Towards the core of the cosmological constant problem
arXiv:1404.4437 · doi:10.1093/ptep/ptv182
Abstract
We apply a new self-tuning mechanism to the well-known Kachru-Kallosh-Linde-Trivedi (KKLT) model to address the cosmological constant problem. In this mechanism the cosmological constant contains a supersymmetry breaking term besides the usual scalar potential of the supergravity, which is distinguished from the usual theories where is directly identified with alone. Also in this mechanism, whether vanishes or not is basically determined by the tensor structure of the scalar potential density, not by the zero or nonzero values of the scalar potential itself. As a result of this application we find that the natural scenario for the vanishing of the present universe is to take one of the AdS (rather than dS) vacua of KKLT as the background vacuum of our present universe. This AdS vacuum scenario has more nice properties as compared with dS vacua of the usual flux compctifications. The background vacuum is stable both classically and quantum mechanically (no tunneling instabilities), and the value is also stable against quantum corrections because in this scenario the perturbative corrections of and quantum fluctuations on the branes are all gauged away by an automatic cancelation between and .
Final version (typos all fixed)
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