Second order general slow-roll power spectrum

被引:78
作者
Choe, J [1 ]
Gong, JO
Stewart, ED
机构
[1] Korea Adv Inst Sci & Technol, Dept Phys, Taejon 305701, South Korea
[2] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 606, Japan
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2004年 / 07期
关键词
cosmological perturbation theory; inflation; physics of the early universe;
D O I
10.1088/1475-7516/2004/07/012
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent combined results from the Wilkinson microwave anisotropy probe (WMAP) and Sloan digital sky survey (SDSS) provide a remarkable set of data which requires more accurate and general investigation. Here we derive formulae for the power spectrum P(k) of the density perturbations produced during inflation in the general slow-roll approximation with second order corrections. Also, using the result, we derive the power spectrum in the standard slow-roll picture with previously unknown third order corrections.
引用
收藏
页码:225 / 235
页数:11
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