PPT-Advanced LIGO status Hiro Yamamoto LIGO lab/Caltech

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Introduction Initial LIGO and advanced LIGO Sensitivities Commissioning status Targeting the first observations 1 Some slides are from ET aLIGO and beyond

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Advanced LIGO status Hiro Yamamoto LIGO lab/Caltech: Transcript


Introduction Initial LIGO and advanced LIGO Sensitivities Commissioning status Targeting the first observations 1 Some slides are from ET aLIGO and beyond LIGOG14001331 by David Shoemaker. on surfaces that is an order of magnitude faster than stateoftheart methods while still pro ducing 64257elds of equal or better quality Fields produced by the method are globally optimal in the sense that they minimize a simple wellde64257ned quadr Kamiyama & Yamamoto Visual representation of prosody for tactful communication:2 Figure 1. Sentences /kaite itadakemaseka/ (left) and /kaite itadakemasedesjoka/ (right) pronounced by the instructor Mars Science Laboratory. Your Name Here. MSL Science Team. 9/27/12. NASA/JPL-Caltech/MSSS. Curiosity’s Science Objectives. NASA/JPL-Caltech. Curiosity’. s . primary scientific goal is to explore and quantitatively assess a local region on . Yamamoto (KEK) and John W. Mitchell (NASA-GSFC) . for the BESS Collaboration. To be. presented . at . SpacePart12, held at CERN, November 5-7, 2012. Search for Primary Antiparticles and Cosmological Antimatter with BESS. A Case Study with . Remote Association . Test. IST 4 Information and Logic. Yue Li. . and Betsy Fu. (Metal, Iron). (Baby, Cries). (Crush, Dark). (School, Grocery). (Rose, Flower). (Obey, Inch). (Fruit, Apple). The Search for Gravitational Waves with Advanced LIGO. Tiffany Summerscales, . Andrews University Dept. . of Physics. What are gravitational waves?. Einstein’s theory of General Relativity predicts that mass curves the fabric of . Barry C Barish. LIGO Laboratory . 1-Sept-2017. 17-Aug-17. PAX Workshop - Amsterdam. 2. Context of G3: Where will we be?. Particle Physics. 17-Aug-17. PAX Workshop - Amsterdam. 3. Gravitational Waves. https://www.ligo.caltech.edu/system/video_items/files/4/EinsteinsMessengerLIGO.mp4?1436490806. 2017 Nobel Prize in Physics. : Rainer Weiss - Barry C. . Barish. -Kip S. . Thorne. "for . decisive contributions to the LIGO detector and the observation of gravitational waves". -Style. Peter Couvares. Syracuse . University, LIGO . Scientific . Collaboration. Condor Week 2013. 1 May 2013. Who am I. ? What is LIGO?. Former Condor Team member (‘99-’08).. Now at Syracuse . Figure1:PhysicalandlogicalarchitectureofHIRO-NET:theblueareasaretheLowerTier(BLE),whiletheorangearearepresentstheUpperTier(VHF).Inparticular,SectionIVaccuratelydescribestheLowerTierfunctionalitiesofHI 1 A Brief History of LIGO One hundred years ago, using his recently general relativity theory, Albert Einstein predicted the existence of gravitational waves and described their properties. To Einstei LIGO is an acronym for Laser Interferometer Gravitational-wave Observatory. The word 1ABriefHistoryofLIGOOnehundredyearsagousinghisrecentlygeneralrelativitytheoryAlbertEinsteinpredictedtheexistenceofgravitationalwavesanddescribedtheirpropertiesToEinsteinthesewavesseemedtooweakevertobe Under a Dark MoonUntitled ndInk on paper17 x 22 31 inCollection of the artistUntitled ndInk on paper10 x 7 inCollection of the artistUntitled ndInk on paper2 x 5 30292827 inCollection of the artis

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