A NATURAL APPROACH TO SOME COSMOLOGICAL PROBLEMS

被引：8

作者：

OVRUT, BA

THOMAS, S

机构：

[1] Department of Physics, University of Pennsylvania, Philadelphia

来源：

PHYSICS LETTERS B | 1992年 / 277卷 / 1-2期

关键词：

D O I：

10.1016/0370-2693(92)90956-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It is shown that the cosine potential energy naturally induced in theories with an antisymmetric rank two tensor field, provides a framework for understanding both inflationary cosmology and large scale structure. A new scenario for producing large scale structure, based on the late time effect of the Hawking temperature during inflation, is also proposed.

引用

页码：53 / 57

页数：5

共 22 条

[1]

FREESE K, 1990, FERMILABPUB90177A PR

[2]

FROLICH J, 1975, P NATO ADV STUDY I

[3] ACTION INTEGRALS AND PARTITION-FUNCTIONS IN QUANTUM GRAVITY [J].

GIBBONS, GW ;

HAWKING, SW .

PHYSICAL REVIEW D, 1977, 15 (10) :2752-2756

[4]

Goncharov A. S., 1987, Soviet Physics - JETP, V65, P635

[5] LIMITS ON INFLATIONARY MODELS OF THE UNIVERSE [J].

HAWKING, SW .

PHYSICS LETTERS B, 1985, 150 (05) :339-341

[6]

Hill C. T., 1989, Comments on Nuclear and Particle Physics, V19, P25

[7]

KOLB EW, 1990, EARLY UNIVERSE

[8]

LALAK Z, 1991, UPR0474T U PENNS PRE

[9]

LINDE A, 1990, PARTICLE PHYSICS INF

[10] AXIONIC DOMAIN-WALL PRODUCTION DURING INFLATION [J].

LINDE, AD ;

LYTH, DH .

PHYSICS LETTERS B, 1990, 246 (3-4) :353-358

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