Effects of a nonvanishing cosmological constant on the spherically symmetric vacuum manifold
Effects of a nonvanishing cosmological constant on the spherically symmetric vacuum manifold
复制标题
非零宇宙学常数对球对称真空流形的影响
DOI：
10.1103/physrevd.15.3513
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发表时间：
1977
影响因子：
5
通讯作者：
R. C. Roeder
中科院分区：
文献类型：
--
作者：
K. Lake;R. C. Roeder
本文详细研究了当宇宙常数，...λ..，不假定为零。For .. lambda.. > 0且3 m <或=.. lambda../ sup-1/sup 2/它表明，这些表面构成的交界处的无限数量的区域和完整的流形可以表示在一个因果的方式由有限数量的区域。
The conformal structure of timelike 2-surfaces of the vacuum manifold is examined in detail in the cases when the cosmological constant, ..lambda.., is not assumed to be zero. For ..lambda.. > 0 with 3m < or = ..lambda../sup -1///sup 2/ it is shown that these surfaces constitute the junction of an infinite number of regions and that the complete manifold may be represented in a causal way by a finite number of regions.