MATTERS of GRAVITY *******Anniversary Edition*******
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LIGO Detector and Hardware Introduction
LIGO Detector and Hardware Introduction Virtual Open Data Workshop May 2020 LIGO-G2000795 Outline • Introduction 45W • Interferometry 40W 1.6kW 200kW Locking Optical cavities • Hardware • Noise Fundamental Technical • Commissioning/Observation Runs • Future Detector Plans • Bibliography Gravitational Waves • Metric tensor perturbation in GR = + 2 polarization in GR Scalar and other possible waves ℎ • Free falling masses • Change in laser propagation time • Phase difference in light ∝ ℎ • Interferometry detects phase difference ∝ ℎ • Astronomical Sources Modeling Modeled Unmodeled /Length Modeled vs Unmodeled Short Inspirals (BBH, Bursts Short vs Long BNS, BH/NS) (Supernova) Long Continuous Waves Stochastic Known vs Unknown (Pulsars) Background Sensitivity Estimate • Strain from single photon: = 10 2 • Need strain 10 � −10 ℎ ≅ • Shot noise SNR− 22 = 10 improvement,∝ � 10 photons At1 1002 Hz equivalent to power24 of 20 MW • • With 200 W of input laser power, 45W 200kW 40W 1.6kW requires power gain of 100,000 Total optical gain in LIGO is ~50,000 Ignores other noise sources Gravitational Wave Detector Network GEO 600: Germany Virgo: Italy KAGRA: Japan Interferometry • Book by Peter Saulson • Michelson interferometer Fringe splitting • Fabry-Perot arms Cavity pole, = ⁄4ℱ • Pound-Drever-Hall locking 45W 200kW 40W 1.6kW Match laser frequency to cavity length RF modulation with EOM • Feedback and controls Other LIGO Cavities • Mode cleaners Input and output 45W 200kW 40W 1.6kW Single Gauss-Laguerre mode • Power recycling Output dark -
0045-Flyer-Einstein-En-2.Pdf
FEATHERBEDDINGCOMPANYWEIN HOFJEREMIAHSTATUESYN AGOGEDREYFUSSMOOSCEMETERY MÜNSTERPLATZRELATIVI TYE=MC 2NOBELPRIZEHOMELAND PERSECUTIONAFFIDAVIT OFSUPPORTEMIGRATIONEINSTEIN STRASSELETTERSHOLOCAUSTRESCUE FAMILYGRANDMOTHERGRANDFAT HERBUCHAUPRINCETONBAHNHOF STRASSE20VOLKSHOCHSCHULEFOU NTAINGENIUSHUMANIST 01 Albert Einstein 6 7 Albert Einstein. More than just a name. Physicist. Genius. Science pop star. Philosopher and humanist. Thinker and guru. On a par with Copernicus, Galileo or Newton. And: Albert Einstein – from Ulm! The most famous scientist of our time was actually born on 14th March 1879 at Bahnhofstraße 20 in Ulm. Albert Einstein only lived in the city on the Danube for 15 months. His extended family – 18 of Einstein’s cousins lived in Ulm at one time or another – were a respected and deep-rooted part of the city’s society, however. This may explain Einstein’s enduring connection to the city of his birth, which he described as follows in a letter to the Ulmer Abend- post on 18th March 1929, shortly after his 50th birthday: “The birthplace is as much a unique part of your life as the ancestry of your biological mother. We owe part of our very being to our city of birth. So I look on Ulm with gratitude, as it combines noble artistic tradition with simple and healthy character.” 8 9 The “miracle year” 1905 – Einstein becomes the founder of the modern scientific world view Was Einstein a “physicist of the century”? There‘s no doubt of that. In his “miracle year” (annus mirabilis) of 1905 he pub- lished 4 groundbreaking works along- side his dissertation. Each of these was worthy of a Nobel Prize and turned him into a physicist of international standing: the theory of special relativity, the light quanta hypothesis (“photoelectric effect”), Thus, Albert Einstein became the found- for which he received the Nobel Prize in er of the modern scientific world view. -
A Dissertation Submitted in Partial Satisfaction of the Requirements for the Degree Doctor of Philosophy
