INHOMOGENEOUS INFLATION - NUMERICAL EVOLUTION

被引：46

作者：

KURKISUONIO, H

LAGUNA, P

MATZNER, RA

机构：

[1] LAWRENCE LIVERMORE NATL LAB,LIVERMORE,CA 94550

[2] PENN STATE UNIV,DEPT ASTRON & ASTROPHYS,UNIV PK,PA 16802

[3] UNIV TEXAS,CTR RELAT,AUSTIN,TX 78712

来源：

PHYSICAL REVIEW D | 1993年 / 48卷 / 08期

关键词：

D O I：

10.1103/PhysRevD.48.3611

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe our three-dimensional numerical relativity code for the evolution of inhomogeneous cosmologies. During the evolution, the constraint equations are monitored but not solved. The code has been tested against perturbation theory with good results. We present some runs of inhomogeneous inflation with strongly inhomogeneous initial data.

引用

页码：3611 / 3624

页数：14

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