QUANTUM COSMOLOGY WITH A COMPLEX FIELD

被引：24

作者：

AMENDOLA, L

KHALATNIKOV, IM

LITTERIO, M

OCCHIONERO, F

机构：

[1] UNIV ROMA LA SAPIENZA,IST ASTRON,I-00161 ROME,ITALY

[2] LD LANDAU THEORET PHYS INST,117940 MOSCOW,RUSSIA

来源：

PHYSICAL REVIEW D | 1994年 / 49卷 / 04期

关键词：

D O I：

10.1103/PhysRevD.49.1881

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The classical and quantum cosmology of a complex scalar field is considered. In this model the Euclidean region contour in the minisuperspace is generally a closed curve. The wave function of the Universe, evaluated in the WKB approximation, propagates through scattering or tunneling from the initial classical state to the final classical state. The probability distribution for the Vilenkin choice of boundary conditions shows that the classical universe preferentially starts with a large matter content only if the cosmological constant is set to zero.

引用

页码：1881 / 1885

页数：5

共 15 条

[11] QUANTUM COSMOLOGY AND THE INITIAL STATE OF THE UNIVERSE [J].

VILENKIN, A .

PHYSICAL REVIEW D, 1988, 37 (04) :888-897

[12] BIRTH OF INFLATIONARY UNIVERSES [J].

VILENKIN, A .

PHYSICAL REVIEW D, 1983, 27 (12) :2848-2855

[13] CREATION OF UNIVERSES FROM NOTHING [J].

VILENKIN, A .

PHYSICS LETTERS B, 1982, 117 (1-2) :25-28

[14] QUANTUM COSMOLOGICAL APPROACH TO THE COSMIC NO-HAIR CONJECTURE IN THE BIANCHI TYPE-IX SPACETIME [J].

YOKOYAMA, J ;

MAEDA, K .

PHYSICAL REVIEW D, 1990, 41 (04) :1047-1053

[15]

ZELDOVICH YB, 1984, SOV ASTRON LETT+, V10, P135

← 1 2 →