UNIVERSITY OF CALIFORNIA, SAN DIEGO PUBLIC CATHOLICISM AND RELIGIOUS PLURALISM IN AMERICA: THE ADAPTATION OF A RELIGIOUS CULTURE TO THE CIRCUMSTANCE OF DIVERSITY, AND ITS IMPLICATIONS A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Sociology by Michael J. Agliardo, SJ Committee in charge: Professor Richard Madsen, Chair Professor John H. Evans Professor David Pellow Professor Joel Robbins Professor Gershon Shafir 2008 Copyright Michael J. Agliardo, SJ, 2008 All rights reserved. The Dissertation of Michael Joseph Agliardo is approved, and it is acceptable in quality and form for publication on microfilm and electronically: Chair University of California, San Diego 2008 iii TABLE OF CONTENTS Signature Page ......................................................................................................................... iii Table of Contents......................................................................................................................iv List Abbreviations and Acronyms ............................................................................................vi List of Graphs ......................................................................................................................... vii Acknowledgments ................................................................................................................. viii Vita.............................................................................................................................................x -
Matters of Gravity
MATTERS OF GRAVITY The newsletter of the Division of Gravitational Physics of the American Physical Society Number 49 June 2017 Contents DGRAV News: we hear that . , by David Garfinkle ..................... 3 DGRAV student travel grants, by Beverly Berger .............. 4 Research Briefs: The Discovery of GW170104, by Jenne Driggers and Salvatore Vitale ... 5 Obituary: Remembering Vishu, by Naresh Dadhich and Bala Iyer ........... 8 Remembering Cecile DeWitt-Morette, by Yvonne Choquet-Bruhat ..... 13 arXiv:1706.06183v2 [gr-qc] 22 Jun 2017 Remembering Larry Shepley, by Richard Matzner and Mel Oakes ...... 15 Remembering Marcus Ansorg, by Bernd Br¨ugmannand Reinhard Meinel . 16 Conference Reports: EGM20, by Abhay Ashtekar ......................... 18 Editor David Garfinkle Department of Physics Oakland University Rochester, MI 48309 Phone: (248) 370-3411 Internet: garfinkl-at-oakland.edu WWW: http://www.oakland.edu/?id=10223&sid=249#garfinkle Associate Editor Greg Comer Department of Physics and Center for Fluids at All Scales, St. Louis University, St. Louis, MO 63103 Phone: (314) 977-8432 Internet: comergl-at-slu.edu WWW: http://www.slu.edu/colleges/AS/physics/profs/comer.html ISSN: 1527-3431 DISCLAIMER: The opinions expressed in the articles of this newsletter represent the views of the authors and are not necessarily the views of APS. The articles in this newsletter are not peer reviewed. 1 Editorial The next newsletter is due December 2017. This and all subsequent issues will be available on the web at https://files.oakland.edu/users/garfinkl/web/mog/ All issues before number 28 are available at http://www.phys.lsu.edu/mog Any ideas for topics that should be covered by the newsletter should be emailed to me, or Greg Comer, or the relevant correspondent. -
A Brief History of Gravitational Waves
Review A Brief History of Gravitational Waves Jorge L. Cervantes-Cota 1, Salvador Galindo-Uribarri 1 and George F. Smoot 2,3,4,* 1 Department of Physics, National Institute for Nuclear Research, Km 36.5 Carretera Mexico-Toluca, Ocoyoacac, Mexico State C.P.52750, Mexico; [email protected] (J.L.C.-C.); [email protected] (S.G.-U.) 2 Helmut and Ana Pao Sohmen Professor at Large, Institute for Advanced Study, Hong Kong University of Science and Technology, Clear Water Bay, 999077 Kowloon, Hong Kong, China. 3 Université Sorbonne Paris Cité, Laboratoire APC-PCCP, Université Paris Diderot, 10 rue Alice Domon et Leonie Duquet 75205 Paris Cedex 13, France. 4 Department of Physics and LBNL, University of California; MS Bldg 50-5505 LBNL, 1 Cyclotron Road Berkeley, CA 94720, USA. * Correspondence: [email protected]; Tel.:+1-510-486-5505 Abstract: This review describes the discovery of gravitational waves. We recount the journey of predicting and finding those waves, since its beginning in the early twentieth century, their prediction by Einstein in 1916, theoretical and experimental blunders, efforts towards their detection, and finally the subsequent successful discovery. Keywords: gravitational waves; General Relativity; LIGO; Einstein; strong-field gravity; binary black holes 1. Introduction Einstein’s General Theory of Relativity, published in November 1915, led to the prediction of the existence of gravitational waves that would be so faint and their interaction with matter so weak that Einstein himself wondered if they could ever be discovered. Even if they were detectable, Einstein also wondered if they would ever be useful enough for use in science. -
