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Einstein Telescope

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471: 404:, Cottessen and various locations in the German-Belgian border area. In April 2022, the Dutch gouvernment made €42 million available from the National Growth Fund for preparatory work of the ET and also reserved €870 million for construction. As the Einstein Telescope is an international project, the Netherlands, Belgium and Germany are cooperating in feasibility studies for the telescope in the Meuse-Rhine Euroregion. For example, studies are under way into the differences in planning laws and regulations and their significance for the project. Ultimately, these feasibility studies should lead to a bid book, which will be ready in 2025 at the earliest. 810:
Carlo; Cardini, Alessandro; Paoletti, Federico; Fiori, Irene; Harms, Jan; Majorana, Ettore; Rapagnani, Piero; Ricci, Fulvio; Punturo, Michele; et al. (Matteo Di Giovanni, Carlo Giunchi, Gilberto Saccorotti, Andrea Berbellini, Lapo Boschi, Marco Olivieri, Rosario De Rosa, Luca Naticchioni, Giacomo Oggiano, Massimo Carpinelli, Domenico D’Urso, Stefano Cuccuru, Valeria Sipala, Enrico Calloni, Luciano Di Fiore, Aniello Grado, Carlo Migoni, Alessandro Cardini, Federico Paoletti, Irene Fiori, Jan Harms, Ettore Majorana, Piero Rapagnani, Fulvio Ricci, Michele Punturo) (2020).
86: 64: 46: 171:. Nevertheless, the sensitivity needed to test Einstein's theory of gravity in strong field conditions or to realize a precision gravitational wave astronomy, mainly of massive stellar bodies or of highly asymmetric (in mass) binary stellar systems, goes beyond the expected performances of the advanced detectors and of their subsequent upgrades. For example, the fundamental limitations at low frequency of the sensitivity of the second generation detectors are given by the 283: 271: 207: 295: 259: 231: 247: 219: 485: 187:
Through its four technical working groups, the ET-FP7 project is addressing the basic questions in the realization of this proposed observatory: site location and characteristics (WP1), suspension design and technologies (WP2), detector topology and geometry (WP3), detection capabilities requirements
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beams run through the 10-kilometre arms, the tunnel tubes. A laser beam is split into two beams and these are reflected by mirrors at the ends of the arms in the underground chambers. From the three vertices, a lift will reach ground level. Maintenance will be carried out inside the tunnel via these
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and avoid having an orientation to which the telescope is insensitive, a minimum of two detectors are required. While this could be done with two 90° interferometers at 45° to each other, the triangular form allows the arms to be shared. The 60° arm angle reduces each interferometer's sensitivity,
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Di Giovanni, Matteo; Giunchi, Carlo; Saccorotti, Gilberto; Berbellini, Andrea; Boschi, Lapo; Olivieri, Marco; De Rosa, Rosario; Naticchioni, Luca; Oggiano, Giacomo; Carpinelli, Massimo; d'Urso, Domenico; Cuccuru, Stefano; Sipala, Valeria; Calloni, Enrico; Di Fiore, Luciano; Grado, Aniello; Migoni,
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The low-frequency interferometers (1 to 250 Hz) will use optics cooled to 10 K (−441.7 °F; −263.1 °C), with a beam power of about 18 kW in each arm cavity. The high-frequency ones (10 Hz to 10 kHz) will use room-temperature optics and a much higher recirculating
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To circumvent these limitations new infrastructures are necessary: an underground site for the detector, to limit the effect of the seismic noise, and cryogenic facilities to cool down the mirrors to directly reduce the thermal vibration of the test masses.
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The Einstein Telescope in the Meuse-Rhine Euroregion involves a triangular-shaped tunnel with arms of 10 kilometres long. The telescope will be located 250 to 300 metres underground. At the three vertices there will be large underground chambers.
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The impact on employment would be impressive: in the 9 years of construction, considering direct and induced effects, employment is estimated at 36,000 units, with a local induced (65-75% of the total amount) equal to a turnover of 4.329 billion
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has stable ground with little disturbance to the environment. But it also has a network of knowledge partners to cooperate with, companies that can supply the high-tech, and pleasant, accessible living and working environments.
