ELiTES The European-Japanese collaboration in Gravitational Wave research Dr. Michele Punturo Istituto Nazionale di Fisica Nucleare (INFN) European Gravitational.

Slides:



Advertisements
Similar presentations
Michele Punturo on behalf of the ET team GA # A short introduction to the project.
Advertisements

Michele Punturo European Gravitational Observatory and INFN-Perugia On behalf of the GW ILIAS-next community Gravitational Wave Network.
 ET is a “design study” supported by the European Commission under the Framework Programme 7 (FP7)  It is a ~3 years project supported by EC with about.
Michele Punturo INFN Perugia and EGO On behalf of the Einstein Telescope Design Study Team 1GWDAW-Rome 2010.
G v1Advanced LIGO1 Status of Ground-Based Gravitational-wave Interferometers July 11, 2012 Daniel Sigg LIGO Hanford Observatory Astrod 5, Bangalore,
VIRGO: WHERE WE COME FROM WHERE WE ARE GOING GIOVANNI LOSURDO - INFN Firenze Advanced Virgo Project Leader for the Virgo Collaboration (and the LIGO Scientific.
1 Science Opportunities for Australia Advanced LIGO Barry Barish Director, LIGO Canberra, Australia 16-Sept-03 LIGO-G M.
LIGO-GXX What is LIGO (LSC/GEO/Virgo/…)? Gabriela González, Louisiana State University For the LIGO Scientific Collaboration and the Virgo Collaboration.
LIGO-G W Is there a future for LIGO underground? Fred Raab, LIGO Hanford Observatory.
Laser Interferometer Gravitational-Wave Observatory Who? Presented By: Bonnie Wooley.
1 Observing the Most Violent Events in the Universe Virgo Barry Barish Director, LIGO Virgo Inauguration 23-July-03 Cascina 2003.
Gravitational-waves: Sources and detection
LIGO-DCC G Astronomy group seminar, University of Southampton, Jan 2015.
Gravitational Wave Detectors: new eyes for physics and astronomy Gabriela González Department of Physics and Astronomy Louisiana State University.
ET: Einstein Telescope A new gateway to knowledge T. Csörgő MTA Wigner RCP, Budapest, KRF, Gyöngyös, Hungary
LIGO-G Opening the Gravitational Wave Window Gabriela González Louisiana State University LSC spokesperson For the LIGO Scientific Collaboration.
E.T. Design Study Harald Lück. 3 main noise sources Thermal Noise Seismic Shot Noise.
E.T. Design Study & European roadmaps Michele Punturo/Harald Lück.
Status of LIGO Data Analysis Gabriela González Department of Physics and Astronomy Louisiana State University for the LIGO Scientific Collaboration Dec.
LIGO- G D Status of LIGO Stan Whitcomb ACIGA Workshop 21 April 2004.
LIGO-G Z LIGO at the start of continuous observation Prospects and Challenges Albert Lazzarini LIGO Scientific Collaboration Presentation at NSF.
LIGO-G D LIGO Laboratory1 Stoyan Nikolov LIGO-G D The LIGO project’s quest for gravitational waves Presenting LIGO to the students of.
WG3 Report Michele Punturo Harald Lück. WG3 composition Co-Chairmen M.Punturo INFN Perugia, Italy H.Lück MPI für Gravitationsphysik, AEI, Hannover, Germany.
Fundamental Physics, Astrophysics and Cosmology with ET p1 Michele Punturo on behalf of the ET team GA # A short introduction to the project.
PX444 – The Distant Universe Lecture 13 The History of Star Formation.
G Z The LIGO gravitational wave detector consists of two observatories »LIGO Hanford Observatory – 2 interferometers (4 km long arms and 2 km.
LIGO-G M Press Conference Scientific Operation of LIGO Gary H Sanders Caltech (on behalf of a large team) APS April Meeting Philadelphia 6-April-03.
Michele Punturo INFN Perugia and EGO 11st ELiTES meeting.
ELiTES 1 st General Meeting Tokyo, October 2012 Federico Ferrini – EGO Director Thanks to the European Union Delegation.
The quest for gravitational waves. 2 The Universe has been studied essentially through EM radiation. GWs have a different origin. The Scientific Motivation.
GW – the first GW detection ! Is it a start of GW astronomy ? If “yes” then which ? «Счастлив, кто посетил сей мир в его минуты роковые !...» Ф.Тютчев.
Toward ET ? Michele Punturo INFN and EGO 1ET: EU framework.
By Jan Haas. Overview 1. Gravitation as a wave 2. Weber bars 3. Laser interferometers 4. LISA.
+ GRAVITATIONAL WAVES The announcement of a global discovery Eleonora Cossi, INFN – Communications Office UFF COM ON THE VIRGO SIDE.
Harald Lück AEI Hannover. Thank you Science Team! You did a great job!
ELiTES 4 th General Meeting Michele Punturo EGO and INFN.
Michele Punturo EGO & INFN Perugia 1 2nd ET meeting, Erice Oct'09.
THE NEXT GENERATIONS OF GRAVITATIONAL WAVE DETECTORS (*) Giovanni Losurdo INFN Firenze – Virgo collaboration (*) GROUND BASED, INTERFEROMETRIC.
LIGO-G Z 1 Gravitational Wave Searches Peter R. Saulson Syracuse University Department of Physics Spokesperson, LIGO Scientific Collaboration.
Gravitational Wave Data Analysis  GW detectors  Signal processing: preparation  Noise spectral density  Matched filtering  Probability and statistics.
Overview of iLCGT & bLCGT Kazuaki Kuroda LCGT Collaboration F2f meeting 27 September, 2010.
Michele Punturo INFN Perugia and EGO 1MGR13- ET.
Lessons to be learned from the ET design study Michele Punturo INFN Perugia ET-0005A-16 Dawn Meeting
The Quest for Gravitational Waves: a global strategy
Advanced Detector Status Report and Future Scenarios
Dawn II, July 8, 2016 GaTech Organizing the international community: issues, open questions, opportunities Dave Reitze LIGO Laboratory, Caltech LIGO Laboratory.
Current and future ground-based gravitational-wave detectors
GW Policy: The Future: G3 Detectors
The Search for Gravitational Waves with Advanced LIGO
EGO The Infrastructure for Gravitational Wave Research in Europe
THE NEXT GENERATION OF GRAVITATIONAL WAVE DETECTORS
Commission II meeting – 7 March 2009
Is there a future for LIGO underground?
Advanced VIRGO Experiment
LIGO detectors: past, present and future
CERN LVC workshop roundtable (what’s coming next?)
DAWN III Workshop: What’s Next for Gravitational Wave Astronomy?
Nergis Mavalvala (age 47)
ILIAS WP3 activities report and ET organization
DIRECT DETECTION OF GRAVITATIONAL WAVES FROM NEUTRON STARS
The Age of Real-time Big Science
Gravitational wave detection and the quantum limit
Status of LIGO Patrick J. Sutton LIGO-Caltech
OK Alexander Dietz Louisiana State University
The Laser Interferometer Gravitational-wave Observatory
ELiTES The acronym ELiTES stands for:
Update on Status of LIGO
Detection of Gravitational Waves with Interferometers
WG3 Activities M.Punturo & H.Lueck WG3 - 4th ILIAS GW meeting.
The views of Virgo collaboration groups on upgraded/advanced Virgo
Presentation transcript:

