论文标题
黑洞：关于克尔假设的普遍性
Black holes: on the universality of the Kerr hypothesis
论文作者
论文摘要
黑洞（BHS）和Kerr几何形状描述的是天体物理，深色，紧凑的物体在多大程度上？我们踏上了违抗这种非凡思想的普遍性的行使，通常称为“克尔假设”。在建立了其理由和及时性之后，我们为深色紧凑物体的替代模型定义了一组最小的合理性标准。然后，作为原理的证明，我们讨论了具体，动态强大的非kerr bhs和无地模仿者，即1）通过基本的理论，尤其是动态的测试，2）匹配（某些）天文学可观察到的（某些）天文学可观察结果，而3）仅在某些（摩克镜）尺度上出现。这些示例说明了如何挑战克尔假说的普遍性（在所有宏观尺度上）。
To what extent are all astrophysical, dark, compact objects both black holes (BHs) and described by the Kerr geometry? We embark on the exercise of defying the universality of this remarkable idea, often called the "Kerr hypothesis". After establishing its rationale and timeliness, we define a minimal set of reasonability criteria for alternative models of dark compact objects. Then, as proof of principle, we discuss concrete, dynamically robust non-Kerr BHs and horizonless imitators, that 1) pass the basic theoretical, and in particular dynamical, tests, 2) match (some of the) state of the art astrophysical observables and 3) only emerge at some (macroscopic) scales. These examples illustrate how the universality (at all macroscopic scales) of the Kerr hypothesis can be challenged.
