CONDITIONS FOR INFLATION IN AN INITIALLY INHOMOGENEOUS UNIVERSE

被引：40

作者：

DERUELLE, N

GOLDWIRTH, DS

机构：

[1] UNIV CAMBRIDGE,DEPT APPL MATH & THEORET PHYS,CAMBRIDGE CB3 9EW,ENGLAND

[2] TEL AVIV UNIV,RAYMOND & BEVERLY SACKLER FAC EXACT SCI,SCH PHYS & ASTRON,IL-69976 TEL AVIV,ISRAEL

来源：

PHYSICAL REVIEW D | 1995年 / 51卷 / 04期

关键词：

D O I：

10.1103/PhysRevD.51.1563

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using a long wavelength iteration scheme to solve Einstein's equations near the big-bang singularity of a universe driven by a massive scalar field, we find how big initial quasi-isotropic inhomogeneities can be before they can prevent inflation to set in. © 1995 The American Physical Society.

引用

页码：1563 / 1568

页数：6

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