AdS5 x S5 Black Hole Metric at O(alpha'3)
Abstract
We compute O(α'3) corrections to the AdS5× S5 black hole metric. We find that the radius of the S5 depends on the radial AdS5 coordinate. This completes the computation of Gubser, Klebanov and Tseytlin (hep-th/9805156). The fact that the metric no longer factorizes should modify the value of the Wilson line at finite temperature and the glueball mass spectrum.
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