PPT-General Black Hole solutions in D=5 SUGRA

in D5 SUGRA To be published in PRD 高エネルギー加速器研究機構　 KEK 素粒子原子核研究所　理論センター 宇宙 物理グルーブ 富沢真也　 共同研究者溝口俊弥. IU Astronomy. Mini-University 2014. Monster Black Holes. What . is a . black . h. ole. ,. anyway?. A black hole is….. …an object whose gravity is so intense that light cannot escape. How Big . By Irina . Plaks. What is a black hole?. . A . black hole is a . region in . spacetime. where . the gravitational field is so strong that . nothing, not even light, can escape it.. Black Holes and the General Theory of Relativity. Thermodynamics with Lambda: Some Consequences. L. David . Kubiz. ňák. (Perimeter Institute). . Lambda and Quasi-Lambda workshop. University of Massachusetts, Amherst, MA, USA. April 10 – April 12, 2014. Soliton. Collisions. Frans. Pretorius. Princeton University. . Workshop on. Tests of Gravity and Gravitational Physics. May 19-21, 2009. Case Western Reserve University, Cleveland, Ohio. Outline. Why explore high speed black . . Holes. Ginnie Baldwin. PHYSICS 1050: Astronomy. Fall 2011. BLACK HOLE. WHAT IS A BLACK HOLE?. A black hole is a concentration of matter so dense that not even light can escape its gravitational pull.. General Relativity. Principle of equivalence:. There is no experiment that will discern the difference between the effect of gravity and the effect of acceleration.. Or…. Gravitational and inertial mass are equivalent.. Escape Velocity. The minimum velocity needed to leave the vicinity of a body without ever being pulled back by the . body’. s . gravity is the . escape velocity. . . Escape Velocity. The escape velocity from a body depends on its . . The Obvious Question. Once matter enters a black hole, is it fated never to reappear? . The answer seemed obvious – a clear . “. yes. ”. . – until about . forty . years . ago.. Oops!. Apparently not! . Yi-Hsieh Wang, Ted Jacobson, Mark Edwards, and Charles W. Clark. arXiv:1705.01907 . Black hole explosions?. Experimental black-hole evaporation?. Black hole lasers. Implementation in Bose-Einstein condensates. Syed. Ali . Raza. General Relativity Project. Overview. Kerr Metric for rotating Black holes. Kerr Metric for extreme angular momentum. Static Limit and the . ergosphere. Radial and Tangential motion of light. Ted Jacobson. University of Maryland. Gravity and Black Holes, Cambridge, July 4, 2017 . Wheeler to . Bekenstein. (1971):. “If I drop a teacup into a black hole, . I conceal from all the world the. L. David . Kubiz. ňák. (Perimeter Institute). . Lambda and Quasi-Lambda workshop. University of Massachusetts, Amherst, MA, USA. April 10 – April 12, 2014. Plan of the talk. Black holes as thermodynamic objects . Jeroen van Dongen & Sebastian de Haro. U. Amsterdam & Cambridge U.. BHI, Harvard, May 2017. Questions. :. Why. BH . central. object of . theoretical. . study. ?. How have . theorists. . interacted. A. xion . S. uperradian. T. instabilities. BLASTs. João G. Rosa. Aveiro University. w. ith. . Tom . Kephart. . (Vanderbilt University). Phys.. Rev. . Lett. . . 120,. 231102 (2018) (. Editors’ Suggestion.