PPT-Ultralow Absorption Conductive Coatings for Charge Dissipation in LIGO mirrors
Author : ceila | Published Date : 2023-11-16
Aykutlu Dana Ashot Markosyan Riccardo Bassiri Edgard Bonilla Brian Lantz Martin Fejer LIGO Group Stanford University CA 94305 The Need for a Conductive Coating
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Ultralow Absorption Conductive Coatings for Charge Dissipation in LIGO mirrors: Transcript
Aykutlu Dana Ashot Markosyan Riccardo Bassiri Edgard Bonilla Brian Lantz Martin Fejer LIGO Group Stanford University CA 94305 The Need for a Conductive Coating Charging is believed to degrade. for the 1. st. Advanced LIGO Science Run. Jordan Camp. NASA Goddard Space Flight Center. Moriond. Gravitation Meeting. March 25, 2015. Search Team. Lindy Blackburn (. CfA. ). Nelson Christensen (Carleton College). Poynting. dominated outflows. Yuri . Lyubarsky. Ben-Gurion . University . Ubiquity . of relativistic . outflows in astrophysics. Crab nebula in X-rays. M 87. GRB lightcurves. R. elativistic outflows are associated with: . Justin Hodgkiss. SCPS postgraduate workshop. 15 January 2013. Goal. To get the audience to . appreciate. your . science story. What’s the story?. Be very clear in your head before making slides. Distil. Approach. :. Collaborators. :. Accomplishments. :. Development of high reflectivity coatings to increase system throughput, particularly in the far-UV . (FUV) spectral . range. Study other dielectric fluoride coatings and other deposition technologies such as Ion Beam Sputtering (IBS) that is expected to produce the nearest to ideal morphology optical thin film coatings and thus low scatter.. . Conductive Polymers. 7.03.2010. Dennis. Literature Seminar. Polymers are typically utilized in electrical and electronic applications as . insulators. ,where advantage is taken of their very high . Justin Hodgkiss. SCPS postgraduate workshop. 15 January 2013. Goal. To get the audience to . appreciate. your . science story. What’s the story?. Be very clear in your head before making slides. Distil. An Indo-US joint mega-project concept proposal. . IndIGO Consortium. (. Ind. ian . I. nitiative in . G. ravitational-wave . O. bservations). Tarun . Souradeep. IUCAA . (. Spokesperson, IndIGO). Laser . Interferometer . Gravitational . Wave . Observatory. Hiroaki Yamamoto Caltech/LIGO. Introduction. Newton’s gravity to Einstein’s general relativity. Gravitational Wave. Source and signal. 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 . Introduction. Initial LIGO and advanced LIGO. Sensitivities. Commissioning status. Targeting . the first . observations. 1. Some . slides are . from “. ET-. aLIGO. . and . beyond”, LIGO-G14001331, by David Shoemaker. -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 . LIGO is an acronym for Laser Interferometer Gravitational-wave Observatory. The word A Mirror Jonah Kanner. , Branson Stephens. , . Michele . Vallisneri. , Alan Weinstein, Roy . Williams. 8/11/14. LOSC. 1. LIGO-. G1400509v4. Why LOSC? . Access data with ease. No need to login to LDAS cluster.
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