THE DYNAMIC BEHAVIOR OF SCALAR FIELDS NEAR THE INITIAL SINGULARITY

被引:8
作者
DERITIS, R [1 ]
PLATANIA, G [1 ]
SCUDELLARO, P [1 ]
STORNAIOLO, C [1 ]
机构
[1] IST NAZL FIS NUCL,SEZ NAPOLI,I-80125 NAPLES,ITALY
关键词
D O I
10.1007/BF00769249
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Analyzing the Klein-Gordon equation in a homogeneous, Isotropic and spatially flat universe model, we find the conditions for the existence of a universe dominated by a scalar field in its early stages. © 1990 Plenum Publishing Corporation.
引用
收藏
页码:97 / 109
页数:13
相关论文
共 12 条
[1]  
ALBRECHT A, 1982, PHYS REV LETT, V48, P389
[2]  
BELINSKY VA, 1985, ZH EKSP TEOR FIZ, V62, P195
[3]  
CHIELLINI A, 1940, REND SEMIN FS U CAGL, V10, P16
[4]  
GUTH A, 1981, PHYS REV D, V23, P327
[6]   AN UNUSUAL COSMOLOGICAL SOLUTION FOR LAMDA-PHI-4 THEORY WITH BROKEN SYMMETRY [J].
MADSEN, MS .
GENERAL RELATIVITY AND GRAVITATION, 1986, 18 (08) :879-882
[7]   SCALAR FIELDS IN CURVED SPACETIMES [J].
MADSEN, MS .
CLASSICAL AND QUANTUM GRAVITY, 1988, 5 (04) :627-639
[8]   CHAOTIC INFLATION [J].
MADSEN, MS ;
COLES, P .
NUCLEAR PHYSICS B, 1988, 298 (04) :701-725
[9]   COSMOLOGICAL CONSEQUENCES OF A ROLLING HOMOGENEOUS SCALAR FIELD [J].
RATRA, B ;
PEEBLES, PJE .
PHYSICAL REVIEW D, 1988, 37 (12) :3406-3427
[10]  
Singh T., 1987, International Journal of Modern Physics A, V2, P645, DOI 10.1142/S0217751X87000235