English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Employing higher curvature corrections to Einstein--Maxwell gravity hasgarnered a great deal of attention motivated by the high energy regime inquantum nature of black hole physics. In addition, one may employ gravity'srainbow to encode quantum gravity effects into the black hole solutions. Inthis paper, we regard an energy dependent static spacetime with varioustopologies and study its black hole solutions in the context of Gauss--BonnetBorn--Infeld (GB--BI) gravity. We study thermodynamic properties and examinethe first law of thermodynamics. Using suitable local transformation, we endowthe Ricci--flat black hole solutions with a global rotation and study theeffects of rotation on thermodynamic quantities. We also investigate thermalstability in canonical ensemble through calculating the heat capacity. Weobtain the effects of various parameters on the horizon radius of stable blackholes. Finally, we discuss second order phase transition in the extended phasespace thermodynamics and investigate the critical behavior.

Energy-dependent topological anti-de Sitter black holes in Gauss-Bonnet Born-Infeld gravity