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Magnetic black holes and monopoles in a nonminimal Einstein-Yang-Mills theory with a cosmological constant: Exact solutions

机译:非最小爱因斯坦 - 杨 - 米尔斯的磁黑洞和单极子   具有宇宙常数的理论:精确解

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摘要

Alternative theories of gravity and their solutions are of considerableimportance since at some fundamental level the world can reveal new features.Indeed, it is suspected that the gravitational field might be nonminimallycoupled to the other fields at scales not yet probed, bringing into theforefront nonminimally coupled theories. In this mode, we consider a nonminimalEinstein-Yang-Mills theory with a cosmological constant. Imposing sphericalsymmetry and staticity for the spacetime and a magnetic Wu-Yang ansatz for theYang-Mills field, we find expressions for the solutions of the theory. Furtherimposing constraints on the nonminimal parameters, we find a family of exactsolutions of the theory depending on five parameters, namely, two nonminimalparameters, the cosmological constant, the magnetic charge, and the mass. Thesesolutions represent magnetic monopoles and black holes in magnetic monopoleswith de Sitter, Minkowskian, and anti-de Sitter asymptotics, depending on thesign and value of the cosmological constant $\Lambda$. We classify completelythe family of solutions with respect to the number and the type of horizons andshow that the spacetime solutions can have, at most, four horizons. Forparticular sets of the parameters, these horizons can become double, triple,and quadruple. For instance, for a positive cosmological constant $\Lambda$,there is a critical $\Lambda_c$ for which the solution admits a quadruplehorizon, evocative of the $\Lambda_c$ that appears for a given energy densityin both the Einstein static and Eddington-Lema\^{\i}tre dynamical universes. Asan example of our classification, we analyze solutions in the Drummond-Hathrellnonminimal theory that describe nonminimal black holes. Another application iswith a set of regular black holes previously treated.
机译:引力的替代理论及其解决方案非常重要,因为在某些基本层面上,世界可以揭示新的特征。实际上,人们怀疑引力场可能以尚未探索的规模非最小耦合至其他场,从而引入了前面的非最小耦合理论。 。在这种模式下,我们考虑具有宇宙学常数的非最小爱因斯坦-杨米尔斯理论。通过对时空施加球对称性和静态性,并对杨-米尔斯场施加吴五星磁场,我们找到了该理论解的表达式。进一步对非最小参数施加约束,我们根据五个参数,即两个非最小参数,宇宙学常数,磁电荷和质量,找到了该理论的精确解系列。这些解表示磁单极子和带有de Sitter,Minkowskian和anti-de Sitter渐近论的磁单极子中的黑洞,具体取决于宇宙常数$ \ Lambda $的符号和值。我们根据地平线的数量和类型对解决方案家族进行了完全分类,并显示时空解决方案最多可以具有四个地平线。对于特定的参数集,这些范围可以变为两倍,三倍和四倍。例如,对于一个正的宇宙常数$ \ Lambda $,存在一个临界的$ \ Lambda_c $,对于该常数,该解决方案接受一个四倍水平的表示,回想了在给定能量密度下在爱因斯坦静态和爱丁顿方程中出现的$ \ Lambda_c $。 Lema \ ^ {\ i} tre动力宇宙。作为分类的示例,我们分析了Drummond-Hathrellnonminimal理论中描述非最小黑洞的解决方案。另一个应用是一组预先处理过的规则黑洞。

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