PPT-Advanced localization of massive black hole coalescences wi

Ryan Lang Scott Hughes MIT 7 th International LISA Symposium June 17 2008 Overview LISA source coalescing massive black hole binaries Focus on the inspiral circular orbits Key question What is the . 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 . Ryan Lang. Scott Hughes. MIT. 7. th. International LISA Symposium. June 17, 2008. Overview. LISA source: coalescing massive black hole binaries. Focus on the . inspiral. , circular orbits.. Key question: What is the . . 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. Priyamvada Natarajan . Yale University. . Volonteri. ; Johnson. ; Park ; . Ricotti. ; . Khochfar. ; Di . Matteo. ; Yoshida ; . Haiman. ; Tanaka ; . Schneider Dubois ; . Bournoud. ; Loeb ; . Emanuele. . Berti. , University of . Mississippi/Caltech. Texas Symposium, São Paulo, Dec 18 2012. What are . “strong field. ” tests?. Alternatives to GR: massive scalars. BH . dynamics and . superradiance. 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 . Gabriela . Gonz. ález. Louisiana State University. LSC spokesperson. For the LIGO Scientific Collaboration and . the Virgo Collaboration. LIGO Livingston Observatory,. Louisiana, USA. LIGO Hanford Observatory. 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.