Spontaneous Decay of the Effective Cosmological Constant
Abstract
We discuss the notion that quantum fields may induce an effective time-dependent cosmological constant which decays from a large initial value. It is shown that such cosmological models are viable in a non-de Sitter spacetime.
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Submitted on 10 Feb 1998 (v1), last revised 12 Feb 1998 (this version, v2)
Updated
arXiv.org
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