ar X iv : h ep - t h / 99 10 11 1 v 1 1 4 O ct 1 99 9 Correlation functions for chiral primaries in D = 6 Supergravity on AdS 3 × S 3

ar X iv : h ep - t h / 99 03 05 4 v 2 2 0 O ct 1 99 9 INJE - TP - 99 - 2 Scattering from an AdS 3 bubble and an exact AdS

ar X iv : h ep - t h / 99 03 20 9 v 1 2 4 M ar 1 99 9 SMI - Th – 99 / 04 AdS 3 / CFT 2 correspondence at finite temperature

The AdS/CFT correspondence is established for the AdS 3 space compactified on a solid torus with the CFT field on the boundary. Correlation functions that correspond to the bulk theory at finite temperature are obtained in the regularization a'la Gubser, Klebanov, and Polyakov. The BTZ black hole solutions in AdS 3 are T-dual to the solution in the AdS 3 space without singularity.

ar X iv : h ep - p h / 99 10 24 8 v 1 6 O ct 1 99 9 1 Effect of σ ( 600 ) - Production in pp̄ → 3 π 0 at rest

ar X iv : h ep - t h / 95 11 20 5 v 2 6 D ec 1 99 5 Quantum dynamics of N = 1 , D = 4 supergravity chiral compensator

A new four-dimensional N = 1 superfield model is suggested. The model is induced by supertrace anomaly of matter superfields in curved superspace and leads to effective theory of supergravity chiral compensator. A renormal-ization structure of this model is studied, one-loop counterterms are calculated and renormalization group equations are investigated. It is shown that the theory under consi...

ar X iv : h ep - p h / 99 10 50 6 v 1 2 7 O ct 1 99 9 hep - ph / 9910506 SHEP 99 / 18 Fine - Tuning Constraints on Supergravity Models

We discuss fine-tuning constraints on supergravity models. The tightest constraints come from the experimental mass limits on two key particles: the lightest CP even Higgs boson and the gluino. We also include the lightest chargino which is relevant when universal gaugino masses are assumed. For each of these particles we show how fine-tuning increases with the experimental mass limit, for four...