Gravitational Waves
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Abstracts and Speaker Profiles
Project: Laser Interferometer Gravitational-Wave Observatory (LIGO) Dr. David Reitze, Executive Director, LIGO Laboratory The Gravitational Wave Astronomical Revolution: India's Emerging Role Abstract: • The past four years have witnessed a revolution in astronomy, enabled by the first detections of gravitational waves from colliding black holes and neutron stars through the direct observation of their gravitational wave emissions by the LIGO and Virgo observatories. These discoveries have profound implications for our understanding of the Universe. Gravitational waves provide unique information about nature's most energetic astrophysical events, revealing insights into the nature of gravity, matter, space, and time that are unobtainable by any other means. In this talk, I will briefly discuss how we detect gravitational waves, how gravitational-wave observatories will revolutionize astronomy in the coming years and decades, and how India is poised to play a key role in the future gravitational wave astronomy. About the Speaker: • David Reitze holds joint positions as the Executive Director of the LIGO Laboratory at the California Institute of Technology and as a Professor of Physics at the University of Florida. His research focuses on the development of gravitational-wave detectors. He received a B.A. in Physics with Honors from Northwestern Univ. and a Ph. D. in Physics from the University of Texas of Austin. He is a Fellow of the American Association for the Advancement of Science, the American Physical Society, and the Optical Society. and was jointly awarded the 2017 US National Academy of Sciences Award for Scientific Discovery for his leadership role in LIGO. He is a member of the international LIGO Scientific Collaboration that received numerous awards for the first direct detection of gravitational waves in 2015, including the Special Breakthrough Prize in Fundamental Physics, the Gruber Prize for Cosmology, the Princess Asturias Award for Scientific and Technical Achievement, and the American Astronomical Society Bruno Rossi Prize. -
TSR6908.MHR3.Avenger
AVENGERS CAMPAIGN FRANCHISES Avengers Branch Teams hero/heroine and the sponsoring nation, Table A: UN Proposed Avengers Bases For years, the Avengers operated avengers membership for national heroes and New Members relatively autonomously, as did the has become the latest political power chip Australia: Sydney; Talisman I Fantastic Four and other superhuman involved in United Nations negotiations. China: Moscow; Collective Man teams. As the complexities of crime Some member nations, such as the Egypt: Cairo; Scarlet Scarab fighting expanded and the activities of the representatives of the former Soviet France: Paris; Peregrine Avengers expanded to meet them, the Republics and their Peoples' Protectorate, Germany: Berlin; Blitzkrieg, Hauptmann team's needs changed. Their ties with have lobbied for whole teams of powered Deutschland local law enforcement forces and the beings to be admitted as affiliated Great Britain: Paris; Spitfire, Micromax, United States government developed into Avengers' branch teams. Shamrock having direct access to U.S. governmental The most prominent proposal nearing a Israel: Tel Aviv; Sabra and military information networks. The vote is the General Assembly's desired Japan: Undecided; Sunfire Avengers' special compensations (such as establishment of an Avengers' branch Korea: Undecided; Auric, Silver domestic use of super-sonic aircraft like team for the purpose of policing areas Saudi Arabia: Undecided; Arabian Knight their Quintets) were contingent on working outside of the American continent. This Soviet Republics: Moscow; Peoples' with the U.S. National Security Council. proposal has been welcomed by all Protectorate (Perun, Phantasma, Red After a number of years of tumultuous member nations except the United States, Guardian, Vostok) and Crimson Dynamo relations with the U.S. -
Acceptance Speech Kip S. Thorne
Ceremony of the Doctorate Honoris Causa Award to Prof. Kip S. Thorne Universitat Politècnica de Catalunya•BarcelonaTech (UPC). 25th May 2017. Acceptance Speech Kip S. Thorne Thank you, Enrique, for your much too generous description of me and my contributions to science. This honorary doctorate from the Universitat Politècnica de Catalunya is of great significance to me. It honors, especially, my contributions to LIGO’s discovery of gravitational waves. For this reason, I regard myself as sharing it with the large team of scientists and engineers, whose contributions were essential to our discovery. There are only two types of waves that bring us information about the universe: electromagnetic waves and gravitational waves. They travel at the same speed, but aside from this, they could not be more different. Electromagnetic waves—which include light, infrared waves, microwaves, radio waves, ultraviolet waves, X-rays and gamma rays— these are all oscillations of