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

机译:磁性黑洞和垄断在非初始的爱因斯坦 - 阳厂理论中具有宇宙学常数:精确的解决方案

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摘要

Alternative theories of gravity and their solutions are of considerable importance since, at some fundamental level, the world can reveal new features. Indeed, it is suspected that the gravitational field might be nonminimally coupled to the other fields at scales not yet probed, bringing into the forefront nonminimally coupled theories. In this mode, we consider a nonminimal Einstein-Yang-Mills theory with a cosmological constant. Imposing spherical symmetry and staticity for the spacetime and a magnetic Wu-Yang ansatz for the Yang-Mills field, we find expressions for the solutions of the theory. Further imposing constraints on the nonminimal parameters, we find a family of exact solutions of the theory depending on five parameters-two nonminimal parameters, the cosmological constant, the magnetic charge, and the mass. These solutions represent magnetic monopoles and black holes in magnetic monopoles with de Sitter, Minkowskian, and anti-de Sitter asymptotics, depending on the sign and value of the cosmological constant Lambda. We classify completely the family of solutions with respect to the number and the type of horizons and show that the spacetime solutions can have, at most, four horizons. For particular sets of the parameters, these horizons can become double, triple, and quadruple. For instance, for a positive cosmological constant., there is a critical Lambda(c) for which the solution admits a quadruple horizon, evocative of the Lambda(c) that appears for a given energy density in both the Einstein static and Eddington-Lemaitre dynamical universes. As an example of our classification, we analyze solutions in the Drummond-Hathrell nonminimal theory that describe nonminimal black holes. Another application is with a set of regular black holes previously treated.
机译:由于在一些基本一级,世界可以揭示新功能,重力及其解决方案的替代理论具有重要意义。实际上,怀疑引力场可能是不是尚未探测的尺度的其他领域,引入前端的非偏离理论。在这种模式下,我们考虑非富有的爱因斯坦 - 杨工厂,具有宇宙学常数。为杨米尔斯领域施加球形对称和静态对称和磁武杨安萨茨的球形对称和静态,我们发现了对该理论的解决方案的表达。进一步施加对非生体参数的限制,我们发现了一个理论的精确解决方案的家庭,这取决于五个参数 - 两个非初始参数,宇宙常数,磁性电荷和质量。这些解决方案代表了磁隔离的磁并垄断和黑洞,与De Satter,Minkowskian和Anti-de Satter渐近学相反,取决于宇宙常数λ的标志和价值。我们完全分类了各种解决方案,以及视野的类型和类型,并表明即最多四个地平线可以具有。对于特定的参数集,这些视野可以变成双重,三倍和四倍。例如,对于阳性宇宙常数,还有一个关键的λ(c),该溶液承认四肢地平线,突出的λ(c)唤起,所述Lambda(c)似乎在爱因斯坦静态和埃丁顿 - 勒米特黎的给定能量密度动态宇宙。作为我们分类的一个例子,我们分析了描述非初生黑洞的德拉蒙特 - 赫内尔非分析理论的解决方案。另一个应用程序是先前处理过的一组常规黑洞。

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  • 来源
    《Physical review, D》 |2016年第1期|共21页
  • 作者单位

    Kazan Fed Univ Inst Phys Dept Gen Relat &

    Gravitat Kremlevskaya Str 18 Kazan 420008 Russia;

    Univ Lisbon Ctr Multidisciplinar Astrofis CENTRA IST Dept Fis Ave Rovisco Pais 1 P-1049001 Lisbon Portugal;

    Kazan Fed Univ Inst Phys Dept Gen Relat &

    Gravitat Kremlevskaya Str 18 Kazan 420008 Russia;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 粒子物理学;场论;
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