LIGO Present and Future. Barry Barish Directory of the LIGO Laboratory
|
|
- Cecilia Lewis
- 5 years ago
- Views:
Transcription
1 LIGO Present and Future Barry Barish Directory of the LIGO Laboratory
2 LIGO I Schedule and Plan LIGO I has been built by LIGO Lab (Caltech & MIT) 1996 Construction Underway (mostly civil) 1997 Facility Construction (vacuum system) 1998 Interferometer Construction (complete facilities) 1999 Construction Complete (interferometers in vacuum) 2000 Detector Installation (commissioning subsystems) 2001 Commission Interferometers (first coincidences) 2002 Sensitivity studies (initiate LIGO I Science Run) LIGO I data run (one year integrated data at h ~ ) Begin Advanced LIGO installation 2
3 LIGO Scientific Collaboration March 02 LSC Institutional Membership 35 institutions > 350 collaborators University of Adelaide ACIGA Australian National University ACIGA California State Dominquez Hills Caltech LIGO Caltech Experimental Gravitation CEGG Caltech Theory CART University of Cardiff GEO Carleton College Cornell University University of Gainesville Glasgow University GEO University of Hannover GEO Harvard-Smithsonian India-IUCAA IAP Nizhny Novgorod Iowa State University Joint Institute of Laboratory Astrophysics LIGO Livingston LIGOLA LIGO Hanford LIGOWA Louisiana State University Louisiana Tech University MIT LIGO Max Planck (Garching) GEO Max Planck (Potsdam) GEO University of Michigan Moscow State University NAOJ - TAMA University of Oregon Pennsylvania State University Exp Pennsylvania State University Theory Southern University Stanford University University of Texas@Brownsville University of Western Australia ACIGA University of Wisconsin@Milwaukee International India, Russia, Germany, U.K, Japan and Australia. The international partners are involved in all aspects of the LIGO research program. 3
4 LIGO Sites Hanford Observatory Livingston Observatory 4
5 LIGO Livingston Observatory 5
6 LIGO Hanford Observatory 6
7 Coincidences between the LIGO Sites! Two Sites Three interferometers! Single interferometer non-gaussian level ~50/hour! Local coincidence - Hanford 2K and 4K ( ~1000) ~1/day! Hanford/Livingston coincidence (uncorrelated) <0.1/yr! GEO coincidence further reduces the false signal rate! Data (continuous time-frequency record)! Gravitational wave signal 0.2MB/sec! Total data recorded 16 MB/sec! Gravitational Wave Signal Extraction! Signal from noise (noise analysis, vetoes, coincidences, etc 7
8 LIGO Facility Noise Levels! Fundamental Noise Sources! Seismic at low frequencies! Thermal at mid frequencies! Shot at high frequencies! Facility Noise Sources (example)! Residual Gas! 10-6 torr H 2 unbaked! 10-9 torr H 2 baked 8
9 Beam Pipe and Enclosure! Minimal Enclosure (no services)! Beam Pipe! 1.2m diam; 3 mm stainless! 65 ft spiral weld sections! 50 km of weld (NO LEAKS!) 9
10 Baking out the LIGO Beam Pipe insulation ~ 2000 amps for one month Fermilab Magnet Power Supply 10
11 Vacuum Chambers and Seismic Isolation Vacuum Chambers constrained layer damped springs Vacuum Chamber Gate Valve passive isolation 11
12 LIGO I Suspension and Optics Single suspension 0.31mm music wire fused silica Surface figure = λ/ 6000 surface uniformity < 1nm rms scatter < 50 ppm absorption < 2 ppm internal Q s >
13 Commissioning the LIGO I Subsystems stablization Tidal 10-Watt Laser Wideband 15 m 4 km PSL IO Interferometer 10-1 Hz/Hz 1/ Hz/Hz 1/ Hz/Hz 1/2 Nd:Yag mm Output power >8 Watt TEM00 mode LIGO I Goal 13
14 LIGO Prestablized Laser Data vs Simulation 14
15 LIGO I Interferometer Configuration Requires test masses to be held in position to meter: Locking the interferometer end test mass Light bounces back and forth along arms about 150 times Light is recycled about 50 times input test mass Laser signal 15
16 Locking the LIGO I Interferometers One meter, about 40 inches 10, , ,000 1,000 Human Earthtides, hair, about 100 microns Wavelength Microseismic of motion, light, about 1 1 micron Atomic Precision diameter, required 10to -10 lock, meterabout meter Nuclear diameter, meter LIGO sensitivity, meter 16
17 Watching LIGO Lock Composite Video Y Arm Laser signal X Arm 17
18 Watching an Early Lock Y arm X arm 2 min Y Arm Reflected light Anti-symmetric port Laser signal X Arm 18
19 Lock Acquisition LIGO I Dynamical Control Model by Matt Evans Caltech 19
20 LIGO Engineering Run (E7) Sensitivities Final LIGO Milestone Coincidences Between the Sites in 2001 Engineering Run 28 Dec 01 to 14 Jan 02 20