electric and magnetic fields that travel through space and time. Gravitational waves are oscillations in the fabric of space and time. Galileo Galilei opened up electromagnetic astronomy 400 years ago, when he built a small optical telescope, turned it on the sky, and discovered the four largest moons of Jupiter. We LIGO scientists opened up gravitational astronomy in 2015 when our complex detectors discovered gravitational waves from two colliding black holes, a billion light years from Earth. The efforts that produced these two discoveries could not have been more different. Galileo made his discovery alone, though he built on ideas and technology of others. We LIGO scientists made our discovery through a tight collaboration of more than 1000 scientists and engineers. -
The Future of Ground-Based Gravitational-Wave Detectors
Penn State Theory Seminar, March 2, 2018 The Future of Ground-based Gravitational-wave Detectors David Reitze LIGO Laboratory California Institute of Technology LIGO-G1800292-v1 LIGO Hanford Observatory LIGO-G1800292 Outline ● Why Make Bigger and Better Detectors? ● Improving Advanced LIGO: A+ ● Exploiting the Existing LIGO Facility Limits: Voyager ● Future ‘3G’ Facilities: Cosmic Explorer and Einstein Telescope 2 LIGO-G1800292 Some of the Questions That Gravitational Waves Can Answer ● Outstanding Questions in Fundamental Physics Black Hole Merger and Ringdown » Is General Relativity the correct theory of gravity? » How does matter behave under extreme conditions? » No Hair Theorem: Are black holes truly bald? ● Outstanding Questions in Astrophysics, Astronomy, Cosmology Image credit: W. Benger » Do compact binary mergers cause GRBs? » What is the supernova mechanism in core-collapse of massive Neutron Star Formation stars? » How many low mass black holes are there in the universe? » Do intermediate mass black holes exist? » How bumpy are neutron stars? » Can we observe populations of weak gravitational wave Image credit: NASA sources? » Can binary inspirals be used as “standard sirens” to measure GW Upper limit map the local Hubble parameter? » Are LIGO/Virgo’s binary black holes a component of Dark Matter? » Do Cosmic Strings Exist? Credit: LIGO Scientific Collaboration3 LIGO-G1800292 LIGO-G1800292 Observing Plans for the Coming 5 Years NOW Abbott, et al., “Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced -
LIGO SCIENTIFIC COLLABORATION LIGO Scientific Collaboration
LIGO SCIENTIFIC COLLABORATION Document Type LIGO-M-1900084 LIGO Scientific Collaboration Program 2019-2020 The LSC Program Committee: Gabriela Gonzalez,´ Stephen Fairhurst, P. Ajith, Patrick Brady, Alessandra Buonanno, Alessandra Corsi, Peter Fritschel, Bala Iyer, Joey Key, Sergey Klimenko, Brian Lantz, Albert Lazzarini, David McClelland, David Reitze, Keith Riles, Sheila Rowan, Alicia Sintes, Josh Smith WWW: http://www.ligo.org/ Processed with LATEX on 2019/05/30 LIGO Scientific Collaboration Program 2019-2020 Contents 1 Overview 3 1.1 The LIGO Scientific Collaboration’s Scientific Mission . .3 1.2 LSC Science Goals: Gravitational Wave Targets . .4 1.3 LSC Science Goals: Gravitational Wave Astronomy . .5 2 LIGO Scientific Operations and Scientific Results 7 2.1 LIGO Observatory Operations . .7 2.2 LSC Detector Commissioning and Detector Improvement activities . .8 2.3 Detector Calibration and Data Timing . .8 2.4 Operating computing systems and services for modeling, analysis, and interpretation . .9 2.5 Detector Characterization . 10 2.6 The operations of data analysis search, simulation and interpretation pipelines . 10 2.7 LSC Fellows Program . 11 2.8 Development of data analysis tools to search and interpret the gravitational wave data . 12 2.9 Dissemination of LIGO data and scientific results . 13 2.10 Outreach to the public and the scientific community . 14 2.11 A+ Upgrade Project . 15 2.12 LIGO-India . 15 2.13 Roles in LSC organization . 15 3 Advancing frontiers of Gravitational-Wave Astrophysics, Astronomy and Fundamental Physics: Improved Gravitational Wave Detectors 17 3.1 Substrates . 17 3.2 Suspensions and seismic isolation . 18 3.3 Optical Coatings . 18 3.4 Cryogenics . -
Making Waves in Spacetime 22 July 2016, by Barbara K
Making waves in spacetime 22 July 2016, by Barbara K. Kennedy This gravity-driven merger warped space and sent waves speeding outward, making ripples in the fabric of spacetime. Before the first indication by LIGO, these waves had not ever been detected on Earth. "We now have far more confidence that mergers of two black holes are common in the nearby universe," Hanna said. "Now that we are able to detect gravitational waves, they are going to be a phenomenal source of new information about our galaxy and an entirely new channel for discoveries about the universe." Credit: Michelle Bixby Physicists have concluded that the newly detected gravitational-wave event was produced during the final moments of the merger of two black holes Waves on Earth's oceans move in endless rhythm whose masses were notably smaller than the along sandy