M.-A. Bizouard, F. Cavalier. GWDAW 8 Milwaukee 19/12/03
|
|
- Holly Cameron
- 5 years ago
- Views:
Transcription
1 Coincidence and coherent analyses for burst search using interferometers M.-A. Bizouard, F. Cavalier on behalf of the Virgo-Orsay group Network model Results of coincidence analysis: loose and tight coincidence Results of coherent analysis Comparison of all scenarios GWDAW 8 Milwaukee 19/12/03
2 Network of detectors For burst events a single detector can t claim for a GW discovery Need several ITF output to reject transient Coincidence with other kind of detectors (optical, ν, ) can help ITF Network: hypotheses of this study ITFs: Identical ITF sensitivity curves ITF Beam pattern and orientation Time delays between ITFs Up to 6 ITFs: Virgo, LIGO Hanford, LIGO Livingston, GEO, TAMA and AIGO Sources = Gaussian peak (width=1ms) and uniformly distributed in the sky Noise = Gaussian and white noise Filtering method: match filtering Monte Carlo simulations to estimate the efficiency versus false alarm rate curves (ROC)
3 h( t) F h ( t) + F h ( t) = + + Fx and F+ depend on detector location Source position Polarisation angle Ψ Network beam patterns x x Sky map = Ψ averaged beam pattern functions 2 2 F = F+ + F x LIGO maps similar by design Virgo and GEO more or less similar due to geometrical proximity Virgo and LIGO maps are orthogonal
4 Single ITF performance (Virgo) Beam Pattern Effect Selected Events Beam pattern effect on the GW SNR Virgo detection efficiency vs the source sky location
5 Coincidence Definition of a time window depending on time delay between detectors ij j i i j n. D D t = t t = c The source location is not known: loose coincidence ij ij t < t max +. η t ij RMS ( t ij max ~ 10ms...42ms) The source position is known: tight coincidence residual ij t <. η t ij RMS ij t RMS t ij RMS has been determined on simulation (SNR dependence): (<0.3 ms for SNR>5) ω 10 ~ 0.15ms 1ms SNR for SNR>6
6 Virgo-LIGO coincidence (loose) Request on 1/3 Twofold coincidence Good sky global coverage: average efficiency of 67% No more blind regions Coincidence less likely: ~ 20% for the 2 LIGO ~ 30% by adding Virgo Large regions almost blind
7 Loose coincidence in LIGO-Virgo network SNR opt =10 Best strategy: twofold coincidences (at least 2 among 3) Twofold coincidence is dominated by the 2 LIGO network (beam pattern matching) Single detector less efficient than coincidences Threefold coincidences are rare
8 Full network loose coincidence SNR opt =10 Twofold coincidence quite likely even at small false alarm rate Threefold coincidences also possible Larger coincidences much rarer
9 Full network tight coincidence Loose vs tight coincidence: - only few % of improvement in the region 1 false alarm per hour - 20% at very low false alarm rate For the Virgo-LIGO network very small improvement SNR opt =10
10 Coherent analysis Coherent statistics derived from a likelihood ratio (Pai, Bose & Dhurandhar (2001) method for coalescing binaries) General case: the source location is not known bank of N templates to cover the full sky for a Gaussian peak signal N goes 1/w 2 for w=1ms and MM=0.97 N ~ 5000 whatever the configuration (up to 6 ITFs)
11 Virgo-LIGO coherent analysis results Significant improvement in detection efficiency with respect to the coincidence case Efficiency remains above 60% for SNR opt = 10 even at a false alarm rate of 1 per week (35% for a twofold coincidence) Still no real hope to detect a weak signal (SNR opt = 5) in the 3 interferometer Virgo-LIGO network
12 Full network coherent analysis Clear enhancement of detection efficiencies by going from 3 to 6 ITFs Almost certain detection for SNR opt = 10 Still more than 80% SNR opt = 7.5 Efficiency remains SNR opt = 5 and below
13 Comparison Coherent/Coincident SNR = 10, False Alarm Rate = Single detector 39% OR strategy in Virgo-LIGO 69% OR strategy in full network 97% Twofold coincidence in Virgo-LIGO 52% Twofold coincidence in full network (loose) 90% Twofold coincidence in full network (tight) 93% Threefold coincidence in Virgo-LIGO 23% Threefold coincidence in full network (loose) 73% Threefold coincidence in full network (tight) 78% Coherent in Virgo-LIGO 78% Coherent in full network 99%
14 Coincident: This study has shown: No large increase of the efficiency when using tight coincidence Virgo-LIGO network: significant enhancement of the twofold efficiency when adding Virgo! One definitely gains more with a 6 ITFs network Increase of the network size is mandatory The sensitivity of the ITF in the network is also a fundamental parameter Virgo+LH4km+LL4km LH2km+LH4km+LL4km : Increase the false alarm rate by 2 orders of magnitude at equal efficiency! Coherent vs coincident: Coherent analysis is much more powerful than coincidence (even tight one) but is heavier to set up Future work: Improvement of the coincident analysis by introducing criteria about the main characteristics of the signal events?
