GENERAL
ABOUT INFN
ORGANISATION CHART
INFN HEADQUARTERS
PRESS OFFICE
ADMINISTRATION
PHONE BOOK
JOB OPPORTUNITIES
 ACTIVITIES
PARTICLE PHYSICS
ASTROPARTICLE PHYSICS
NUCLEAR PHYSICS
THEORETICAL PHYSICS
TECHNOLOGY
EXPERIMENTS
INFN PUBLICATIONS
THESIS
 SERVICES
PORTALE INFN
AGENDA INFN
EDUCATIONAL
WEBCAST
MULTIMEDIA
EU FP7
 

Trasparenza valutazione e merito  

DataWeb Support ticket  -  e-mail  

 

  16-10-2008: EUROPEAN COMMISSION FUNDS DESIGN STUDY FOR UNIQUE FUTURE OBSERVATORY 
 COMPLETE LIST 

© Copyright 2002 INFN The use of photos is free of charge. Please request authorisation from the INFN Communication Office




By allocating three million Euro within the FP7 programme for preliminary studies for the Einstein Telescope (ET) – a pan-European gravitational wave observatory – the European Commission has made a decisive step towards the exploration of the universe with gravitational waves. With this grant, the commission confirms the importance of gravitational wave research for both basic and applied scientific research in Europe. “With its decision, the European Commission recognizes the achievements made by the gravitational wave observatories GEO600 and Virgo, and paves the way for the development of the first pan-European gravitational wave detector”, says Jacques Colas, director of the European Gravitational Observatory (EGO) and project coordinator of the design study for the Einstein Telescope.

The direct detection of gravitational waves – tiny distortions of space-time predicted by Albert Einstein - is one of the most important and fundamental research areas of modern science. Their direct observation will allow us totally new insights into our universe inaccessible to any other technology – including clues as to its very beginning.

The Einstein Telescope Project (ET)
ET is a joint project of eight European research institutes, under the direction of EGO. The participants are EGO an Italian French consortium located near Pisa (Italy), Instituto Nazionale di Fisica Nucleare (INFN) from Italy, the French Centre National de la Recherche Scientifique (CNRS), the German Albert Einstein Institute (AEI) Hannover, the Universities of Birmingham, Cardiff and Glasgow from United Kingdom and the Dutch Vrije Universiteit Amsterdam.

The funds granted now by the European Commission will be used in a design study for ET over the next three years. The design study is an important step towards the third generation of gravitational wave observatories, defining the specifications for the required site and infrastructure and the necessary technologies, and lastly also the total budget needed.

Michele Punturo, scientific coordinator of the Einstein Telescope Design Study: „The first two generations will already launch the age of gravitational wave astronomy, and we expect this third generation observatory to be a hundred times more sensitive than current detectors. The observable volume of the universe will increase by a factor of a million.” Additionally all frequencies that can be measured on Earth, the entire range between 1 Hz and 10 kHz, can be detected by this instrument. “This allows ET to open a new door in gravitational wave research”, says Punturo. The ambitious goal will be reached by combining the cutting edge of all currently known technologies in a single observatory.

Harald Lück, deputy scientific coordinator of the ET Design Study and coordinator of the upgrade of the GEO600 detector adds: “The European experimental gravitational wave research community presents a well consolidated evolution plan, which is synchronized with the US plans, from the current observatories and the second generation interferometers - scheduled to take data in a few years - to the Einstein Telescope project.”


“Observation of gravitational waves would have far-reaching consequences, aside from verifying the General Theory of Relativity: It would become possible to cast an eye on the “early childhood” of our universe for the first time,” says Harald Lück. Up to now observation of the sky is limited to the electromagnetic spectrum (e.g., radio and X-ray telescopes and astronomy in visible light). The information thus available to us can reach us from the past only from a time at least 380,000 years after the Big Bang. Epochs dating back further have thus far remained hidden, as the universe became transparent for electromagnetic radiation only at that time. The various theories on the early universe have therefore remained unverified experimentally. The direct measurement of gravitational waves may allow “listening” back as far as the very first trillionth of a second following the Big Bang: This would give us totally new information about our universe: with gravitational wave astronomy, totally new areas of science will become accessible.

The global network
Gravitational wave research is a global effort because the full information about many gravitational wave sources can only be obtained with several interferometers working simultaneously in different places.
Therefore the US, German-British, Italian-French, and Dutch scientific communities are working close together for a long time: They share technology development, numerical relativity methods and data analysis methods and tools. The joint European project ET will help to further improve this world wide collaboration.