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The presence of an underground mine that would be used for the allocation of the telescope: the solidity and stability of the rock make it possible to build large underground quarries with confidence.
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ET is a design study project in the European Framework Programme (FP7). It has been proposed by 8 European leading gravitational wave experimental research institutes, coordinated by the
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detectors, is well defined. Currently they have been upgraded to their so-called enhanced level and they are expected to reach their design sensitivity in the next few years. LIGO
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Antonio Zoccoli to proceed with the creation of Italy's candidacy dossier, confirming the 350 million euro of economic commitment already allocated by the Sardinia Region.
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It has been classified as one of the quietest places on earth: the seismic activity that interferes with the detection of gravitational waves is essentially nil.
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Each of the three detectors would be composed of two interferometers, one optimized for operation below 30 Hz and one optimized for operation at higher
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In 2015, the Meuse-Rhine Euroregion, specifically the rural area between Maastricht, Liège and Aachen, was mentioned as one of the ET's possible sites. The
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In January 2021 seismological surveys were carried out to validate the site, installing 15 seismometric stations near the Sos Enattos mine.
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gravitational waves in 2015 and Virgo joined this experimental success with the first gravitational wave observed by three detectors
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The presence of groundwater in the area reduces the possibility of having problems with infiltration or seismic and Newtonian noise.
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The arms will be 10 km long (compared to 4 km for LIGO, and 3 km for Virgo and KAGRA), and like
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but that is made up for by the third detector, and the additional redundancy provides a useful cross-check.
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Sos Enattos was chosen for the functional characteristics of the project of the site on the island:
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Although still in the early design study phase, the basic parameters are established.
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This article is about the gravitational wave detector. For the X-ray telescope, see
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The ET is a design study project supported by the European Commission under the
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in strong field conditions and realize precision gravitational wave astronomy.
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and shortly after with the first detection of a binary neutron star merger
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A prototype, or testing facility, called the ETpathfinder was built at
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Prototype Einstein Telescope komt in pand 'zwarte doos' in Maastricht
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Pushing towards the ET sensitivity using 'conventional' technology
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Einstein gravitational wave Telescope conceptual design study
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and "gravity gradient noise" caused by nearby moving objects.
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Max-Planck-Gesellschaft zur Förderung der Wissenschaften e. V.
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Einstein gravitational wave telescope conceptual design study
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Fundamentals of Interferometric Gravitational Wave Detectors
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Stefan Hild; Simon Chelkowski; Andreas Freise (2008-11-24),
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detector, currently under study by some institutions in the
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The evolution of the current gravitational wave detectors
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Gravity's Shadow: The Search for Gravitational Waves
