MAGNETO-HYDRODYNAMIC PERTURBATIONS OF ROBERTSON-WALKER UNIVERSES AND OF ANISOTROPIC BIANCHI TYPE-I UNIVERSES

被引：6

作者：

FENNELLY, AJ

EVANS, CR

机构：

[1] NASA,GEORGE C MARSHALL SPACE FLIGHT CTR,SPACE SCI LAB,NRC,HUNTSVILLE,AL 35812

[2] UNIV TEXAS,DEPT PHYS,AUSTIN,TX 78712

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS | 1980年 / 60卷 / 01期

关键词：

D O I：

10.1007/BF02723065

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

引用

页码：1 / 45

页数：45

共 91 条

[31] PERTURBATIONS OF AN EXPANDING UNIVERSE [J].

HAWKING, SW .

[32]

Heckmann O., 1959, HDB PHYS, V53, P489, DOI [10.1007/978-3-642-459, DOI 10.1007/978-3-642-459]

[33]

HOLT EH, 1965, F PLASMA DYNAMICS

[34] ORIGIN OF MICROWAVE BACKGROUND [J].

HOYLE, F .

[35] COSMOLOGIES OF BIANCHI TYPE I WITH A UNIFORM MAGNETIC FIELD [J].

JACOBS, KC .

[36] COSMIC TURBULENCE AND ORIGIN OF GALAXIES [J].

JONES, BJT .

[37] TILTED HOMOGENEOUS COSMOLOGICAL MODELS [J].

KING, AR ;

ELLIS, GFR .

[38]

KURSKOV AA, 1978, ASTROPHYS SPACE SCI, V56, P67, DOI 10.1007/BF00643461

[39]

Lichnerowicz A., 1967, RELATIVISTIC HYDRODY

[40]

Longair M S, 1973, CARGESE LECTURES PHY, V6, P269