Status of current detectors
Currently, several first generation gravitational wave detectors are active in Europe. The German-British GEO600 observatory, funded by STFC1 and MPG2, is operating close to Hanover while the French-Italian-Dutch Virgo project is located in Cascina near Pisa (Italy). These interferometers pool their data with the three American LIGO interferometers and are currently doing extensive searches for gravitational waves from astrophysical systems.

Searches for gravitational waves from these data sets and the algorithms used in the analysis are the result of many years of research and development in Europe and the U.S. Today European scientists are leading several of the analyses efforts in this international pursuit for the direct detection of gravitational waves.

During the next decade all interferometric gravitational wave detectors will be upgraded to second-generation instruments. Virgo and LIGO will gain a factor of about ten in sensitivity at lower frequencies (up to about a kilohertz) using technology largely developed in Europe. GEO will pioneer high frequency wide-band observing above one kilohertz, again deploying new technologies. If the current instruments do not make the first detections of gravitational waves, it can confidently be expected that this will be done by the second-generation interferometers.

The ET project is well inserted in this scenario. In fact, after the completion of the design study and of a subsequent technical preparation phase, the effective construction can begin, probably in the year 2017 or 2018, just after the second generation observatories have started operating.

Leaders in gravitational wave research
In Europe there is a long tradition and excellent know-how in developing detectors for gravitational waves. It has produced the most sensitive cryogenic resonant bar detectors, and pioneered the development of laser interferometer detectors. The first experiments with coincident observing by interferometers took place in Europe (between the prototypes in Glasgow and Garching), and most of the key design ideas that underlie the sensitivity of interferometers operating today around the world originated in Europe (e.g. high power lasers, laser stabilisation, power recycling, signal recycling). Europe continues to pioneer gravitational wave technology with its leading role in the space-based LISA and LISA-Pathfinder projects.

The technology required for third generation detectors is being studied in several countries besides Europe, including the USA and Japan. All third-generation detectors that are eventually built will need to perform joint observations together (as the previous generation detectors do).

1 STFC: Science and Technology Facilities Council; http://www.scitech.ac.uk/
2 MPG: Max Planck Gesellschaft; http://www.mpg.de/english/portal/index.html
CNRS: Centre National de la Recherche Scientifique; ; http://www.cnrs.fr/
INFN: Istituto Nazionale di Fisica Nucleare; ; http://www.infn.it/

Further information:
http://www.et-gw.eu/
http://geo600.aei.mpg.de/
http://www.virgo.infn.it/



Contact:
Susanne Milde, milde@mildemarketing.de, Tel.: +49 331 583 93 55
Carlo Bradaschia, carlo.bradaschia@pi.infn.it, Tel.: +39 339 67 22 355


 RELATED SITES 
http://www.et-gw.eu/

 RECENT NEWS  
26-03-2013: OPERA observed a third neutrino tau
08-06-2012: Neutrinos sent from CERN to Gran Sasso respect the cosmic speed limit
06-06-2012: OPERA OBSERVES THE SECOND TAU NEUTRINO
18-05-2012: FEL, A SUPER LASER FOR SUPERB
15-05-2012: Research on neutrinos allows the discovery of vortices in the abysses of the eastern Mediterranean
16-03-2012: The Icarus experiment measures the neutrino speed: even neutrinos are not faster than light
23-02-2012: NEUTRINOS: STATEMENT ISSUED BY THE OPERA COLLABORATION
13-12-2011: ato attuale della ricerca dell’Higgs
18-11-2011: NEW TESTS CONFIRM THE RESULTS OF OPERA ON THE NEUTRINO VELOCITY. BUT IT IS NOT YET THE FINAL CONFIRMATION
26-10-2011: Fernando Ferroni appointed as the president of the Italian National Institute for Nuclear Physics

[Back]

 

Ufficio Comunicazione Infn - Piazza dei Caprettari, 70 - 00186 Roma
Tel: 06 68 68 162 - Fax: 06 68 307 944 - email: comunicazione@presid.infn.it

F.M . F.E.

 

 

 

 

 

 CONFERENCES
11-12-2017
TRANSVERSITY 2017
13-12-2017
SM&FT 2017 : THE XVII WORKSHOP ON STATISTICAL MECHANICS AND NONPERTURBATIVE FIELD THEORY
 REVIEWS AREA
PRESS REVIEWS
VIDEO REVIEWS
 PRESS RELEASE
26-03-2013
OPERA OBSERVED A THIRD NEUTRINO TAU
08-06-2012
NEUTRINOS SENT FROM CERN TO GRAN SASSO RESPECT THE COSMIC SPEED LIMIT
06-06-2012
OPERA OBSERVES THE SECOND TAU NEUTRINO
Ricerca Italiana