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For the observatory building in Potsdam, see 1958:Interferometric gravitational-wave instruments 112:, is a proposed third-generation ground-based 1686:(first-ever possible light from bh-bh merger) 1117: 8: 252:Centre National de la Recherche Scientifique 30: 524:, a gravitational wave detector located in 317:, it will be located underground to reduce 1628: 1511: 1353: 1174: 1163: 1124: 1110: 1102: 361:Minister of Education, Culture and Science 240:Max-Planck-Institut für Gravitationsphysik 84: 62: 44: 29: 573: 1698:(first black hole - neutron star merger) 679:'ET - Site Studies and Characterization' 663:'Looking back on ETpathfinder's opening' 506:, the European Gravitational Observatory 556: 188:and astrophysics potentialities (WP4). 872: 870: 779: 777: 697:, 'indico.ego-gw.it', 20 August 2022. 624:(Report). ET-0106C-10. Archived from 615: 613: 611: 224:Istituto Nazionale di Fisica Nucleare 7: 1256:Stanford gravitational wave detector 923:Inaf, Redazione Media (2021-01-20). 375:The Meuse-Rhine Euroregion proposal 1408:European Gravitational Observatory 1005:Consiglio regionale della Sardegna 212:European Gravitational Observatory 198:European Gravitational Observatory 14: 1973:Proposed infrastructure in Europe 1692:(first-ever "mass gap" collision) 1075:Traveling at the Speed of Thought 620:ET Science Team (June 28, 2011). 483: 469: 293: 281: 269: 257: 245: 229: 217: 205: 1149:Gravitational-wave observatory 1096:Website Einstein Telescope EMR 1047:Einstein's Unfinished Symphony 999:Stampa, Ufficio (2022-03-16). 816:Seismological Research Letters 367:. Project leader is Professor 58:gravitational-wave observatory 1: 1841:Gravitational wave background 1393:LIGO Scientific Collaboration 1968:Astronomical interferometers 1644:First observation (GW150914) 1430:TAMA 20, later known as LISM 1133:Gravitational-wave astronomy 952:. 2022-09-27. Archived from 596:ET Design Study Participants 137:gravitational-wave astronomy 126:general theory of relativity 1778:Tests of general relativity 499:Tests of general relativity 133:Framework Programme 7 (FP7) 16:Gravitational wave detector 1989: 1440:Caltech 40m interferometer 455:mandated the president of 120:. It will be able to test 18: 1139: 695:'ET SPB and WP4 of ET-PP' 347:beam power of 3 MW. 92: 1881:Supermassive black holes 905:(in Italian). 2022-03-16 791:(in Italian). 2020-11-25 714:(in Italian). 2023-03-07 264:University of Birmingham 1720:Resonant mass detectors 667:maastrichtuniversity.nl 451:In September 2022, the 544:Taiji Program in Space 381:Meuse-Rhine Euroregion 365:Ingrid van Engelshoven 1905:Rotating neutron star 1716:Laser interferometers 1077:by Daniel Kennefick, 1049:by Marcia Bartusiak, 357:Maastricht University 276:University of Glasgow 1797:Effects / properties 1726:Atom interferometers 1639:List of observations 1566:Pulsar timing arrays 408:The Italian proposal 110:Einstein Observatory 54:Telescope style 21:Einstein Observatory 1886:Stellar black holes 1866:quantum fluctuation 1746:Pulsar timing array 1733:Indirect detection 1673:neutron star merger 1456:INDIGO (LIGO-India) 584:2008arXiv0810.0604H 333:gravitational waves 32: 1773:General relativity 1477:Einstein Telescope 1379:Fermilab holometer 1144:Gravitational wave 1063:by Harry Collins, 828:10.1785/0220200186 669:, 9 November 2021. 628:on October 4, 2017 601:2016-08-15 at the 414:Italian government 300:Cardiff University 114:gravitational wave 106:Einstein Telescope 31:Einstein Telescope 1945: 1944: 1761: 1760: 1712:Direct detection 1560: 1559: 1556: 1555: 1538:Big Bang Observer 1501: 1500: 1341: 1340: 1083:978-0-691-11727-0 789:L'Unione Sarda.it 685:, 20 August 2022. 453:Draghi government 422:Nobel prizewinner 238:, acting through 157:second generation 103: 102: 1980: 1877:Binary inspiral 1871:Phase transition 1862:Cosmic inflation 1629: 1512: 1354: 1175: 1164: 1126: 1119: 1112: 1103: 1033:Peter R. 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Index

Einstein Observatory
Einstein Tower
Albert Einstein
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gravitational-wave observatory
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www.et-gw.eu
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edit on Wikidata
gravitational wave
European Union
Einstein
general theory of relativity
Framework Programme 7 (FP7)
gravitational-wave astronomy
Advanced Virgo
Advanced LIGO
detected
GW170814
GW170817
seismic noise
European Gravitational Observatory
European Union
European Gravitational Observatory
Italy
Istituto Nazionale di Fisica Nucleare
Germany
Max-Planck-Gesellschaft zur Förderung der Wissenschaften e. V.
Max-Planck-Institut für Gravitationsphysik
France

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