Generating the curvature perturbation at the end of inflation

被引：166

作者：

Lyth, DH ^{[1
]}

机构：

[1] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2005年 / 11期

关键词：

CMBR theory; cosmological perturbation theory; inflation; physics of the early universe;

D O I：

10.1088/1475/7516/2005/11/006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The dominant contribution to the primordial curvature perturbation may be generated at the end of inflation. Taking the end of inflation to be sudden, formulae are presented for the spectrum, spectral tilt and non-Gaussianity. They are evaluated for a minimal extension of the original hybrid inflation model.

引用

页数：10

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