A note on infinities in eternal inflation

被引:9
|
作者
Ellis, George F. R. [1 ]
Stoeger, William R. [1 ,2 ]
机构
[1] Univ Cape Town, ZA-7701 Cape Town, South Africa
[2] Univ Arizona, Steward Observ, Vatican Observ Res Grp, Tucson, AZ 85721 USA
关键词
Inflation; Infinity; UNIVERSE;
D O I
10.1007/s10714-008-0715-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In some well-known scenarios of open-universe eternal inflation, developed by Vilenkin and co-workers, a large number of universes nucleate and thermalize within the eternally inflating mega-universe. According to the proposal, each universe nucleates at a point, and therefore the boundary of the nucleated universe is a space-like surface nearly coincident with the future light cone emanating from the point of nucleation, all points of which have the same proper-time. This leads the authors to conclude that at the proper-time t = t (nuc) at which any such nucleation occurs, an infinite open universe comes into existence. We point out that this is due entirely to the supposition of the nucleation occurring at a single point, which in light of quantum cosmology seems difficult to support. Even an infinitesimal space-like length at the moment of nucleation gives a rather different result-the boundary of the nucleating universe evolves in proper time and becomes infinite only in an infinite time. The alleged infinity is never attained at any finite time.
引用
收藏
页码:1475 / 1484
页数:10
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