RELIC GRAVITATIONAL-WAVES AND EXTENDED INFLATION

被引:151
作者
TURNER, MS
WILCZEK, F
机构
[1] UNIV CHICAGO,ENRICO FERMI INST,DEPT PHYS & ASTRON,CHICAGO,IL 60637
[2] UNIV CHICAGO,ENRICO FERMI INST,DEPT ASTROPHYS,CHICAGO,IL 60637
[3] INST ADV STUDY,SCH NAT SCI,PRINCETON,NJ 08540
关键词
D O I
10.1103/PhysRevLett.65.3080
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In extended inflation, a new version of inflation where the transition from an inflationary to a radiation-dominated Universe is accomplished by bubble nucleation, bubble collisions supply a potent and potentially detectable source of gravitational waves. The energy density in relic gravitons from bubble collisions is expected to be about 10-5 of closure density. Their characteristic wavelength depends upon the reheating temperature TRH: (104 cm)[(1014 GeV)/TRH]. If black holes are produced by bubble collisions, they will evaporate producing shorter-wavelength gravitons. © 1990 The American Physical Society.
引用
收藏
页码:3080 / 3083
页数:4
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