CAN BULK VISCOSITY DRIVE INFLATION

被引：45

作者：

PACHER, T

STEINSCHABES, JA

TURNER, MS

机构：

[1] EOTVOS LORAND UNIV,INST THEORET PHYS,H-1088 BUDAPEST,HUNGARY

[2] FERMI NATL ACCELERATOR LAB,THEORET ASTROPHYS GRP,BATAVIA,IL 60510

[3] UNIV CHICAGO,ENRICO FERMI INST,DEPT PHYS & ASTRON,CHICAGO,IL 60637

[4] UNIV CHICAGO,ENRICO FERMI INST,DEPT ASTROPHYS,CHICAGO,IL 60637

来源：

PHYSICAL REVIEW D | 1987年 / 36卷 / 06期

关键词：

D O I：

10.1103/PhysRevD.36.1603

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：1603 / 1606

页数：4

共 14 条

[1] CONSTRAINTS ON GENERALIZED INFLATIONARY COSMOLOGIES [J].

ABBOTT, LF ;

WISE, MB .

NUCLEAR PHYSICS B, 1984, 244 (02) :541-548

[2] COSMOLOGY FOR GRAND UNIFIED THEORIES WITH RADIATIVELY INDUCED SYMMETRY-BREAKING [J].

ALBRECHT, A ;

STEINHARDT, PJ .

PHYSICAL REVIEW LETTERS, 1982, 48 (17) :1220-1223

[3] THE DEFLATIONARY UNIVERSE - AN INSTABILITY OF THE DESITTER UNIVERSE [J].

BARROW, JD .

PHYSICS LETTERS B, 1986, 180 (04) :335-339

[4]

BERNSTEIN J, 1987, RU87B1188 ROCK U REP

[5]

DIOSI L, 1984, ACTA PHYS POL B, V15, P909

[6] INFLATIONARY UNIVERSE - A POSSIBLE SOLUTION TO THE HORIZON AND FLATNESS PROBLEMS [J].

GUTH, AH .

PHYSICAL REVIEW D, 1981, 23 (02) :347-356

[7]

HODGES HM, UNPUB

[8] A NEW INFLATIONARY UNIVERSE SCENARIO - A POSSIBLE SOLUTION OF THE HORIZON, FLATNESS, HOMOGENEITY, ISOTROPY AND PRIMORDIAL MONOPOLE PROBLEMS [J].

LINDE, AD .

PHYSICS LETTERS B, 1982, 108 (06) :389-393

[9]

MATARESSE S, 1985, PHYS REV D, V32, P1316

[10]

STEWART JM, 1973, CARGESE LECTURES PHY, V6

← 1 2 →