We show that the previously obtained subtracted geometry of four-dimensional asymptotically flat multi-charged rotating black holes, whose massless wave equation exhibit $SL(2,\R) \times SL(2,\R) \times SO(3)$ symmetry may be obtained by a suitable scaling limit of certain asymptotically flat multi-charged rotating black holes, which is reminiscent of near-extreme black holes in the dilute gas approximation. The co-homogeneity-two geometry is supported by a dilation field and two (electric) gauge-field strengths. We also point out that these subtracted geometries can be obtained as a particular Harrison transformation of the original black holes. Furthermore the subtracted metrics are asymptotically conical (AC), like global monopoles, thus describing "a black hole in an AC box". Finally we account for the the emergence of the $SL(2,\R) \times SL(2,\R) \times SO(3)$ symmetry as a consequence of the subtracted metrics being Kaluza-Klein type quotients of $ AdS_3\times 4 S^3$. We demonstrate that similar properties hold for five-dimensional black holes.
Supersymmetric Conical Defects: Towards a string theoretic description of black hole formation
AdS_3中的圆锥形缺陷,或称点粒子,是最简单的非平凡引力系统之一,特别令人感兴趣,因为它们的碰撞可以形成黑洞。我们将三维BPS锥型缺陷嵌入到六维N= 4 b超引力中,这是由K3上紧化的IIB弦论产生的。详细分析了球上六维理论所需的Kaluza-Klein约化,包括与三维Chern-Simons超引力的关系。我们表明,通过嵌入三维锥形缺陷得到的六维空间出现在旋转黑弦的近视界极限。分析了这些解的各种性质,并在渐近AdS_3 x S^3空间的CFT对偶中给出了我们的缺陷的一个表示。我们的工作旨在作为分析形成黑洞的碰撞缺陷的第一步。
Scaling Solutions of Matter Form Factors in Asymptotically Safe Quantum Gravity
INAF Osservatorio Astrofisico di Catania(意大利国家天体物理研究所卡塔尼亚天文台);INFN, Sezione di Catania(意大利国家核物理研究所卡塔尼亚分部);Institut für Theoretische Physik, Heidelberg University(海德堡大学理论物理研究所);Institute for Mathematics, Astrophysics and Particle Physics, Radboud University(拉德堡德大学数学、天体物理学和粒子物理研究所);Dipartimento di Fisica e Astronomia, Università di Catania(卡塔尼亚大学物理与天文学系)