Chicago Physics One
CHICAGO PHYSICS ONE 3:25 P.M. December 02, 1942 “All of us... knew that with the advent of the chain reaction, the world would never be the same again.” former UChicago physicist Samuel K. Allison Physics at the University of Chicago has a remarkable history. From Albert Michelson, appointed by our first president William Rainey Harper as the founding head of the physics department and subsequently the first American to win a Nobel Prize in the sciences, through the mid-20th century work led by Enrico Fermi, and onto the extraordinary work being done in the department today, the department has been a constant source of imagination, discovery, and scientific transformation. In both its research and its education at all levels, the Department of Physics instantiates the highest aspirations and values of the University of Chicago. Robert J. Zimmer President, University of Chicago Welcome to the inaugural issue of Chicago Physics! We are proud to present the first issue of Chicago Physics – an annual newsletter that we hope will keep you connected with the Department of Physics at the University of Chicago. This newsletter will introduce to you some of our students, postdocs and staff as well as new members of our faculty. We will share with you good news about successes and recognition and also convey the sad news about the passing of members of our community. You will learn about the ongoing research activities in the Department and about events that took place in the previous year. We hope that you will become involved in the upcoming events that will be announced. -
APS News January 2019, Vol. 28, No. 1
January 2019 • Vol. 28, No. 1 A PUBLICATION OF THE AMERICAN PHYSICAL SOCIETY Plasma physics and plants APS.ORG/APSNEWS Page 3 Highlights from 2018 Blending Paint with Physics The editors of Physics (physics. The experiments sparked a series By Leah Poffenberger aps.org) look back at their favorite of theoretical studies, each attempt- 2018 APS Division of Fluid stories of 2018, from groundbreak- ing to explain this unconventional Dynamics Meeting, Atlanta— ing research to a poem inspired by behavior (see physics.aps.org/ Five years ago, Roberto Zenit, a quantum physics. articles/v11/84). One prediction physics professor at the National Graphene: A New indicates that twisted graphene’s Autonomous University of Mexico, superconductivity might also be Superconductor later reported the first observation was studying biological flows when topological, a desirable property 2018’s splashiest condensed- of the Higgs boson decaying into art historian Sandra Zetina enlisted for quantum computation. matter-physics result came bottom quarks (see physics.aps.org/ him for a project: using fluid from two sheets of graphene. The Higgs Shows up with the articles/v11/91). This decay is the dynamics to uncover the secret Researchers in the USA and Japan Heaviest Quarks most likely fate of the Higgs boson, behind modern art techniques. reported finding superconductiv- After detecting the Higgs boson but it was extremely difficult to At this year’s Division of Fluid ity in stacked graphene bilayers in 2012, the next order of business see above the heavy background Dynamics meeting—his 20th— ids, a person who has developed in which one layer is twisted with was testing whether it behaves as of bottom quarks generated in a Zenit, an APS Fellow and member certain knowledge about the way respect to the other. -
SENTENARYO NG TEORYANG GENERAL RELATIVITY March 14, 2016 (1 - 3 Pm), NIP Auditorium, up Diliman Program Emcees: Ms
