Role of a "Local" Cosmological Constant in Euclidean Quantum Gravity

preprint1996arXivOpen access

Abstract

In 4D non-perturbative Regge calculus a positive value of the effective cosmological constant characterizes the collapsed phase of the system. If a local term of the form S′=∑hε{h1,h2,...}λhVhS'=\sum_{h ε\{h_1,h_2,...\} } λ_h V_h is added to the gravitational action, where {h1,h2,...}\{h_1,h_2,...\} is a subset of the hinges and {λh}\{λ_h\} are positive constants, one expects that the volumes Vh1V_{h_1}, Vh2V_{h_2}, ... tend to collapse and that the excitations of the lattice propagating through the hinges {h1,h2,...}\{h_1,h_2,...\} are damped. We study the continuum analogue of this effect. The additional term S′S' may represent the coupling of the gravitational field to an external Bose condensate.

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