Detecting the next Galactic supernova
Detecting the next Galactic supernova Nicolas Arnaud on behalf of the Virgo-LAL group Now fellow at LHCb-CERN Moriond Gravitation 2003 GW supernova amplitudes Burst online filter performances Comparison
More informationNEVER IGNORE A COINCIDENCE
ALEXANDER L. URBAN LEONARD E. PARKER CENTER FOR GRAVITATION, COSMOLOGY & ASTROPHYSICS NEVER IGNORE A COINCIDENCE ENHANCING LIGO SENSITIVITY TO COMPACT BINARY MERGERS WITH GRB COUNTERPARTS 23 RD MIDWEST
More informationSearch for compact binary systems in LIGO data
Search for compact binary systems in LIGO data Thomas Cokelaer On behalf of the LIGO Scientific Collaboration Cardiff University, U.K. LIGO-G060630-00-Z Plan 1) Overview What kind of gravitational waves
More informationData Analysis Pipeline: The Search for Gravitational Waves in Real life
Data Analysis Pipeline: The Search for Gravitational Waves in Real life Romain Gouaty LAPP - Université de Savoie - CNRS/IN2P3 On behalf of the LIGO Scientific Collaboration and the Virgo Collaboration
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 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 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 informationarxiv:gr-qc/ v1 10 Oct 2001
Network Sensitivity to Geographical Configuration arxiv:gr-qc/0110053v1 10 Oct 2001 Antony C Searle, Susan M Scott and David E McClelland Department of Physics and Theoretical Physics, Faculty of Science,
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 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 informationBenefits of joint LIGO Virgo coincidence searches for burst and inspiral signals
Institute of Physics Publishing Journal of Physics: Conference Series 32 (2006) 212 222 doi:10.1088/1742-6596/32/1/032 Sixth Edoardo Amaldi Conference on Gravitational Waves Benefits of joint LIGO Virgo
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 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 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 informationTime-delay Interferometry (TDI) for LISA
Time-delay Interferometry (TDI) for LISA Sanjeev Dhurandhar IUCAA, Pune TAMA Symposium 19 Feb 5 Plan of the Talk Introduction: LISA GW sources for LISA Laser phase noise cancellation problem Theoretical
More informationGravitational-Wave Data Analysis
Gravitational-Wave Data Analysis Peter Shawhan Physics 798G April 12, 2007 Outline Gravitational-wave data General data analysis principles Specific data analysis methods Classification of signals Methods
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 informationPlans for the LIGO TAMA joint search for gravitational wave bursts
INSTITUTE OF PHYSICS PUBLISHING Class. Quantum Grav. 21 (2004) S1801 S1807 CLASSICAL AND QUANTUM GRAVITY PII: S0264-9381(04)79467-8 Plans for the LIGO TAMA joint search for gravitational wave bursts Patrick
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 informationSearch for Gravitational Wave Transients. Florent Robinet On behalf of the LSC and Virgo Collaborations
Search for Gravitational Wave Transients On behalf of the LSC and Virgo Collaborations 1 Gravitational Waves Gravitational waves = "ripples" in space time Weak field approximation : g = h h 1 Wave equation,
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 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 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 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 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 informationOn the minimum flexing of arms of LISA (Laser Interferometer Space Antenna)
On the minimum flexing of arms of LISA (Laser Interferometer Space Antenna) Dr. SUCHETA KOSHTI IISER, Pune, India. ICSW-7, IPM, Tehran,Iran Jun4, 27 Motivation Einstein s General theory of relativity (GR)
