Cosmic microwave background dipole induced by double inflation

被引:19
作者
Langlois, D [1 ]
机构
[1] HEBREW UNIV JERUSALEM,RACAH INST PHYS,IL-91904 JERUSALEM,ISRAEL
来源
PHYSICAL REVIEW D | 1996年 / 54卷 / 04期
关键词
D O I
10.1103/PhysRevD.54.2447
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The observed CMBR dipole is generally interpreted as the consequence of the peculiar motion of the Sun with respect to the reference frame of the CMBR. This article proposes an alternative interpretation in which the observed dipole is the result of isocurvature perturbations on scales larger than the present Hubble radius. These perturbations are produced in the simplest model of double inflation, depending on three parameters. The observed dipole and quadrupole can be explained in this model, while severely constraining its parameters.
引用
收藏
页码:2447 / 2450
页数:4
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