beaches. Another kind of wave ripples masses of the black holes whose merger produced to our planet from distant black holes in the LIGO's first detection. This new merger united black universe. holes with masses 14 and 8 times the mass of the sun, producing a spinning black hole that is 21 Less than four months after the historic first-ever times the mass of the sun. detection of gravitational waves, scientists on a team that includes Penn State physicists and "It is very significant that these black holes were astronomers detected another gravitational wave much less massive than those in the first washing over the Earth. detection," said Gabriela Gonzalez, professor of physics and astronomy at Louisiana State "I would never have guessed that we would be so University, spokesperson of the international LIGO fortunate to have not only one, but two definitive Scientific Collaboration (LSC), and a former binary black-hole detections within the first few assistant professor of physics at Penn State. -
Program 2020 – 21
LIGO-M2000130 PROGRAM 2020 – 21 Image credit: LIGO/Sonoma State University/A. Simonnet LIGO SCIENTIFIC COLLABORATION Document Type LIGO-M2000130-v3 LIGO Scientific Collaboration Program 2020–2021 The LSC Program Committee: Stephen Fairhurst, Stefan Ballmer, P. Ajith, Christopher Berry, Sukanta Bose, Patrick Brady, Alessandra Buonanno, Joey Shapiro Key, Sergey Klimenko, Brian Lantz, Albert Lazzarini, David Ottaway, David Reitze, Sheila Rowan, Jax Sanders, Alicia M. Sintes, Josh Smith WWW: http://www.ligo.org/ Processed with LATEX on 2020/07/08 LIGO Scientific Collaboration Program 2020–2021 Contents 1 Overview 3 1.1 The LIGO Scientific Collaboration’s Scientific Mission . .3 1.2 LSC Science Goals: Gravitational Wave Targets . .4 1.3 LSC Science Goals: Gravitational Wave Astronomy . .5 2 LIGO Scientific Operations and Scientific Results 7 2.1 Observatory Operations . .7 2.2 Detector Commissioning and Detector Improvement activities . .8 2.3 LSC Fellows Program . .9 2.4 Detector Calibration and Data Timing . .9 2.5 Operating computing systems and services for modeling, analysis, and interpretation . 10 2.6 Detector Characterization . 11 2.7 The operations of data analysis search, simulation and interpretation pipelines . 12 2.8 Deliver data analysis tools to search and interpret the gravitational wave data . 13 2.9 Dissemination of LIGO data and scientific results . 14 2.10 Outreach to the public and the scientific community . 16 2.11 A+ Upgrade Project . 17 2.12 LIGO-India . 17 2.13 Post-A+ planning . 18 2.14 Roles in LSC organization . 18 3 Advancing frontiers of Gravitational-Wave Astrophysics, Astronomy and Fundamental Physics: Improved Gravitational Wave Detectors 19 3.1 Substrates . -
Future Ground-Based Gravitational-Wave Observatories: Synergies with Other Scientific Communities
Future Ground-Based Gravitational-Wave Observatories: Synergies with Other Scientific Communities GWIC April 2021 COMMUNITY NETWORKING SUBCOMMTTEE Michele Punturo, INFN - Perugia, Italy (Co-chair) David Reitze, Caltech, USA (Co-chair) David Shoemaker, MIT, USA STEERING COMMITTEE Michele Punturo, INFN - Perugia, Italy (Co-chair) David Reitze, Caltech, USA (Co-chair) Peter Couvares, Caltech, USA Stavros Katsanevas, European Gravitational Observatory, Italy Takaaki Kajita, University of Tokyo, Japan Vicky Kalogera, Northwestern University, USA Harald Lueck, Albert Einstein Institute, Germany David McClelland, Australian National University, Australia Sheila Rowan, University of Glasgow, UK Gary Sanders, Caltech, USA B.S. Sathyaprakash, Penn State University, USA and Cardiff University, UK David Shoemaker, MIT, USA (Secretary) Jo van den Brand, Nikhef, Netherlands GRAVITATIONAL WAVE INTERNATIONAL COMMITTEE This document was produced by the GWIC 3G Subcommittee and the GWIC 3G Synergies with Scientific Communities Subcommittee Final release, April 2021 Cover: LIGO/Caltech/MIT/Sonoma State (Aurore Simonnet) Contents 1 Introduction ........................................................1 2 Constituencies & Affiliated Communities .......................2 3 Engaging with Constituencies & Communities .................7 4 Summary of Recommendations ................................ 11 1. Introduction Planning for the development of a 3rd generation global gravitational-wave detector array is a multifaceted and complex effort that will necessarily need a high level of community input. Interfacing to extant and new stakeholders in the broader scientific constituencies is absolutely necessary to, first, keep them aware of the activities taking place in the ground-based gravitational-wave community and, second, receive input to inform and evolve the planning. The Community Networking Subcommittee within the GWIC 3G Planning Committee is charged with organizing and facilitating communications between 3rd generation projects and the relevant scientific communities. -
Visiting Associate, California Institute of Technology Maître De Recherche
