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• W2079585986 abstract "In the saddle point approximation, the Euclidean path integral for quantum gravity closely resembles a thermodynamic partition function, with the cosmological constant $Lambda$ playing the role of temperature and the ``density of topologies'' acting as an effective density of states. For $Lambda<0$, the density of topologies grows superexponentially, and the sum over topologies diverges. In thermodynamics, such a divergence can signal the existence of a maximum temperature. The same may be true in quantum gravity: the effective cosmological constant may be driven to zero by a rapid rise in the density of topologies." @default.
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• W2079585986 date "1997-11-24" @default.
• W2079585986 modified "2023-09-25" @default.
• W2079585986 title "Spacetime Foam and the Cosmological Constant" @default.
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• W2079585986 doi "https://doi.org/10.1103/physrevlett.79.4071" @default.
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