SENTENARYO NG TEORYANG GENERAL RELATIVITY March 14, 2016 (1 - 3 pm), NIP Auditorium, UP Diliman Program Emcees: Ms. Cherrie Olaya and Mr. Nestor Bareza National Anthem Welcome Remarks Academician William G. Padolina (NAST) Presentation 1 Einstein: Science, Image, and Impact (Dr. Perry Esguerra) Presentation 2 Einstein and the Music of the Spheres (Dr. Ian Vega) Intermission NIP Resonance Choir Presentation 3 From Einstein’s Universe to the Multiverse (Dr. Reina Reyes) Open Forum* *Moderators: Dr. May Lim and Dr. Nathaniel Hermosa II Closing Remarks Dr. Jose Maria P. Balmaceda (UP College of Science) (Refreshments will be served at the NIP Veranda) What’s Inside? Organizing Committee Messages p.1 Extended Abstracts 8 Dr. Percival Almoro (Chair) Einstein chronology 18 Dr. Perry Esguerra Einstein quotations 19 Dr. Ian Vega Dr. Caesar Saloma (Convenor) Outside Front Cover Outside Back Cover Inside Back Cover Einstein in Vienna, 1921 Depiction of gravitational waves Galaxies By: F. Schmutzer generated by binary neutron stars. By: Hubble Ultra Deep Field (Wikimedia Commons) By: R. Hurt/Caltech-JPL (http://hyperphysics.phy-astr.gsu. (http://www.jpl.nasa.gov/im- edu/hbase/astro/deepfield.html) ages/universe/20131106/pul- sar20131106-full.jpg) Acknowledgements Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 1 2 Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 3 4 Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) http://www.npr.org/sections/thetwo-way/2016/02/11/466286219/in-milestone- scientists-detect-waves-in-space-time-as-black-holes-collide https://www.youtube.com/watch?v=B4XzLDM3Py8 https://soundcloud.com/emily-lakdawalla Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 5 6 Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 7 Einstein: Science, Image, and Impact By Perry Esguerra ‘WHY is it that nobodY for photoluminescence, the ory of relativity. -
Albert Einstein - Wikipedia, the Free Encyclopedia Page 1 of 27
Albert Einstein - Wikipedia, the free encyclopedia Page 1 of 27 Albert Einstein From Wikipedia, the free encyclopedia Albert Einstein ( /ælbərt a nsta n/; Albert Einstein German: [albt a nʃta n] ( listen); 14 March 1879 – 18 April 1955) was a German-born theoretical physicist who developed the theory of general relativity, effecting a revolution in physics. For this achievement, Einstein is often regarded as the father of modern physics.[2] He received the 1921 Nobel Prize in Physics "for his services to theoretical physics, and especially for his discovery of the law of the photoelectric effect". [3] The latter was pivotal in establishing quantum theory within physics. Near the beginning of his career, Einstein thought that Newtonian mechanics was no longer enough to reconcile the laws of classical mechanics with the laws of the electromagnetic field. This led to the development of his special theory of relativity. He Albert Einstein in 1921 realized, however, that the principle of relativity could also be extended to gravitational fields, and with his Born 14 March 1879 subsequent theory of gravitation in 1916, he published Ulm, Kingdom of Württemberg, a paper on the general theory of relativity. He German Empire continued to deal with problems of statistical Died mechanics and quantum theory, which led to his 18 April 1955 (aged 76) explanations of particle theory and the motion of Princeton, New Jersey, United States molecules. He also investigated the thermal properties Residence Germany, Italy, Switzerland, United of light which laid the foundation of the photon theory States of light. In 1917, Einstein applied the general theory of relativity to model the structure of the universe as a Ethnicity Jewish [4] whole. -
Stefan W. Ballmer
Stefan W. Ballmer Curriculum Vitae Department of Physics Phone: +1-315-443-3882 Syracuse University Cell: +1-315-278-1154 Syracuse, NY 13244 Fax: +1-315-443-9103 USA E-mail: [email protected] Citizenship: USA, Switzerland Web: thecollege.syr.edu/people/faculty/ballmer-stefan RECENT AND CURRENT POSITIONS Jun 2016 - Associate Professor of Physics present Syracuse University, Syracuse, NY May 2019 - Visiting Associate Professor of Physics Jun 2019 Institute for Cosmic Ray Research, University of Tokyo, Japan May 2018 - Visiting Associate Professor of Physics Jun 2018 Institute for Cosmic Ray Research, University of Tokyo, Japan May 2017 - Visiting Associate Professor of Physics Jun 2017 University of Tokyo, Japan Jun 2013 - Research leave at the LIGO Hanford Observatory Aug 2014 Commissioning the Advanced LIGO interferometer Aug 2010 - Assistant Professor of Physics May 2016 Syracuse University, Syracuse, NY Dec 2009 - NAOJ Visiting Researcher Aug 2010 National Astronomical Observatory of Japan. Sep 2009 - JSPS Postdoctoral Fellow (Gaikokujin Tokubetsu Kenkyuin) Nov 2009 National Astronomical Observatory of Japan. Jul 2006 - Robert A. Millikan Postdoctoral Fellow Aug 2009 California Institute of Technology, Pasadena, CA EDUCATION Jun 2006 Ph.D. Physics, Massachusetts Institute of Technology (MIT), Cambridge, MA Experimental Astrophysics, Laser Interferometer Gravitational Wave Observatory (LIGO). Apr 2000 Diploma (equivalent to Master of Science), Physics, Swiss Federal Institute of Technology (ETH) Zurich, Switzerland With honor, in Theoretical -
