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. a Kerr parameter solution for spinning BH depends on mass and Kerr parameter aM 0 no spin Schwarzschild black hole solution depends on mass only aM 1 maximally rotating Kerr black hole brPage 3br Space around a spinning Black Hole figure from T Amplifying and Muffling Sound A mplify - ______________________________________________________________ Mu ffle - _______________________________________________________________ Amplifying Sound Exp www.elsevier.com/locate/chemgeo Correspondingauthor.E-mailaddresses:kerra@cf.ac.uk(A.C.Kerr),jmahoney@hawaii.edu(J.J.Mahoney).0009-2541/$-seefrontmatter 孫. 佳叡. Jia-Rui. Sun. National Central University. National Center for Theoretical Sciences. , . September 14, 2010 . Based on arxiv:1006.4092 and 1006.4097, C.-M. Chen, Y.-M. Huang, JRS, . 対応における. Non-. extremal. 補正について. 松尾 善典. Based on . YM-. Tsukioka. -. Yoo. [arXiv:0907.0303]. YM-. Nishioka. [arXiv:1010.4549]. Kerr/CFT. 対応において. Left mover. INDIVIDUAL BOY PERSONAL DATA Name: ______________________________________________________________ T ROO P Date of Birth ____ / ____ / _ __ ___ BSA ID# __________ _____________________ NO.________ A Using . Optima. to optimize resource allocations. Outline. Background. How . Optima . works. Data . requirements for . Optima. Using . Optima. in practice. Optima. vs. Spectrum. Outline. Background. 218 Kerr Administration Building, Corvallis OR 97331 - 2120 T 541 - 737 - 2241 | F 541 - 737 - 4494 | E financial.aid@oregonstate.edu / F INANCIAL AID 101 3 - 13 - 2012 Retaking Coursework at the www.self - esteem - experts.com ______________________________________________________________ See Our Complete List of Self Est eem Activities (www.self - esteem - experts.com/self - esteem - activi DOG OWNER’S ,AST NAME FIRST NAME(S) ( ________ ( HOME # WORK # CELL # ADDRESS CITY Email Address _____________________________________________________________________ 1102.0529. http. ://www.physik.uzh.ch/events/lisa2016/uploads/031/lisa2016_sahughes.pdf. Self force:. EMRI . waveform. status: the . math. /GR side. Dissipative: . radiates E,J. Conservative. :. . shift from geodesic motion. EMN Meeting: Quantum Comm. & Quantum Imaging, Berlin, Aug 2016. John S. Colton. Physics Department. Brigham Young . University, Provo, Utah. Student researchers: . Ken Clark. Daniel Craft. Jane Cutler. Benjamin Hardy, . Bowling Green State University. . Joseph . Grames, . Thomas Jefferson National Accelerator Facility. * . This work is supported by . the . National Science Foundation, Research Experience for Undergraduates award 1359026 and the Department of Energy, Laboratory Directed Research and Development contract DE-AC05-06OR23177.. Measurement Corbyn Mellinger Dr. Xu Group June 10, 2016 Common Magneto - optical Effects • Faraday Effect: magnetization of material affects transmission of polarized light • Kerr Effect: magneti