21 LIGO + GEO Interferometers 28 Dec Jan 2002 (402 hr) Singles data All segments Segments >15min L1 locked 284hrs (71%) 249hrs (62%) L1 clean 265hrs (61%) 231hrs (53%) L1 longest clean segment: 3:58 H1 locked 294hrs (72%) 231hrs (57%) H1 clean 267hrs (62%) 206hrs (48%) H1 longest clean segment: 4:04 H2 locked 214hrs (53%) 157hrs (39%) H2 clean 162hrs (38%) 125hrs (28%) H2 longest clean segment: 7:24 Coincidence Data All segments Segments >15min 2X: H2, L1 locked 160hrs (39%) 99hrs (24%) clean 113hrs (26%) 70hrs (16%) H2,L1 longest clean segment: 1:50 3X : L1+H1+ H2 locked 140hrs (35%) 72hrs (18%) clean 93hrs (21%) 46hrs (11%) L1+H1+ H2 : longest clean segment: 1:18 4X: L1+H1+ H2 +GEO: 77 hrs (23 %) 26.1 hrs (7.81 %) 5X: ALLEGRO + Conclusion: Large Duty Cycle Looks Attainable 21
22 LIGO Sensitivity History Hanford 2K Livingston 4K
23 LIGO I Astrophysical Sources Search Efforts! Compact binary inspiral: chirps! NS-NS waveforms are well described! BH-BH need better waveforms! search technique: matched templates! Supernovae / GRBs: bursts! burst signals in coincidence with signals in electromagnetic radiation! prompt alarm (~ one hour) with neutrino detectors! Pulsars in our galaxy: periodic! search for observed neutron stars (frequency, doppler shift)! all sky search (computing challenge)! r-modes! Cosmological Signals stochastic background 23
24 Stochastic Background Sensitivity! Detection! Cross correlate Hanford and Livingston Interferometers! Good Sensitivity! GW wavelength 2x detector baseline f 40 Hz! Initial LIGO Sensitivity Ω 10-5! Advanced LIGO Sensitivity Ω
25 Stochastic Background Coherence Plots 25
26 Stochastic Background Sensitivities 26
27 LIGO I Status and Plans! LIGO construction complete! LIGO commissioning and testing on track! Engineering test runs underway, during period when emphasis is on commissioning, detector sensitivity and reliability. (Short upper limit data runs interleaved)! First Science Search Run : first search run will begin during 2003; goal is to obtain and analyze one year of integrated data at h ~ by 2006! Significant improvements in sensitivity anticipated to begin about
28 Advanced LIGO Status and Plans! GEO, ACIGA and LIGO form a very strong international partnership to develop and manage Advanced LIGO! Working toward NSF construction proposal to be submitted in Fall 2002! Advanced R&D program is proceeding well! Baseline design and installation scenarios established (alternative carried)! Bottoms-up costing has nearly been completed! Plan assumes long lead funds available in 2004; major construction funds in 2005! Supports an installation by
LIGO Update
LIGO Update ------------ The Search for Gravitational Waves Barry Barish Caltech Trustees 10-Sept-02 ! Goals Laser Interferometer Gravitational-wave Observatory» First direct detection of gravitational
More informationLIGO Status and Plans. Barry Barish / Gary Sanders 13-May-02
LIGO Status and Plans Barry Barish / Gary Sanders 13-May-02 LIGO overall strategy! Strategy presented to NSB by Thorne / Barish in 1994! Search with a first generation interferometer where detection of
More informationStatus of LIGO. David Shoemaker LISA Symposium 13 July 2004 LIGO-G M
Status of LIGO David Shoemaker LISA Symposium 13 July 2004 Ground-based interferometric gravitational-wave detectors Search for GWs above lower frequency limit imposed by gravity gradients» Might go as
More informationStatus and Prospects for LIGO
Status and Prospects for LIGO Crab Pulsar St Thomas, Virgin Islands Barry C. Barish Caltech 17-March-06 LIGO Livingston, Louisiana 4 km 17-March-06 Confronting Gravity - St Thomas 2 LIGO Hanford Washington
More informationGravity -- Studying the Fabric of the Universe
Gravity -- Studying the Fabric of the Universe Barry C. Barish Caltech "Colliding Black Holes" Credit: National Center for Supercomputing Applications (NCSA) AAAS Annual Meeting Denver, Colorado 17-Feb-03
More informationLaser Interferometer Gravitationalwave Observatory LIGO Industrial Physics Forum. Barry Barish 7 November 2000 LIGO-G9900XX-00-M
Laser Interferometer Gravitationalwave Observatory LIGO 2000 Industrial Physics Forum Barry Barish 7 November 2000 Sir Isaac Newton Perhaps the most important scientist of all time! Invented the scientific
More informationDiscovery of Gravita/onal Waves
Discovery of Gravita/onal Waves Avto Kharchilava QuarkNet Workshop, August 2016 https://www.ligo.caltech.edu/news/ligo20160211 Gravity Einstein s General theory of relativity: Gravity is a manifestation
More informationProbing for Gravitational Waves
Probing for Gravitational Waves LIGO Reach with LIGO AdLIGO Initial LIGO Barry C. Barish Caltech YKIS2005 Kyoto University 1-July-05 Einstein s Theory of Gravitation a necessary consequence of Special
