PLAUSIBLE DOUBLE INFLATION

被引：54

作者：

HOLMAN, R

KOLB, EW

VADAS, SL

WANG, Y

机构：

[1] UNIV CHICAGO,ENRICO FERMI INST,CHICAGO,IL 60637

[2] FERMI NATL ACCELERATOR LAB,NASA FERMILAB ASTROPHYS CTR,BATAVIA,IL 60510

[3] UNIV CHICAGO,DEPT ASTRON & ASTROPHYS,CHICAGO,IL 60637

[4] UNIV CHICAGO,DEPT PHYS,CHICAGO,IL 60637

来源：

PHYSICS LETTERS B | 1991年 / 269卷 / 3-4期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1016/0370-2693(91)90165-M

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It is likely that extended inflation is followed by an epoch of slowroll inflation. Such a sequence of events may lead to a very interesting perturbation spectrum with significant power on the scale of the transition between the extended and slowroll phase, superimposed upon a power-law spectrum with deviations from the Harrison-Zel'dovich slope. Normalization of the spectra above and below the transition scale is expected to differ.

引用

页码：252 / 256

页数：5

共 20 条

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