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- W4327989519 abstract "String stars, or Horowitz-Polchinski solutions, are Euclidean string theory saddles with a normalizable condensate of thermal winding strings. String stars were suggested as a possible description of stringy (Euclidean) black holes close to the Hagedorn temperature. In this work, we continue the study initiated in arXiv:2202.06966 by investigating the thermodynamic properties of string stars in asymptotically (thermal) anti-de Sitter backgrounds. First, we discuss the case of AdS$_3$ with mixed RR and NS-NS fluxes (including the pure NS-NS system) and comment on a possible BTZ/string transition unique to AdS$_3$. Second, we present new ``winding-string gas'' saddles for confining holographic backgrounds such as the Witten model, and determine the subleading correction to their Hagedorn temperature. We speculate a black brane/string transition in these models and argue for a possible relation to the deconfined phase of 3+1 dimensional pure Yang-Mills." @default.
- W4327989519 created "2023-03-21" @default.
- W4327989519 creator A5001477312 @default.
- W4327989519 date "2023-03-16" @default.
- W4327989519 modified "2023-09-30" @default.
- W4327989519 title "The black hole/string transition in AdS$_3$ and confining backgrounds" @default.
- W4327989519 doi "https://doi.org/10.48550/arxiv.2303.09567" @default.
- W4327989519 hasPublicationYear "2023" @default.
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