ON THE SCALAR FIELD-DYNAMICS IN A SPATIALLY FLAT FRIEDMAN UNIVERSE

被引:202
作者
MUSLIMOV, AG
机构
[1] Ioffe Inst. for Phys. and Technol., Acad. of Sci., Leningrad
关键词
D O I
10.1088/0264-9381/7/2/015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The dynamics of a spatially homogeneous scalar field, generating a conformally flat Friedman metric, is considered. It is assumed that the scalar field is weakly coupled to ordinary matter and is described by a rather arbitrary potential. The examples of some exact and asymptotic solutions to the non-linear differential equation appearing in the problem, are presented. The possible implications of the solutions for cosmology are briefly pointed out.
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页码:231 / 237
页数:7
相关论文
共 11 条
[1]   COSMIC NO-HAIR THEOREMS AND INFLATION [J].
BARROW, JD .
PHYSICS LETTERS B, 1987, 187 (1-2) :12-16
[2]   INFLATIONARY MODELS WITH EXPONENTIAL POTENTIALS [J].
BURD, AB ;
BARROW, JD .
NUCLEAR PHYSICS B, 1988, 308 (04) :929-945
[3]  
IVANOV GG, 1983, GRAVIATION GENERAL R, V20, P37
[4]  
IVANOV GG, 1980, IZV VUZ F, V12, P18
[5]  
KRECHET VG, 1979, PROBLEMS THEORY GRAV
[6]  
Liouville, 1853, J MATH PURE APPL, V36, P71
[7]  
MUSLIMOV AG, 1989, 1317 LEN I PHYS TECH
[8]   IDENTITY FOR T-ORDERED EXPONENTIALS WITH APPLICATIONS TO QUANTUM-MECHANICS [J].
ONOFRI, E .
ANNALS OF PHYSICS, 1976, 102 (02) :371-387
[10]  
RATRA B, 1987, PUPT1072 PRINC U PRE