A self-tuning mechanism in (3+p)d gravity-scalar theory
Eun Kyung Park, Pyung Seong Kwon

TL;DR
This paper introduces a novel self-tuning mechanism in (3+p)d gravity-scalar brane models that stabilizes the bulk geometry against SM-brane quantum fluctuations by employing a background NS-brane, especially in zero bulk cosmological constant scenarios.
Contribution
It proposes a new self-tuning mechanism involving NS-branes in (3+p)d gravity-scalar theories, ensuring bulk geometry stability and addressing hierarchy issues.
Findings
Bulk geometry remains unchanged by SM-brane quantum fluctuations.
The model naturally suggests the existence of a background NS-brane.
In the zero cosmological constant case, the transverse space forms an orbifold with a deficit angle.
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…
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