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Nonminimal black holes with regular electric field

机译:具有规则电场的最小黑洞

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We discuss the problem of identification of coupling constants, which describe interactions between photons and spacetime curvature, using exact regular solutions to the extended equations of the nonminimal Einstein-Maxwell theory. We argue the idea that three nonminimal coupling constants in this theory can be reduced to the single guiding parameter, which plays the role of nonminimal radius. We base our consideration on two examples of exact solutions obtained earlier in our works: the first of them describes a nonminimal spherically symmetric object (star or black hole) with regular radial electric field; the second example represents a nonminimal Dirac-type object (monopole or black hole) with regular metric. We demonstrate that one of the inflexion points of the regular metric function identifies a specific nonminimal radius, thus marking the domain of dominance of nonminimal interactions.
机译:我们讨论对耦合常数的识别问题,该问题描述了使用非最小爱因斯坦-麦克斯韦理论的扩展方程的精确正则解,描述了光子与时空曲率之间的相互作用。我们认为,该理论中的三个非最小耦合常数可以简化为单个引导参数,该参数起着非最小半径的作用。我们基于早先在工作中获得的精确解的两个示例进行考虑:第一个描述具有规则径向电场的非最小球形对称物体(星形或黑洞);第二个示例表示具有常规度量的非最小Dirac型对象(单极或黑洞)。我们证明了常规度量函数的拐点之一标识了特定的非最小半径,从而标记了非最小交互作用的优势域。

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