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X-WR-CALNAME:The black hole/string transition in anti de Sitter space
X-WR-TIMEZONE:Pacific Time (US & Canada)
BEGIN:VEVENT
DTSTAMP:20260608T225837Z
UID:tag:localist.com\,2008:EventInstance_44345222041133
DTSTART:20231002T210000Z
DTEND:20231002T223000Z
DESCRIPTION:Erez Urbach's talk has been canceled.\n\nAbstract: String stars
 \, or Horowitz-Polchinski solutions\, are string theory saddles with norma
 lizable 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 w
 ill discuss the thermodynamic properties of string stars in asymptotically
  (thermal) anti-de Sitter background (including AdS3 with NS-NS flux)\, th
 eir possible connection to small black holes in AdS\, and their implicatio
 ns 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.
GEO:37.428507;-122.172389
LOCATION:Varian Physics Lab\, Conference Room 355
SUMMARY:Canceled: The black hole/string transition in anti de Sitter space
URL;VALUE=URI:https://events.stanford.edu/event/the_black_holestring_transi
 tion_in_anti_de_sitter_space
CATEGORIES:Lecture/Presentation/Talk
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