November 2014 DAVID HOWARD REITZE Address LIGO Laboratory California Institute of Technology MS 100-36 1200 E. California Avenue Pasadena, CA 91125 Telephone (626) 395-6274 (office); (626) 395-2763 (fax) E-mail [email protected] PROFESSIONAL APPOINTMENTS August 2011-Present Executive Director, LIGO Laboratory California Institute of Technology, Pasadena, CA August 2003-Present Professor of Physics (on long term leave) The University of Florida, Gainesville, FL August 1998-August 2003 Associate Professor of Physics The University of Florida, Gainesville, FL August 1993-July 1998 Assistant Professor of Physics The University of Florida, Gainesville, FL November 1992- August 1993 Physicist, Ultrashort Pulse Laser Group, L Division Lawrence Livermore National Laboratory, Livermore, CA October 1990- October 1992 Postdoctoral Member of Technical Staff Bell Communications Research (Bellcore), Red Bank, NJ AFFILIATE APPOINTMENTS 1996, 2000, 2007-2011 Visiting Associate, California Institute of Technology 2001, 2008 Maître de Recherche, Laboratoire d’Optique Appliquée, Palaiseau, France EDUCATION September 1983 Ph. D. in Physics - December 1990 The University of Texas at Austin, Austin, TX Thesis Advisor: Michael Downer, Professor of Physics Thesis Title: Femtosecond Melting Dynamics in Silicon and Carbon September 1979 B. A. in Physics - June 1983 Northwestern University, Evanston, IL HONORS, AWARDS, SERVICE 2015 Fellow, Optical Society of America (OSA) 2014-present Member, National Research Council Committee on Atomic, Molecular, and Optical -
National Science Foundation LIGO BIOS
BIOS France Córdova is 14th director of the National Science Foundation. Córdova leads the only government agency charged with advancing all fields of scientific discovery, technological innovation, and STEM education. Córdova has a distinguished resume, including: chair of the Smithsonian Institution’s Board of Regents; president emerita of Purdue University; chancellor of the University of California, Riverside; vice chancellor for research at the University of California, Santa Barbara; NASA’s chief scientist; head of the astronomy and astrophysics department at Penn State; and deputy group leader at Los Alamos National Laboratory. She received her B.A. from Stanford University and her Ph.D. in physics from the California Institute of Technology. Gabriela González is spokesperson for the LIGO Scientific Collaboration. She completed her PhD at Syracuse University in 1995, then worked as a staff scientist in the LIGO group at MIT until 1997, when she joined the faculty at Penn State. In 2001, she joined the faculty at Louisiana State University, where she is a professor of physics and astronomy. The González group’s current research focuses on characterization of the LIGO detector noise, detector calibration, and searching for gravitational waves in the data. In 2007, she was elected a fellow of the American Physical Society for her experimental contributions to the field of gravitational wave detection, her leadership in the analysis of LIGO data for gravitational wave signals, and for her skill in communicating the excitement of physics to students and the public. David Reitze is executive director of the LIGO Laboratory at Caltech. In 1990, he completed his PhD at the University of Texas, Austin, where his research focused on ultrafast laser-matter interactions. -
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 -
Extensions of Remarks E1424 HON. BILL FOSTER HON. BILL FLORES
E1424 CONGRESSIONAL RECORD — Extensions of Remarks September 16, 2014 these institutions can continue serving Amer- rest of the Chamber Board for their leadership ship from Rollins College, Crummer Graduate ican consumers. and dedication to our community. I would also School of Business. In addition, H.R. 5461 incorporates three like to recognize and thank Russ Slinkard, the I am honored to recognize Julio Rocha, dur- other bills that originated in the Financial Serv- President and Chief Executive Officer of the ing Hispanic Heritage Month, for his leader- ices Committee and previously received over- Joliet Region Chamber of Commerce and In- ship and contributions to the Central Florida whelming bipartisan support: H.R. 634, the dustry, and all of the staff. Community. Business Mitigation and Price Stabilization The Joliet Region Chamber of Commerce f Act; H.R. 3211, the Mortgage Choice Act; and and Industry has been a partner to the city as H.R. 4167, the Restoring Proven Financing for it has grown and changed over the past 100 HONORING JAMISON DUNN American Employees Act. years. The Chamber plays a vital role in the In this time when there seems to be so little economic health of Joliet and the surrounding HON. SAM GRAVES that Republicans and Democrats in Wash- area. OF MISSOURI ington agree on, I think it’s important to note Again, I would like to congratulate the Joliet IN THE HOUSE OF REPRESENTATIVES just how much bipartisan support all of these Region Chamber of Commerce and Industry Tuesday, September 16, 2014 bills earned. for 100 years of service to our community.