ELiTES The European-Japanese collaboration in Gravitational Wave research Dr. Michele Punturo Istituto Nazionale di Fisica Nucleare (INFN) European Gravitational Observatory

Japan Society for the Promotion of Science What is ELiTES? The acronym ELiTES stands for: ET LCGT Telescopes: Exchanges of Scientists Let analyse the name of the project That is easy! But exchange from …. to ….? FP7-European Commission ELiTES € ELiTES ELiTES ¥ ELiTES Japan Society for the Promotion of Science ELiTES 3rd ELiTES meeting

What is ELiTES? The acronym ELiTES stands for: What are ET and LCGT? ET LCGT Telescopes: Exchanges of Scientists What are ET and LCGT? ET is a (project for a far) future Gravitational Wave (GW) Observatory in Europe LCGT, now named KAGRA, is a (near) future GW detector under construction in Japan Prof. Kentaro Somiya will introduce you to the GW physics, whereas I would like to explain you why and how we are collaborating 3rd ELiTES meeting

Gravitational Waves GW are foreseen by the General Relativity of Albert Einstein and are emitted in catastrophic events in the universe: Coalescences of Neutron Stars or Black Holes Supernovae Explosions Big Bang To detect the emitted GW a series of giant detectors has been realised 3rd ELiTES meeting

Science is competition A series of detectors has been active in the World in the 2000-2011 decade GEO, Hannover, 600 m LIGO Hanford, 4 km: 2 ITF on the same site! TAMA, Tokyo, 300 m Virgo, Cascina, 3 km LIGO Livingston, 4 km 3rd ELiTES meeting

Science is competition A new detector is under construction in Japan (KAGRA), the others are under upgrade (new technologies) GEO, Hannover, 600 m ~2018 aLIGO Hanford, 4 km 2015 ~2022 2016 AdV, Cascina, 3 km aLIGO Livingston, 4 km 3rd ELiTES meeting

Science is collaboration To reconstruct the position in the Universe of the GW source, we need at least 3 detectors in the world (better if 4, 5, …) 3rd ELiTES meeting

Science is collaboration It is not a series of detectors, but a network of detectors GEO, Hannover, 600 m DATA ~2018 aLIGO Hanford, 4 km 2015 ~2022 2016 AdV, Cascina, 3 km aLIGO Livingston, 4 km 3rd ELiTES meeting

Science is collaboration Exchange of technologies WP1, WP2:Suspensions materials, fibres WP1: Suspensions design and test WP3: Infrastructures & Vacuum apparatuses WP2: Coatings, Optics 3rd ELiTES meeting

Conclusions This is the 3rd ELiTES general meeting, organised in Tokyo and hosted by the European Delegation probably one more meeting remains (early in 2016), but we are already thinking to the future (H2020?), because we need to collaborate if we want to achieve our scientific targets 3rd ELiTES meeting

End 3rd ELiTES meeting