Translational invariance and the anisotropy of the cosmic microwave background

被引:35
作者
Carroll, Sean M. [1 ]
Tseng, Chien-Yao [1 ]
Wise, Mark B. [1 ]
机构
[1] CALTECH, Pasadena, CA 91125 USA
来源
PHYSICAL REVIEW D | 2010年 / 81卷 / 08期
关键词
INFLATIONARY UNIVERSE SCENARIO; ANGULAR POWER SPECTRUM; TEMPERATURE ANISOTROPY; MOSAIC OBSERVATIONS; ISOTROPY; PERTURBATIONS; FLUCTUATIONS; PROPAGATION; COSMOLOGY; FLATNESS;
D O I
10.1103/PhysRevD.81.083501
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Primordial quantum fluctuations produced by inflation are conventionally assumed to be statistically homogeneous, a consequence of translational invariance. In this paper we quantify the potentially observable effects of a small violation of translational invariance during inflation, as characterized by the presence of a preferred point, line, or plane. We explore the imprint such a violation would leave on the cosmic microwave background anisotropy, and provide explicit formulas for the expected amplitudes < a(lm)a(l'm')*> of the spherical-harmonic coefficients.
引用
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页数:11
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