High Energy Physics - Theory
[Submitted on 14 Nov 2000 (v1), last revised 23 Mar 2001 (this version, v3)]
Title:Model for self-tuning the cosmological constant
View PDFAbstract: 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.
Submission history
From: Jihn E. Kim [view email][v1] Tue, 14 Nov 2000 11:10:37 UTC (6 KB)
[v2] Wed, 15 Nov 2000 03:25:12 UTC (6 KB)
[v3] Fri, 23 Mar 2001 09:02:38 UTC (8 KB)
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