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 informationThe direct detection of gravitational waves: The first discovery, and what the future might bring
The direct detection of gravitational waves: The first discovery, and what the future might bring Chris Van Den Broeck Nikhef - National Institute for Subatomic Physics Amsterdam, The Netherlands Physics
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 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 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 informationThe search for continuous gravitational waves: analyses from LIGO s second science run
The search for continuous gravitational waves: analyses from LIGO s second science run Michael Landry LIGO Hanford Observatory on behalf of the LIGO Scientific Collaboration http://www.ligo.org April APS
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 informationarxiv:gr-qc/ v1 16 Feb 2007
International Journal of Modern Physics D c World Scientific Publishing Company arxiv:gr-qc/0702096v1 16 Feb 2007 Data Analysis of Gravitational Waves Using A Network of Detectors Linqing Wen Max Planck
More informationCore-Collapse Supernova Science with Advanced LIGO and Virgo
Core-Collapse Supernova Science with Advanced LIGO and Virgo Fifty-One Erg Raleigh, 06/01/2015 Marek Szczepańczyk Mösta et al 2014 LIGO Scientific Collaboration and Virgo Collaboration The Advanced GW
More informationmeasuring GW polarizations beyond GR recent results and future prospects
measuring GW polarizations beyond GR recent results and future prospects LIGO Laboratory California Institute of Technology Massachusetts Institute of Technology Oct 2, 2018 Einstein Symposium Harvard
More informationCristina Valeria Torres University of Texas at Brownsville. Amber L. Stuver LIGO Livingston Observatory. LIGO-G v1 LIGO-G v1
Capitalizing on GW polarization bias for a pair of interferometric detectors To increase parameter estimation speed and Investigate the potential implications for stellar evolution models. Cristina Valeria
More informationChirplets pour la détection des ondes gravitationnelles
Chirplets pour la détection des ondes gravitationnelles Éric Chassande-Mottin AstroParticule et Cosmologie, Paris et collaborateurs : Satya Mohapatra, Miriam Miele, Laura Cadonati, Zacharya Nemtzow Outline
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 Present and Future. Barry Barish Directory of the LIGO Laboratory
LIGO Present and Future Barry Barish Directory of the LIGO Laboratory LIGO I Schedule and Plan LIGO I has been built by LIGO Lab (Caltech & MIT) 1996 Construction Underway (mostly civil) 1997 Facility
More informationLIGO s continuing search for gravitational waves
LIGO s continuing search for gravitational waves Patrick Brady University of Wisconsin-Milwaukee LIGO Scientific Collaboration LIGO Interferometers LIGO is an interferometric detector» A laser is used
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 informationGW150914: Observation of gravitational waves from a binary black hole merger
IL NUOVO CIMENTO 39 C (2016) 310 DOI 10.1393/ncc/i2016-16310-2 Colloquia: La Thuile 2016 GW150914: Observation of gravitational waves from a binary black hole merger F. Marion on behalf of the LIGO Scientific
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 informationGravitational wave detection with Virgo and LIGO experiment - Case of the long bursts
Gravitational wave detection with Virgo and LIGO experiment - Case of the long bursts Samuel Franco Supervisor: Patrice Hello Laboratoire de l Accélérateur Linéaire (Orsay) 06/12/2013 Samuel Franco (LAL)
More informationSearching for gravitational waves from neutron stars