More informationLIGO and the Search for Gravitational Waves
LIGO and the Search for Gravitational Waves Barry Barish Caltech Princeton University 2-May-02 Einstein s Theory of Gravitation Newton s Theory instantaneous action at a distance Einstein s Theory information
More informationThe LIGO Experiment Present and Future
The LIGO Experiment Present and Future Keith Riles University of Michigan For the LIGO Scientific Collaboration APS Meeting Denver May 1 4, 2004 LIGO-G040239-00-Z What are Gravitational Waves? Gravitational
More informationLIGO: The Laser Interferometer Gravitational Wave Observatory
LIGO: The Laser Interferometer Gravitational Wave Observatory Credit: Werner Benger/ZIB/AEI/CCT-LSU Michael Landry LIGO Hanford Observatory/Caltech for the LIGO Scientific Collaboration (LSC) http://www.ligo.org
More informationGravitational Waves and LIGO
Gravitational Waves and LIGO Ray Frey, University of Oregon 1. GW Physics and Astrophysics 2. How to detect GWs The experimental challenge 3. Prospects June 16, 2004 R. Frey QNet 1 General Relativity Some
More informationLIGO and the Search for Gravitational Waves
LIGO and the Search for Gravitational Waves Barry Barish University of Toronto 26-March-02 Sir Isaac Newton Universal Gravitation! Three laws of motion and law of gravitation (centripetal force) disparate
More informationLIGO Status and Advanced LIGO Plans. Barry C Barish OSTP 1-Dec-04
LIGO Status and Advanced LIGO Plans Barry C Barish OSTP 1-Dec-04 Science Goals Physics» Direct verification of the most relativistic prediction of general relativity» Detailed tests of properties of gravitational
More informationLong-term strategy on gravitational wave detection from European groups
Longterm strategy on gravitational wave detection from European groups Barry Barish APPEC Meeting London, UK 29Jan04 International Interferometer Network Simultaneously detect signal (within msec) LIGO
More informationGravitationswellen. Wirkung auf Punktmassen. für astrophysikalische Quellen h ~ h L L
G-Wellendetektoren Gravitationswellen Wirkung auf Punktmassen h L L für astrophysikalische Quellen h ~ 10-22 - 10-21 Chirp Signal We can use weak-field gravitational waves to study strong-field general
More informationLIGO and the Quest for Gravitational Waves
LIGO and the Quest for Gravitational Waves "Colliding Black Holes" Credit: National Center for Supercomputing Applications (NCSA) LIGO-G030523-00-M Barry C. Barish Caltech UT Austin 24-Sept-03 1 A Conceptual
More informationProbing the Universe for Gravitational Waves
Probing the Universe for Gravitational Waves "Colliding Black Holes" Credit: National Center for Supercomputing Applications (NCSA) Barry C. Barish Caltech Argonne National Laboratory 16-Jan-04 LIGO-G030523-00-M
More informationProbing the Universe for Gravitational Waves
Probing the Universe for Gravitational Waves Barry C. Barish Caltech Crab Pulsar Georgia Tech 26-April-06 General Relativity the essential idea G μν = 8πΤ μν Gravity is not a force, but a property of space
More informationThe Search for Gravitational Waves
The Search for Gravitational Waves Barry Barish Caltech University of Iowa 16-Sept-02 Newton Universal Gravitation! Three laws of motion and law of gravitation (centripetal force) disparate phenomena»
More informationLIGO: On the Threshold of Gravitational-wave Astronomy
LIGO: On the Threshold of Gravitational-wave Astronomy Stan Whitcomb LIGO/Caltech IIT, Kanpur 18 December 2011 Outline of Talk Quick Review of GW Physics and Astrophysics LIGO Overview» Initial Detectors»
More information6WDWXVRI/,*2. Laser Interferometer Gravitational-wave Observatory. Nergis Mavalvala MIT IAU214, August 2002 LIGO-G D
6WDWXVRI/,*2 Laser Interferometer Gravitational-wave Observatory Hanford, WA Livingston, LA Nergis Mavalvala MIT IAU214, August 2002 *UDYLWDWLRQDOZDYH,QWHUIHURPHWHUVWKHSULQ LSOH General Relativity (Einstein
More informationThe LIGO Project: a Status Report
The LIGO Project: a Status Report LIGO Hanford Observatory LIGO Livingston Observatory Laura Cadonati LIGO Laboratory, MIT for the LIGO Scientific Collaboration Conference on Gravitational Wave Sources
More informationAdvanced LIGO, LIGO-Australia and the International Network
Advanced LIGO, LIGO-Australia and the International Network Stan Whitcomb LIGO/Caltech IndIGO - ACIGA meeting on LIGO-Australia 8 February 2011 Gravitational Waves Einstein in 1916 and 1918 recognized
More informationGravitational Wave Detection from the Ground Up
