INFLATION AND BROKEN LORENTZ SYMMETRY IN THE VERY EARLY UNIVERSE

被引:31
作者
GASPERINI, M [1 ]
机构
[1] IST NAZL FIS NUCL,TURIN,ITALY
关键词
D O I
10.1016/0370-2693(85)90197-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:84 / 86
页数:3
相关论文
共 11 条
[1]   CONSTRAINTS ON GENERALIZED INFLATIONARY COSMOLOGIES [J].
ABBOTT, LF ;
WISE, MB .
NUCLEAR PHYSICS B, 1984, 244 (02) :541-548
[2]  
DESABBATA V, 1985, TOPOLOGICAL PROPERTI
[3]   INFLATIONARY UNIVERSE - A POSSIBLE SOLUTION TO THE HORIZON AND FLATNESS PROBLEMS [J].
GUTH, AH .
PHYSICAL REVIEW D, 1981, 23 (02) :347-356
[4]   THE INFLATIONARY UNIVERSE [J].
LINDE, AD .
REPORTS ON PROGRESS IN PHYSICS, 1984, 47 (08) :925-986
[5]  
LUCCHIN F, 1985, ISAS2585EP PREPR
[6]   LORENTZ NON-INVARIANCE [J].
NIELSEN, HB ;
PICEK, I .
NUCLEAR PHYSICS B, 1983, 211 (02) :269-296
[7]   BETA-FUNCTION IN A NON-COVARIANT YANG-MILLS THEORY [J].
NIELSEN, HB ;
NINOMIYA, M .
NUCLEAR PHYSICS B, 1978, 141 (1-2) :153-177
[8]   THE REDEI-LIKE MODEL AND TESTING LORENTZ INVARIANCE [J].
NIELSEN, HB ;
PICEK, I .
PHYSICS LETTERS B, 1982, 114 (2-3) :141-146
[9]   INFLATION-DRIVING SCALAR FIELD [J].
PI, SY .
NUCLEAR PHYSICS B, 1985, 252 (1-2) :127-140
[10]  
ROSEN N, 1985, PH858 TECHN PREPR