Joshua R. Smith
Joshua R. Smith The Nicholas and Lee Begovich Center for Gravitational-Wave Physics and Astronomy Department of Physics California State University Fullerton 800 N. State College Blvd. Fullerton, CA 92831 E-mail: [email protected] Phone: (657)-278-3716 Web: https://physics.fullerton.edu/∼josmith/ Appointments 2016– Dan Black Director of Gravitational-Wave Physics and Astronomy 2018– Professor of Physics 2014–2018 Associate Professor of Physics 2010–2014 Assistant Professor of Physics California State University Fullerton (CSUF) 2007–2009 Postdoctoral Research Associate in Physics Syracuse University 2006–2007 Postdoctoral Fellow in Physics Albert Einstein Institute Hannover / EGO-Virgo Education 2002–2006 Ph.D. Physics (Dr. rer. nat.), Leibniz Universitat¨ Hannover • Advisor: Karsten Danzmann • Thesis: “Formulation of Instrument Noise Analysis Techniques and Their Use in the Commissioning of the Gravitational Wave Observatory GEO 600” 1998–2002 B.Sc. Physics, Syracuse University • Advisor: Peter Saulson • Thesis: “Thermal Noise Associated with Silicate Bonding” Leadership 2012– Director, The Nicholas and Lee Begovich Center for Gravitational-Wave Physics and Astron- omy, CSUF 2019– Co-I, Cosmic Explorer Project, Member, Cosmic Explorer Consortium 2016–2017 Member, Executive Committee, APS Far West Section 2011–2015 Chair, Detector Characterization Group, LIGO Scientific Collaboration 2011–2015 Member, Executive Committee, LIGO Scientific Collaboration 2008– Member, Council, LIGO Scientific Collaboration 2008–2010 Co-chair, Glitch Working -
A Brief History of LIGO
A Brief History of LIGO One hundred years ago, using his recently formulated general relativity theory, Albert Einstein predicted the existence of gravitational waves and described their properties. To Einstein these waves seemed too weak ever to be detected, even for the strongest sources that he could conceive. Over the subsequent decades, our improving knowledge of the universe (black holes, neutron stars, supernovae …) and the march of technology (lasers, computers, solid state electronics, low loss optics….) have changed that. In the 1960s, Joseph Weber at the University of Maryland pioneered the effort to build detectors for gravitational waves, using large cylinders of aluminum that vibrate in response to a passing wave, an approach which broke the ground for the field of gravitational-wave searches. LIGO’s approach, using laser interferometry to monitor the relative motion of freely hanging mirrors, was proposed as a theoretical concept form in 1962 by Michael Gertsenshtein and Vladislav Pustovoit in Moscow Russia, and independently several years later by Weber and by Rainer Weiss in America. In 1967, Weiss investigated a laser interferometer limited at some frequencies by quantum shot noise, and in 1972 he completed the invention of the interferometric gravitational wave detector by identifying all the fundamental noise sources that such a detector must face, and conceiving ways to deal with each of them, and by showing that — at least in principle — these ways could lead to detector sensitivities good enough to detect waves from astrophysical sources. Prototype interferometric gravitational wave detectors (“interferometers”) were built in the late 1960s by Robert Forward and colleagues at Hughes Research Laboratories (with mirrors mounted on a vibration isolated plate rather than free swinging), and in the 1970s (with free swinging mirrors between which light bounced many times) by Weiss at MIT, and then by Hans Billing and colleagues in Garching Germany, and then by Ronald Drever, James Hough and colleagues in Glasgow Scotland.