A self-tuning mechanism in (3+p)d gravity-scalar theory
arXiv:hep-th/0702171 · doi:10.1088/1126-6708/2007/11/051
Abstract
We present a new type of self-tuning mechanism for ()d brane world models in the framework of gravity-scalar theory. This new type of self-tuning mechanism exhibits a remarkable feature. In the limit , being the string coupling, the geometry of bulk spacetime remains virtually unchanged by an introduction of the Standard Model(SM)-brane, and consequently it is virtually unaffected by quantum fluctuations of SM fields with support on the SM-brane. Such a feature can be obtained by introducing Neveu-Schwarz(NS)-brane as a background brane on which our SM-brane is to be set. Indeed, field equations naturally suggest the existence of the background NS-brane. Among the given such models, of the most interest is the case with , where represents the bulk cosmological constant. This model contains a pair of coincident branes (of the SM- and the NS-branes), one of which is a codimension-2 brane placed at the origin of 2d transverse space (), another a codimension-1 brane placed at the edge of . These two branes are (anti) T-duals of each other, and one of them may be identified as our SM-brane plus the background NS-brane. In the presence of the background NS-brane (and in the absence of ), the 2d transverse space becomes an orbifold with an appropriate deficit angle. But this is only possible if the ()d Planck scale and the string scale () are of the same order, which accords with the hierarchy assumption \cite{1,2,3} that the electroweak scale is the only short distance scale existing in nature.
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