Abstract

In this paper, we formulate two new classes of black hole solutions in higher curvature quartic quasitopological gravity with nonabelian Yang–Mills theory. At first step, we consider the SO(n) and SO(n-1,1) semisimple gauge groups. We obtain the analytic quartic quasitopological Yang–Mills black hole solutions. Real solutions are only accessible for the positive value of the redefined quartic quasitopological gravity coefficient, mu _{4}. These solutions have a finite value and an essential singularity at the origin, r=0 for space dimension higher than 8. We also probe the thermodynamic and critical behavior of the quasitopological Yang–Mills black hole. The obtained solutions may be thermally stable only in the canonical ensemble. They may also show a first order phase transition from a small to a large black hole. In the second step, we obtain the pure quasitopological Yang–Mills black hole solutions. For the positive cosmological constant and the space dimensions greater than eight, the pure quasitopological Yang–Mills solutions have the ability to produce both the asymptotically AdS and dS black holes for respectively the negative and positive constant curvatures, k=-1 and k=+1. This is unlike the quasitopological Yang–Mills theory which can lead to just the asymptotically dS solutions for Lambda >0. The pure quasitopological Yang–Mills black hole is not thermally stable.

Highlights

  • Quasitopological gravity is one of the candidates of the modified theories having the ability to resolve the Einstein’s equation defects [2,3]

  • From the viewpoint of the anti-de Sitter (AdS)/CFT correspondence, quasitopological gravity can cause a broader class of four-dimensional CFT’s which includes three independent parameters relating the central charges of the conformal field theories with the coupling parameters of the gravitational spacetimes [2,4–7]

  • This is while that the quartic quasitopological gravity contributes to the field equations for space dimensions n ≥ 4, except for n = 7 [2]

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Summary

Introduction

Quasitopological gravity is one of the candidates of the modified theories having the ability to resolve the Einstein’s equation defects [2,3]. Based on the advantages of the quasitopological gravity over the Lovelock theory as mentioned, we are willing to obtain the solutions of the pure quasitopological Yang–Mills black hole in the second part of this paper. 2, we obtain the black hole solutions of the (n + 1)-dimensional quartic quasitopological gravity coupled to the Yang–Mills theory and discuss the physical properties of the solutions. 4. In the second part of this paper, we obtain the pure quasitopological Yang–Mills black hole solution and investigate the physical properties in Sect.

Thermodynamic behaviors of the quasitopological Yang–Mills black hole
Critical exponents
Pure quasitopological Yang–Mills black hole solutions
Thermodynamic behaviors of the pure quasitopological Yang–Mills black holes
Concluding remarks
Coefficients of the quartic quasitopological gravity
Gauge potentials for some gauge groups
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