.nuclphysb.2007.04.007

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title = "Inflation with holographic dark energy",

abstract = "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.",

author = "Bin Chen and Miao Li and Yi Wang",

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AU - Li, Miao

AU - Wang, Yi

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AB - 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.

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DO - 10.1016/j.nuclphysb.2007.04.007

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SN - 0550-3213

VL - 774

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EP - 267

JO - Nuclear Physics B

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ER -

Inflation with holographic dark energy

Abstract

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