Power-Yang-Mills black holes and black branes in quartic quasi-topological gravity
Askar Ali, Khalid Saifullah

TL;DR
This paper investigates higher-dimensional quartic quasi-topological black holes in power-Yang-Mills theory, analyzing their solutions, thermodynamics, stability, and extending to rotating black branes within the AdS/CFT framework.
Contribution
It introduces new solutions for power-Yang-Mills black holes in quartic quasi-topological gravity and studies their thermodynamic stability and properties in various ensembles.
Findings
Real solutions exist only for positive quartic quasi-topological coefficients.
Black holes can have one, two horizons, or naked singularities depending on parameters.
Stability regions are identified for smaller black holes in grand canonical ensemble.
Abstract
We study higher dimensional quartic quasi-topological black holes in the framework of non-abelian power-Yang-Mills theory. It is shown that real solutions of the gravitational field equations exist only for positive values of quartic quasi-topological coefficient. Depending on the values of the mass parameter and Yang-Mills charge, they can be interpreted as black holes with one horizon, two horizons and naked singularity. It is also shown that the solution associated with these black holes has an essential curvature singularity at the centre . Thermodynamic and conserved quantities for these black holes are computed and we show that the first law has been verified. We also check thermodynamic stability in both canonical and grand canonical ensembles. In addition to this, we also formulate new power-Yang-Mills black hole solutions in pure quasi-topological gravity. The physical and…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Astrophysical Phenomena and Observations
