The cosmological constant problems
In David B. Cline (ed.) Sources and Detection of Dark Matter and Dark Energy in the Universe, Berlin, Heidelberg, 2001, pp. 18–26
Abstract
The old cosmological constant problem is to understand why the vacuum energy is so small; the new problem is to understand why it is comparable to the present mass density. Several approaches to these problems are reviewed. Quintessence does not help with either; anthropic considerations offer a possibility of solving both. In theories with a scalar field that takes random initial values, the anthropic principle may apply to the cosmological constant, but probably to nothing else.
