Role of a "Local" Cosmological Constant in Euclidean Quantum Gravity
G. Modanese
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'=Σh ε\h1,h2,...\ λh Vh is added to the gravitational action, where \h1,h2,...\ is a subset of the hinges and \λh\ are positive constants, one expects that the volumes Vh1, Vh2, ... tend to collapse and that the excitations of the lattice propagating through the hinges \h1,h2,...\ are damped. We study the continuum analogue of this effect. The additional term S' may represent the coupling of the gravitational field to an external Bose condensate.
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