Towards a Naturally Small Cosmological Constant from Branes in 6D Supergravity
Y. Aghababaie, C.P. Burgess, S.L. Parameswaran, F. Quevedo

TL;DR
This paper explores a 6D supergravity model where branes can self-tune the effective 4D cosmological constant to a small value, potentially explaining dark energy and linking it to observable effects in gravity tests.
Contribution
It demonstrates a classical self-tuning mechanism in 6D supergravity with branes, and analyzes an explicit anomaly-free model with partial success due to topological constraints.
Findings
3-branes can remain classically flat regardless of tension
Self-tuning may be stabilized by bulk supersymmetry
Explicit model shows partial realization of the mechanism
Abstract
We investigate the possibility of self-tuning of the effective 4D cosmological constant in 6D supergravity, to see whether it could naturally be of order 1/r^4 when compactified on two dimensions having Kaluza-Klein masses of order 1/r. In the models we examine supersymmetry is broken by the presence of non-supersymmetric 3-branes (on one of which we live). If r were sub-millimeter in size, such a cosmological constant could describe the recently-discovered dark energy. A successful self-tuning mechanism would therefore predict a connection between the observed size of the cosmological constant, and potentially observable effects in sub-millimeter tests of gravity and at the Large Hadron Collider. We do find self tuning inasmuch as 3-branes can quite generically remain classically flat regardless of the size of their tensions, due to an automatic cancellation with the curvature and…
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