Nonperturbative sum over topologies in 2D Lorentzian quantum gravity
AIP Conf. Proc. -- November 3, 2006 -- Volume 861, pp. 391-397
ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE;
doi:10.1063/1.2399601
Issue Date: 3 November 2006
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The recent progress in the Causal Dynamical Triangulations (CDT) approach to quantum gravity indicates that gravitation is nonperturbatively renormalizable. We review some of the latest results in 1+1 and 3+1 dimensions with special emphasis on the 1+1 model. In particular we discuss a nonperturbative implementation of the sum over topologies in the gravitational path integral in 1+1 dimensions. The dynamics of this model shows that the presence of infinitesimal wormholes leads to a decrease in the effective cosmological constant. Similar ideas have been considered in the past by Coleman and others in the formal setting of 4D Euclidean path integrals. A remarkable property of the model is that in the continuum limit we obtain a finite space-time density of microscopic wormholes without assuming fundamental discreteness. This shows that one can in principle make sense out of a gravitational path integral including a sum over topologies, provided one imposes suitable kinematical restrictions on the state-space that preserve large scale causality. ©2006 American Institute of Physics
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KEYWORDS and PACS
PUBLICATION DATA
0094-243X (print)
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