PPT-Black Hole Thermodynamics with Lambda: Some Consequences

Author : tatyana-admore | Published Date : 2018-10-20

L David Kubiz ňák Perimeter Institute Lambda and QuasiLambda workshop University of Massachusetts Amherst MA USA April 10 April 12 2014 Plan of the talk Black

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Black Hole Thermodynamics with Lambda: Some Consequences: Transcript


L David Kubiz ňák Perimeter Institute Lambda and QuasiLambda workshop University of Massachusetts Amherst MA USA April 10 April 12 2014 Plan of the talk Black holes as thermodynamic objects . Information. . Scramblers. How. . information. . survives. . falling. . into. a black hole. Master thesis Wilke van der Schee. Supervised by prof. Gerard ’t Hooft. August 19, 2010. Introduction. 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.. 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 . M87. Hercules A radio jets. Active Galactic Nuclei (AGNs) and Supermassive Black Holes. The identification by Maarten Schmidt (1963, . Nature. , 197, 1040) of the radio source 3C 273 as a . “. star. . 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. 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.

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