1998/08/20 by Jacek Pawelczyk, Stefan Theisen · 2 citations
Physics and Astronomy · #AdS black hole #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Computation #Extremal black hole #Glueball #Metric (unit) #Noncommutative and Quantum Gravity Theories #Primordial black hole #RADIUS #hep-th
paper · pdf · doi:10.1088/1126-6708/1998/09/010
published as JHEP 9809:010,1998 · 7 pages, TeX (harvmac)
arxiv created 1998/08/20 · openalex publication_date 1998/09/14 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
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.