Searching for gravitational waves from neutron stars Ian Jones D.I.Jones@soton.ac.uk General Relativity Group, Southampton University Ian Jones Searching for gravitational waves from neutron stars 1/23
More informationGravitational wave data analysis
Max Planck Institut für Gravitationsphysik Albert Einstein Institut, Germany Pasadena, June 2011 1 Introduction to gravitational waves 2 3 4 5 6 Gravitational Waves GR can be formulated in terms of a spacetime
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 informationSearch for inspiralling neutron stars in LIGO S1 data
INSTITUTE OF PHYSICS PUBLISHING Class. Quantum Grav. 21 (2004) S691 S696 CLASSICAL AND QUANTUM GRAVITY PII: S0264-9381(04)68883-6 Search for inspiralling neutron stars in LIGO S1 data Gabriela González
More informationarxiv: v1 [gr-qc] 25 Jul 2008
Source Tracking for Sco X-1 arxiv:87.4171v1 [gr-qc] 25 Jul 28 1. Introduction K Hayama 1, S D Mohanty 1, S Desai 2, M Rakhmanov 1, T Summerscales 3, S Yoshida 4 1 The University of Texas at Brownsville,
More informationResults from LIGO Searches for Binary Inspiral Gravitational Waves
Results from LIGO Searches for Binary Inspiral Gravitational Waves Peter Shawhan (LIGO Laboratory / Caltech) For the LIGO Scientific Collaboration American Physical Society April Meeting May 4, 2004 Denver,
More informationMapping Inspiral Sensitivity of Gravitational Wave Detectors
Mapping Inspiral Sensitivity of Gravitational Wave Detectors Anthony D. Castiglia Mentor: John T. Whelan Rochester Institute of Technology 12 August, 2011 Acknowledgments Mentor: John T. Whelan NSF Grant
More informationData quality vetoes and their effect on searches for gravitational waves from compact binary systems
Data quality vetoes and their effect on searches for gravitational waves from compact binary systems Samantha Usman August 12, 2014 Abstract Data quality flags have been designed to prevent problems caused
More informationSearch for the gravity wave signature of GRB030329/SN2003dh
Laser Interferometer Gravitational-Wave Observatory (LIGO) Search for the gravity wave signature of GRB030329/SN2003dh ABSTRACT Optimal Integration length Well detectable Sine- Gaussian simulation One
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 informationarxiv:gr-qc/ v1 3 Jan 2007
Detailed comparison of LIGO and Virgo Inspiral Pipelines in Preparation for a Joint Search F. Beauville 8, M.-A. Bizouard 1, L. Blackburn 3, L. Bosi 11, L. Brocco 12, D. Brown 2,7, D. Buskulic 8, F. Cavalier
More informationGravitational Wave Astronomy s Next Frontier in Computation
Gravitational Wave Astronomy s Next Frontier in Computation Chad Hanna - Penn State University Penn State Physics Astronomy & Astrophysics Outline 1. Motivation 2. Gravitational waves. 3. Birth of gravitational
More informationLIGO Observational Results
LIGO Observational Results Patrick Brady University of Wisconsin Milwaukee on behalf of LIGO Scientific Collaboration LIGO Science Goals Direct verification of two dramatic predictions of Einstein s general
More informationLarge-scale Cryogenic Gravitational wave Telescope (LCGT) TAMA/CLIO/LCGT Collaboration Kazuaki KURODA
29-March, 2009 JPS Meeting@Rikkyo Univ Large-scale Cryogenic Gravitational wave Telescope (LCGT) TAMA/CLIO/LCGT Collaboration Kazuaki KURODA Overview of This talk Science goal of LCGT First detection of
More informationGRAVITATIONAL WAVE SOURCES AND RATES FOR LISA
GRAVITATIONAL WAVE SOURCES AND RATES FOR LISA W. Z. Korth, PHZ6607, Fall 2008 Outline Introduction What is LISA? Gravitational waves Characteristics Detection (LISA design) Sources Stochastic Monochromatic
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 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 informationInterferometric. Gravitational Wav. Detectors. \p World Scientific. Fundamentals of. Peter R. Sawlson. Syracuse University, USA.