Gravitational Wave Detection from the Ground Up Peter Shawhan (University of Maryland) for the LIGO Scientific Collaboration LIGO-G080393-00-Z From Simple Beginnings Joe Weber circa 1969 AIP Emilio Segre
More informationOverview Ground-based Interferometers. Barry Barish Caltech Amaldi-6 20-June-05
Overview Ground-based Interferometers Barry Barish Caltech Amaldi-6 20-June-05 TAMA Japan 300m Interferometer Detectors LIGO Louisiana 4000m Virgo Italy 3000m AIGO Australia future GEO Germany 600m LIGO
More informationAdvanced LIGO, Advanced VIRGO and KAGRA: Precision Measurement for Astronomy. Stefan Ballmer For the LVC Miami 2012 Dec 18, 2012 LIGO-G
Advanced LIGO, Advanced VIRGO and KAGRA: Precision Measurement for Astronomy Stefan Ballmer For the LVC Miami 2012 Dec 18, 2012 LIGO-G1201293 Outline Introduction: What are Gravitational Waves? The brief
More informationLIGO and Detection of Gravitational Waves Barry Barish 14 September 2000
LIGO and Detection of Gravitational Waves Barry Barish 14 September 2000 Einstein s Theory of Gravitation Newton s Theory instantaneous action at a distance Einstein s Theory information carried by gravitational
More informationThe Status of Enhanced LIGO.
The Status of Enhanced LIGO. Aidan Brooks. December 2008 AIP Congress 2008, Adelaide, Australia 1 Outline Gravitational Waves» Potential sources» Initial LIGO interferometer Enhanced LIGO upgrades» Increased
More informationThe Quest to Detect Gravitational Waves
The Quest to Detect Gravitational Waves Peter Shawhan California Institute of Technology / LIGO Laboratory What Physicists Do lecture Sonoma State University March 8, 2004 LIGO-G040055-00-E Outline Different
More informationProbing the Universe for Gravitational Waves
Probing the Universe for Gravitational Waves Barry C. Barish Caltech Crab Pulsar University of Illinois 16-Feb-06 General Relativity the essential idea G μν = 8πΤ μν Gravity is not a force, but a property
More informationGravitational Wave Astronomy
Gravitational Wave Astronomy Giles Hammond SUPA, University of Glasgow, UK on behalf of the LIGO Scientific Collaboration and the Virgo Collaboration 14 th Lomonosov conference on Elementary Particle Physics
More informationProspects for joint transient searches with LOFAR and the LSC/Virgo gravitational wave interferometers
Prospects for joint transient searches with LOFAR and the LSC/Virgo gravitational wave interferometers Ed Daw - University of Sheffield On behalf of the LIGO Scientific Collaboration and the Virgo collaboration
More informationSearching for gravitational waves. with LIGO detectors
Werner Berger, ZIB, AEI, CCT Searching for gravitational waves LIGO Hanford with LIGO detectors Gabriela González Louisiana State University On behalf of the LIGO Scientific Collaboration KITP Colloquium,
More informationLIGO I status and advanced LIGO proposal
LIGO I status and advanced LIGO proposal Hiro Yamamoto LIGO Lab / Caltech LIGO I» basic design» current status advanced LIGO» outline of the proposal» technical issues GW signals and data analysis ICRR
More informationDevelopment of ground based laser interferometers for the detection of gravitational waves
Development of ground based laser interferometers for the detection of gravitational waves Rahul Kumar ICRR, The University of Tokyo, 7 th March 2014 1 Outline 1. Gravitational waves, nature & their sources
More informationState of LIGO. Barry Barish. S1 sensitivities. LSC Meeting LLO Hanford, WA 10-Nov GEO -- L 2km -- H 4km -- L 4km LIGO-G M
S1 sensitivities -- GEO -- L 2km -- H 4km -- L 4km State of h 0 LIGO Barry Barish LSC Meeting LLO Hanford, WA 10-Nov-03 Goals and Priorities LSC -Aug 02 Interferometer performance» Integrate commissioning
More informationGravitational Wave Detectors: Back to the Future
Gravitational Wave Detectors: Back to the Future Raffaele Flaminio National Astronomical Observatory of Japan University of Tokyo, March 12th, 2017 1 Summary Short introduction to gravitational waves (GW)
More informationThe Present Gravitational Wave Detection Effort
The Present Gravitational Wave Detection Effort Keith Riles University of Michigan LIGO Scientific Collaboration International Conference on Topics in Astroparticle and Underground Physics Rome July 1,
More informationThe Detection of Gravitational Waves with LIGO. Barry C. Barish. California Institute of Technology, Pasadena, CA 91125
The Detection of Gravitational Waves with LIGO Barry C. Barish California Institute of Technology, Pasadena, CA 91125 Gravitational wave emission is expected to arise from a variety of astrophysical phenomena.
