The black hole/string transition in anti de Sitter space

by Erez Urbach

at Particles and Fields Seminar

Mon, 08 May 2023, 14:00
Sacta-Rashi Building for Physics (54), room 207


String stars, or Horowitz-Polchinski solutions, are string theory saddles with normalizable condensates of thermal-winding strings. In the past, string stars were offered as a possible description of stringy (Euclidean) black holes in asymptotically flat spacetime, close to the Hagedorn temperature. I will discuss the thermodynamic properties of string stars in asymptotically (thermal) anti-de Sitter background (including AdS3 with NS-NS flux), their possible connection to small black holes in AdS, and their implications for holography. I will also present new ``winding-string gas'' saddles for confining holographic backgrounds such as the Witten model, and their relation to the deconfined phase of 3+1 pure Yang-Mills.

Created on 01-05-2023 by Lublinsky, Michael (lublinm)
Updaded on 01-05-2023 by Lublinsky, Michael (lublinm)