SINGAPORE HONGKONG Fundamentals of Interferometric Gravitational Wav Detectors Second Edition Peter R. Sawlson Martin A. Pomerantz '37 Professor of Physics Syracuse University, USA \p World Scientific
More informationGRB-triggered searches for gravitational waves from compact binary inspirals in LIGO and Virgo data during S5/VSR1
GRB-triggered searches for gravitational waves from compact binary inspirals in LIGO and Virgo data during S5/VSR1 Nickolas Fotopoulos (UWM) for the LIGO Scientific Collaboration and the Virgo Collaboration
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 informationLIGO S2 Inspiral Hardware Injections
LIGO S2 Inspiral Hardware Injections Steve Fairhurst University of Wisconsin-Milwaukee LSC Inspiral Working Group GWDAW December 19, 2003. LIGO-G030688-00-Z Introduction Hardware injections provide a good
More informationLecture 8: Signal Detection and Noise Assumption
ECE 830 Fall 0 Statistical Signal Processing instructor: R. Nowak Lecture 8: Signal Detection and Noise Assumption Signal Detection : X = W H : X = S + W where W N(0, σ I n n and S = [s, s,..., s n ] T
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 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 informationTest for scalar-tensor theory from observations of gravitational wave bursts with a network of interferometric detectors
Test for scalar-tensor theory from observations of gravitational wave bursts with a network of interferometric detectors Project page : http://www.aei.mpg.de/~kahaya/ridge-scalar/index.html Kazuhiro Hayama
More informationSqueezing manipulation with atoms
Squeezing manipulation with atoms Eugeniy E. Mikhailov The College of William & Mary March 21, 2012 Eugeniy E. Mikhailov (W&M) Squeezing manipulation LSC-Virgo (March 21, 2012) 1 / 17 About the college
More informationarxiv: v2 [gr-qc] 14 Feb 2015
Postprocessing methods used in the search for continuous gravitational-wave signals from the Galactic Center arxiv:141.5997v2 [gr-qc] 14 Feb 215 Berit Behnke, 1, a Maria Alessandra Papa, 1, 2, b and Reinhard
More informationLIGO-G Test of scalar-tensor gravity theory from observations of gravitational wave bursts with advanced detector network.
LIGO-G1139 Test of scalar-tensor gravity theory from observations of gravitational wave bursts with advanced detector network Kazuhiro Hayama National Astronomical Observatory of Japan Max Planck Institute
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 informationReconstruction of chirp mass in searches for gravitational wave transients
Classical and Quantum Gravity LETTER Reconstruction of chirp mass in searches for gravitational wave transients To cite this article: V Tiwari et al Class. Quantum Grav. 0LT0 Manuscript version: Accepted
More informationGravitational-Wave Data Analysis: Lecture 3
Gravitational-Wave Data Analysis: Lecture 3 Peter S. Shawhan Gravitational Wave Astronomy Summer School May 30, 2012 Outline for Today Gaining confidence in a signal candidate Consistency tests Data quality
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 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 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 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 informationA template bank to search for gravitational waves from inspiralling compact binaries: II. Phenomenological model
LIGO-P070089-01-Z A template bank to search for gravitational waves from inspiralling compact binaries: II. Phenomenological model T. Cokelaer 1 1 School of Physics and Astronomy, Cardiff University, Cardiff
More informationAll-sky LIGO Search for Periodic Gravitational Waves in the Fourth Science Run (S4)
All-sky LIGO Search for Periodic Gravitational Waves in the Fourth Science Run (S4) Keith Riles University of Michigan For the LIGO Scientific Collaboration APS Meeting, Jacksonville, Florida April 14-17,