More informationGearing up for Gravitational Waves: the Status of Building LIGO
Gearing up for Gravitational Waves: the Status of Building LIGO Frederick J. Raab, LIGO Hanford Observatory LIGO s Mission is to Open a New Portal on the Universe In 1609 Galileo viewed the sky through
More informationThe Laser Interferometer Gravitational-Wave Observatory In Operation
The Laser Interferometer Gravitational-Wave Observatory In Operation "Colliding Black Holes" Credit: National Center for Supercomputing Applications (NCSA) Reported on behalf of LIGO colleagues by Fred
More informationPresent and Future. Nergis Mavalvala October 09, 2002
Gravitational-wave Detection with Interferometers Present and Future Nergis Mavalvala October 09, 2002 1 Interferometric Detectors Worldwide LIGO TAMA LISA LIGO VIRGO GEO 2 Global network of detectors
More informationAdvanced LIGO Status Report
Advanced LIGO Status Report Gregory Harry LIGO/MIT On behalf of the LIGO Science Collaboration 22 September 2005 ESF PESC Exploratory Workshop Perugia Italy LIGO-G050477 G050477-00-R Advanced LIGO Overview
More informationThe Advanced LIGO detectors at the beginning of the new gravitational wave era
The Advanced LIGO detectors at the beginning of the new gravitational wave era Lisa Barsotti MIT Kavli Institute LIGO Laboratory on behalf of the LIGO Scientific Collaboration LIGO Document G1600324 LIGO
More informationGravitational Waves. Kip S. Thorne Bethe Centenial Symposium on Astrophysics Cornell University 3 June, 2006
Gravitational Waves Kip S. Thorne Bethe Centenial Symposium on Astrophysics Cornell University 3 June, 2006 INTRODUCTION The Warped Side of the Universe & Gravitational Waves 2 Black Hole: Made of Warped
More informationNext Generation Interferometers
Next Generation Interferometers TeV 06 Madison Rana Adhikari Caltech 1 Advanced LIGO LIGO mission: detect gravitational waves and initiate GW astronomy Next detector» Should have assured detectability
More informationNonequilibrium issues in macroscopic experiments
Nonequilibrium issues in macroscopic experiments L. Conti, M. Bonaldi, L. Rondoni www.rarenoise.lnl.infn.it European Research Council Gravitational Wave detector Motivation: GWs will provide new and unique
More information+56'0+0)614#8+6#6+10#.#8'5U +056'+0510).+0'5(41/6*'0+8'45' Barry C. Barish
+56'0+0)614#8+6#6+10#.#8'5U +056'+0510).+0'5(41/6*'0+8'45' Barry C. Barish .$'46 +056'+0 +45##%'9610 Perhaps the most important scientist of all time! Invented the scientific method in Principia Greatest
More informationSearching for Stochastic Gravitational Wave Background with LIGO
Searching for Stochastic Gravitational Wave Background with LIGO Vuk Mandic University of Minnesota 09/21/07 Outline LIGO Experiment:» Overview» Status» Future upgrades Stochastic background of gravitational
More informationLIGOʼs first detection of gravitational waves and the development of KAGRA
LIGOʼs first detection of gravitational waves and the development of KAGRA KMI2017 Jan. 2017 Tokyo Institute of Technology Kentaro Somiya Self Introduction Applied Physics (U Tokyo) NAOJ 2000-04 Albert-Einstein
More informationCollaborating on Mega Science Facilities
Collaborating on Mega Science Facilities Barry Barish Caltech LIGO Livingston, Louisiana NEON Workshop Tucson 13-April-09 Big Science at NSF? Advancements in science» Individual Investigators The heart
More informationGround-based GW detectors: status of experiments and collaborations
Ground-based GW detectors: status of experiments and collaborations C.N.Man Univ. Nice-Sophia-Antipolis, CNRS, Observatoire de Cote d Azur A short history GW & how to detect them with interferometry What
More informationThe Search for Gravitational Waves
The Search for Gravitational Waves Fred Raab, LIGO Hanford Observatory, on behalf of the LIGO Scientific Collaboration 21 October 2008 Outline What are gravitational waves? What do generic detectors look
More informationStatus of the LIGO Project
Status of the LIGO Project Gary Sanders California Institute of Technology LSC Meeting University of Florida - March 4, 1999 1 LIGO-G990012-00-M LIGO-G990022-02-M LIGO Schedule at Very Top Level 1996 Construction
