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We study the near horizon geometry of both static and stationary extremal Oliva Tempo Troncoso (OTT) black holes. For each of these cases, a set of consistent asymptotic conditions is… Click to show full abstract
We study the near horizon geometry of both static and stationary extremal Oliva Tempo Troncoso (OTT) black holes. For each of these cases, a set of consistent asymptotic conditions is introduced. The canonical generator for the static configuration is shown to be regular. For the rotating OTT black hole, the asymptotic symmetry is described by the time reparametrization, the chiral Virasoro and centrally extended $u(1)$ Kac-Moody algebras.
Keywords:
horizon ott;
black hole;
near horizon;
hole asymptotic;
ott black
Journal Title: Chinese Physics C
Year Published: 2019
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Journal Title: Chinese Physics C
Year Published: 2019
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!