Model for self-tuning the cosmological constant

Details Model for self-tuning the cosmological constant Model for self-tuning the cosmological constant

2000-11-14

arxiv.org/abs/hep-th/0011118v3

Phys.Rev.Lett. 86 (2001) 4223-4226

Physics

High Energy Physics

High Energy Physics - Theory

LaTeX file of 4 pages, to appear in Phys. Rev. Lett

Scientific paper

10.1103/PhysRevLett.86.4223

The vanishing cosmological constant in the four dimensional space-time is obtained in a 5D Randall-Sundrum model with a brane (B1) located at $y=0$. The matter fields can be located at the brane. For settling any vacuum energy generated at the brane to zero, we need a three index antisymmetric tensor field $A_{MNP}$ with a specific form for the Lagrangian. For the self-tuning mechanism, the bulk cosmological constant should be negative.

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