More informationGravitational Wave Astronomy the sound of spacetime. Marc Favata Kavli Institute for Theoretical Physics
Gravitational Wave Astronomy the sound of spacetime Marc Favata Kavli Institute for Theoretical Physics What are gravitational waves? Oscillations in the gravitational field ripples in the curvature of
More informationLIGO Detection of Gravitational Waves. Dr. Stephen Ng
LIGO Detection of Gravitational Waves Dr. Stephen Ng Gravitational Waves Predicted by Einstein s general relativity in 1916 Indirect confirmation with binary pulsar PSR B1913+16 (1993 Nobel prize in physics)
More informationThe gravitational wave detector VIRGO
The gravitational wave detector VIRGO for the VIRGO collaboration Raffaele Flaminio Laboratoire d Annecy-le-Vieux de Physique des Particules (LAPP) IN2P3 - CNRS Summary I. A bit of gravitational wave physics
More informationSearching for gravitational waves with LIGO
Searching for gravitational waves with LIGO An introduction to LIGO and a few things gravity wave Michael Landry LIGO Hanford Observatory California Institute of Technology Spokane Astronomical Society
More informationAdvanced LIGO Research and Development
Advanced LIGO Research and Development David Shoemaker NSF Annual Review of LIGO 17 October 2003 LIGO Laboratory 1 LIGO mission: detect gravitational waves and initiate GW astronomy Commissioning talk
More informationGravitational Waves & Precision Measurements
Gravitational Waves & Precision Measurements Mike Smith 1 -20 2 HOW SMALL IS THAT? Einstein 1 meter 1/1,000,000 3 1,000,000 smaller Wavelength of light 10-6 meters 1/10,000 4 10,000 smaller Atom 10-10
More informationHow to measure a distance of one thousandth of the proton diameter? The detection of gravitational waves
How to measure a distance of one thousandth of the proton diameter? The detection of gravitational waves M. Tacca Laboratoire AstroParticule et Cosmologie (APC) - Paris Journée GPhys - 2016 July 6th General
More informationApril 21-23, Barry Barish LIGO-G M
LIGO NSF Review April 21-23, 1999 Overview Barry Barish LIGO Plans main activity 1996 Construction Underway -mostly civil 1997 Facility Construction -vacuum system 1998 Interferometer Construction -complete
More informationAdvanced LIGO: Context and Overview
Advanced LIGO Advanced LIGO: Context and Overview Gravitational waves offer a remarkable opportunity to see the universe from a new perspective, providing access to astrophysical insights that are available
More informationSqueezed Light Techniques for Gravitational Wave Detection
Squeezed Light Techniques for Gravitational Wave Detection July 6, 2012 Daniel Sigg LIGO Hanford Observatory Seminar at TIFR, Mumbai, India G1200688-v1 Squeezed Light Interferometry 1 Abstract Several
More informationOverview of Gravitational Wave Observations by LIGO and Virgo
Overview of Gravitational Wave Observations by LIGO and Virgo Giovanni Andrea Prodi Virgo Group at Padova-Trento, LIGO Scientific Collaboration and Virgo Collaboration Vulcano Workshop 2016, May 23 Published
More informationTakaaki Kajita, JGRG 22(2012) Status of KAGRA RESCEU SYMPOSIUM ON GENERAL RELATIVITY AND GRAVITATION JGRG 22. November
Takaaki Kajita, JGRG 22(2012)111402 Status of KAGRA RESCEU SYMPOSIUM ON GENERAL RELATIVITY AND GRAVITATION JGRG 22 November 12-16 2012 Koshiba Hall, The University of Tokyo, Hongo, Tokyo, Japan RESCEU
More informationWhat can LIGO detect? Abstract
What can LIGO detect? Adam Getchell Physics Department, University of California, Davis, 95616 Abstract This briey reviews the literature on gravitational wave astronomy, including theoretical basis, experimental
More informationSearching for Gravitational Waves from Coalescing Binary Systems
Searching for Gravitational Waves from Coalescing Binary Systems Stephen Fairhurst Cardiff University and LIGO Scientific Collaboration 1 Outline Motivation Searching for Coalescing Binaries Latest Results
More informationGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral Lazzaro Claudia for the LIGO Scientific Collaboration and the Virgo Collaboration 25 October 2017 GW170817 PhysRevLett.119.161101
