CONDITIONS FOR INFLATION IN AN INITIALLY INHOMOGENEOUS UNIVERSE

被引：39

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

共 15 条

[1]

Belinskii V. A., 1972, Soviet Physics - JETP, V35, P838

[2]

BELINSKII VA, 1973, ZH EKSP TEOR FIZ, V36, P591

[3] ON THE DEGRESS OF GENERALITY OF INFLATION IN FRIEDMANN COSMOLOGICAL MODELS WITH A MASSIVE SCALAR FIELD [J].

BELINSKY, VA ;

ISHIHARA, H ;

KHALATNIKOV, IM ;

SATO, H .

PROGRESS OF THEORETICAL PHYSICS, 1988, 79 (03) :676-684

[4]

BELINSKY VA, 1987, ZH EKSP TEOR FIZ, V66, P441

[5] INFLATION IN INHOMOGENEOUS COSMOLOGY [J].

CALZETTA, E ;

SAKELLARIADOU, M .

PHYSICAL REVIEW D, 1992, 45 (08) :2802-2805

[6] GROWTH OR DECAY OF COSMOLOGICAL INHOMOGENEITIES AS A FUNCTION OF THEIR EQUATION OF STATE [J].

COMER, GL ;

DERUELLE, N ;

LANGLOIS, D ;

PARRY, J .

PHYSICAL REVIEW D, 1994, 49 (06) :2759-2768

[7]

DERUELLE N, UNPUB

[8] SPHERICAL INHOMOGENEOUS COSMOLOGIES AND INFLATION - NUMERICAL-METHODS [J].

GOLDWIRTH, DS ;

PIRAN, T .

PHYSICAL REVIEW D, 1989, 40 (10) :3263-3279

[9] INHOMOGENEOUS INITIAL CONDITIONS FOR INFLATION [J].

GOLDWIRTH, DS .

PHYSICAL REVIEW D, 1991, 43 (10) :3204-3213

[10] INITIAL CONDITIONS FOR INFLATION [J].

GOLDWIRTH, DS ;

PIRAN, T .

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1992, 214 (04) :223-292

← 1 2 →