More informationarxiv:gr-qc/ v1 4 Dec 2003
Testing the LIGO Inspiral Analysis with Hardware Injections arxiv:gr-qc/0312031 v1 4 Dec 2003 Duncan A. Brown 1 for the LIGO Scientific Collaboration 1 Department of Physics, University of Wisconsin Milwaukee,
More informationWork of the LSC Pulsar Upper Limits Group (PULG) Graham Woan, University of Glasgow on behalf of the LIGO Scientific Collaboration
Work of the LSC Pulsar Upper Limits Group (PULG) Graham Woan, University of Glasgow on behalf of the LIGO Scientific Collaboration GWDAW 2003 1 Pulsar Upper Limits Group (PULG) Community of LSC members
More informationSearching for Intermediate Mass Black Holes mergers
Searching for Intermediate Mass Black Holes mergers G. A. Prodi, Università di Trento and INFN for the LIGO Scientific collaboration and the Virgo collaboration special credits to Giulio Mazzolo and Chris
More informationApplications of change point detection in Gravitational Wave Data Analysis. Soumya D. Mohanty AEI
Applications of change point detection in Gravitational Wave Data Analysis Soumya D. Mohanty AEI Plan of the talk Brief introduction to change point detection and its relevance to GW data analysis Contrast
More informationInnovative Technologies for the Gravitational-Wave Detectors LIGO and Virgo
Innovative Technologies for the Gravitational-Wave Detectors LIGO and Virgo Jan Harms INFN, Sezione di Firenze On behalf of LIGO and Virgo 1 Global Network of Detectors LIGO GEO VIRGO KAGRA LIGO 2 Commissioning
More informationM.Alessandra Papa. Max Planck Inst. f. Gravitationsphysik and Univ. of Wisconsin- Milwaukee. ICGC Conference 2007, December Pune
Gravitational Wave Data Analysis M.Alessandra Papa Max Planck Inst. f. Gravitationsphysik and Univ. of Wisconsin- Milwaukee ICGC Conference 2007, December Pune Gravitational wave data analysis * legacy
More informationGravitational Wave Astronomy using 0.1Hz space laser interferometer. Takashi Nakamura GWDAW-8 Milwaukee 2003/12/17 1
Gravitational Wave Astronomy using 0.1Hz space laser interferometer Takashi Nakamura GWDAW-8 Milwaukee 2003/12/17 1 In 2001 we considered what we can do using 0.1 hertz laser interferometer ( Seto, Kawamura
More informationGravitational Wave Observatories III: Ground Based Interferometers. Neil J. Cornish
Gravitational Wave Observatories III: Ground Based Interferometers Neil J. Cornish Outline Interferometer design Sources of noise LIGO data analysis, theory and search results Astrophysical rates Gravitational
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 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 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 informationParameter estimation for signals from compact binary inspirals injected into LIGO data
IOP PUBLISHING Class. Quantum Grav. 26 (2009) 204010 (10pp) CLASSICAL AND QUANTUM GRAVITY doi:10.1088/0264-9381/26/20/204010 Parameter estimation for signals from compact binary inspirals injected into
More informationSearching for Gravitational Waves from Binary Inspirals with LIGO
Searching for Gravitational Waves from Binary Inspirals with LIGO Duncan Brown University of Wisconsin-Milwaukee for the LIGO Scientific Collaboration Inspiral Working Group LIGO-G030671-00-Z S1 Binary
More informationDetection theory 101 ELEC-E5410 Signal Processing for Communications
Detection theory 101 ELEC-E5410 Signal Processing for Communications Binary hypothesis testing Null hypothesis H 0 : e.g. noise only Alternative hypothesis H 1 : signal + noise p(x;h 0 ) γ p(x;h 1 ) Trade-off
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 informationS. V. Dhurandhar IUCAA Pune, India
Extended hierarchical search (EHS) for inspiraling compact binaries S. V. Dhurandhar IUCAA Pune, India * A. Sengupta, A. Lazzarini, P. Shawhan LIGO-G040556-00-R Plan of the Talk The 1-step (flat) search
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 information