More informationFuture underground gravitational wave observatories. Michele Punturo INFN Perugia
Future underground gravitational wave observatories Michele Punturo INFN Perugia Terrestrial Detectors Advanced detectors 2015-2025 GEO, Hannover, 600 m aligo Hanford, 4 km 2015 2016 AdV, Cascina, 3 km
More informationGravitational Waves: From Einstein to a New Science
Gravitational Waves: From Einstein to a New Science LIGO-G1602199 Barry C Barish Caltech - LIGO 1.3 Billion Years Ago 2 Black Holes Regions of space created by super dense matter from where nothing can
More informationHow the detection happened
For the first time, scientists have observed ripples in the fabric of spacetime called gravitational waves, arriving at the earth from a cataclysmic event in the distant universe. This confirms a major
More informationStatus of the International Second-generation Gravitational-wave Detector Network
Status of the International Second-generation Gravitational-wave Detector Network Albert Lazzarini Deputy Director, LIGO Laboratory California Institute of Technology On behalf of the LIGO Scientific Collaboration
More informationOverview of future interferometric GW detectors
Overview of future interferometric GW detectors Giovanni Andrea Prodi, University of Trento and INFN, many credits to Michele Punturo, INFN Perugia New perspectives on Neutron Star Interiors Oct.9-13 2017,
More informationGravitational Waves and LIGO: A Technical History
Gravitational Waves and LIGO: A Technical History Stan Whitcomb IEEE SV Tech History Committee Event 11 October 2018 LIGO-G180195-v3 Goal of Talk Review a few of the technical developments that enabled
More informationAdvanced LIGO Research and Development
Advanced LIGO Research and Development David Shoemaker NSF Annual Review of LIGO 17 November 2003 LIGO Laboratory 1 LIGO mission: detect gravitational waves and initiate GW astronomy Commissioning talk
More informationFigure 1: An example of the stretching and contracting of space-time caused by a gravitational wave.
SEARCHING FOR GRAVITATIONAL WAVES Nelson Christensen, for the LIGO Scientific Collaboration Physics and Astronomy, Carleton College, Northfield, Minnesota 55057 USA Abstract The search for gravitational
More informationSqueezed Light for Gravitational Wave Interferometers
Squeezed Light for Gravitational Wave Interferometers R. Schnabel, S. Chelkowski, H. Vahlbruch, B. Hage, A. Franzen, and K. Danzmann. Institut für Atom- und Molekülphysik, Universität Hannover Max-Planck-Institut
More informationStatus and Plans for Future Generations of Ground-based Interferometric Gravitational-Wave Antennas
Status and Plans for Future Generations of Ground-based Interferometric Gravitational-Wave Antennas 4 th international LISA Symposium July 22, 2002 @ Penn State University Seiji Kawamura National Astronomical
More informationLIGO Status Report 1. LIGO I. 2. E7 run (Dec.28,2001 ~ Jan.14,2002) 3. Advanced LIGO. Hiro Yamamoto
LIGO Status Report Hiro Yamamoto LIGO Laboratory / California Institute of Technology 1. LIGO I 2. E7 run (Dec.28,2001 ~ Jan.14,2002) 3. Advanced LIGO References : M.Coles (G020009), D.Coyne and D.Shoemaker
More informationAN OVERVIEW OF LIGO Adapted from material developed by Brock Wells Robert L. Olds Junior High School, Connell, WA August 2001
AN OVERVIEW OF LIGO Adapted from material developed by Brock Wells Robert L. Olds Junior High School, Connell, WA August 2001 The purpose of this guide is to provide background about the LIGO project at
More informationNewtonian instantaneous action at a distance General Relativity information carried by gravitational radiation at the speed of light
Modern View of Gravitation Newtonian instantaneous action at a distance G µ = 8 µ # General Relativity information carried by gravitational radiation at the speed of light Gravitational Waves GR predicts
More informationWe are born deaf to the sounds of the universe. Soon we will be able to listen to the gravitational sounds of the universe!
LIGO-G050519-00-Z If we were all born deaf the discovery of hearing would be momentous. We are born deaf to the sounds of the universe. Soon we will be able to listen to the gravitational sounds of the
More informationGravity. Newtonian gravity: F = G M1 M2/r 2
Gravity Einstein s General theory of relativity : Gravity is a manifestation of curvature of 4- dimensional (3 space + 1 time) space-time produced by matter (metric equation? g μν = η μν ) If the curvature
More informationGary Sanders LIGO/Caltech LSC Meeting, LLO March 16, 2004 LIGO-G M
State of State the LIGO of LIGO Laboratory Gary Sanders LIGO/Caltech LSC Meeting, LLO March 16, 2004 A 10 Year Anniversary LIGO s near death experience of early 1994» LIGO s second chance What was our
More informationGravitational wave detection. K.A. Strain
Gravitational wave detection K.A. Strain Contents gravitational waves: introduction sources of waves, amplitudes and rates basics of GW detection current projects future plans and hopes Gravitational Waves:
More informationHanbury Brown and Gravitational Waves
Hanbury Brown and Gravitational Waves Barry Barish Sydney, AIP Conference 10-July-02 Robert Hanbury Brown a role model for laboratory scientists! Tonbridge School» Studied classics Greek and Latin! Brighton
More informationSearches for Gravitational waves associated with Gamma-ray bursts
Searches for Gravitational waves associated with Gamma-ray bursts Raymond Frey University of Oregon for the LIGO Scientific Collaboration and the Virgo Collaboration 1 Current network of groundbased GW
More informationOutline. 1. Basics of gravitational wave transient signal searches. 2. Reconstruction of signal properties
Gravitational Wave Transients state-of-the-arts: detection confidence and signal reconstruction G.A.Prodi, University of Trento and INFN, for the LIGO Scientific Collaboration and the Virgo Collaboration
More informationObservation of Gravitational Waves from a Binary Black Hole Merger by Abbott et al. 2016, Phys. Rev. Lett. 116,
Observation of Gravitational Waves from a Binary Black Hole Merger by Abbott et al. 2016, Phys. Rev. Lett. 116, 061102 LIGO: The Beginning of Gravitational-wave Astronomy* (GW150914) Stephen C. McGuire,
More informationLaser Interferometer Gravitational-Wave Observatory (LIGO)! A Brief Overview!
Laser Interferometer Gravitational-Wave Observatory (LIGO) A Brief Overview Sharon Brunett California Institute of Technology Pacific Research Platform Workshop October 15, 2015 Credit: AEI, CCT, LSU LIGO
More informationFrequency dependent squeezing for quantum noise reduction in second generation Gravitational Wave detectors. Eleonora Capocasa
Frequency dependent squeezing for quantum noise reduction in second generation Gravitational Wave detectors Eleonora Capocasa 10 novembre 2016 My thesis work is dived into two parts: Participation in the
More informationFinding Black Holes with Lasers
Finding Black Holes with Lasers Andreas Freise Royal Institute of Great Brtitain 18.02.2013 [Image shows guide laser at Allgäu Public Observatory in Ottobeuren, Germany. Credit: Martin Kornmesser] LIGO-G1300827
More informationSynergy with Gravitational Waves
Synergy with Gravitational Waves Alexandre Le Tiec and Jérôme Novak Laboratoire Univers et Théories Observatoire de Paris / CNRS LIGO, Virgo, ( elisa, ET,... ( What is a gravitational wave? A gravitational
More informationStatus of the KAGRA Project
Status of the KAGRA Project Takaaki Kajita, for the KAGRA collaboration (~230 members) ICRR, Univ. of Tokyo Kajita_at_icrr.u-tokyo.ac.jp GWPAW2015 June, 2015, Osaka Outline Introduction: Overview of KAGRA
More informationGravitational wave cosmology Lecture 2. Daniel Holz The University of Chicago
Gravitational wave cosmology Lecture 2 Daniel Holz The University of Chicago Thunder and lightning Thus far we ve only seen the Universe (and 95% of it is dark: dark matter and dark energy). In the the
More informationB F Schutz AEI, Potsdam, Germany and Cardiff University, Wales, UK. The GWIC Roadmap
AEI, Potsdam, Germany and Cardiff University, Wales, UK The GWIC Roadmap GWIC (http://gwic.ligo.org) 2 GWIC The Gravitational Wave International Committee, was formed in 1997 to facilitate international
More informationGRAVITATIONAL WAVES THE NEW GENERATION OF LASER INTERFEROMETRIC DETECTORS
GRAVITATIONAL WAVES THE NEW GENERATION OF LASER INTERFEROMETRIC DETECTORS BARRY C. BARISH LIGO 18-34, California Institute of Technology, Pasadena, CA USA E-mail: barish@ligo.caltech.edu The effort to
More informationThe Science and Detection of Gravitational Waves
Barry C. Barish LIGO 18-4, California Institute of Technology, Pasadena, CA 9115, USA E-mail: barish@ligo.caltech.edu The Science and Detection of Gravitational Waves One of the most important consequences
More information