This article is about the gravitational wave detector. For the X-ray telescope, see Einstein Observatory. For the observatory building in Potsdam, see Einstein Tower.
Einstein Telescope (ET) or Einstein Observatory, is a proposed third-generation ground-based gravitational wave detector, currently under study by some institutions in the European Union. It will be able to test Einstein's general theory of relativity in strong field conditions and realize precision gravitational wave astronomy.
The ET is a design study project supported by the European Commission under the Framework Programme 7 (FP7). It concerns the study and the conceptual design for a new research infrastructure in the emergent field of gravitational-wave astronomy.
Motivation
The evolution of the current gravitational wave detectors Advanced Virgo and Advanced LIGO, as second generation 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 detected gravitational waves in 2015 and Virgo joined this experimental success with the first gravitational wave observed by three detectors GW170814 and shortly after with the first detection of a binary neutron star merger GW170817. 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 seismic noise, the related gravitational gradient noise (so-called Newtonian noise) and the thermal noise of the suspension last stage and of the test masses.
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.[1]
Technical groups
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 and astrophysics potentialities (WP4).
Participants
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 European Gravitational Observatory:[2]
Although still in the early design study phase, the basic parameters are established.[3]
Like KAGRA, it will be located underground to reduce seismic noise and "gravity gradient noise" caused by nearby moving objects.
The arms will be 10 km long (compared to 4 km for LIGO, and 3 km for Virgo and KAGRA), and like LISA, there will be three arms in an equilateral triangle, with two detectors in each corner.
In order to measure the polarization of incoming gravitational waves 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, but that is made up for by the third detector, and the additional redundancy provides a useful cross-check.
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 frequencies.
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.[3]: 15–16 The high-frequency ones (10 Hz to 10 kHz) will use room-temperature optics and a much higher recirculating beam power of 3 MW.[3]: 15
ETpathfinder
A prototype, or testing facility, called the ETpathfinder was built at Maastricht University's Randwyck Campus in the Netherlands.[4] The facility was opened in November 2021 by Dutch Minister of Education, Culture and Science, Ingrid van Engelshoven. Project leader is Professor Stefan Hild. ETpathfinder will be a useful research centre in its own right after the ET has been built. The candidate sites for the ET are the Meuse–Rhine Euroregion, Sardinia, and Saxony. [5][6][7]
The Meuse-Rhine Euroregion proposal
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 Meuse-Rhine Euroregion 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.
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. Laser 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 shafts.
From 2021, Nikhef will carry out exploratory drilling in Terziet, Banholt, 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.
Sos Enattos was chosen for the functional characteristics of the project[11] of the site on the island:
It has been classified as one of the quietest places on earth:[12] the seismic activity that interferes with the detection of gravitational waves is essentially nil.[13]
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.[14]
The presence of groundwater in the area reduces the possibility of having problems with infiltration or seismic and Newtonian noise.[14]
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,[15] with a local induced (65-75% of the total amount) equal to a turnover of 4.329 billion euros.[11]
In January 2021 seismological surveys were carried out to validate the site, installing 15 seismometric stations near the Sos Enattos mine.[16]
In September 2022, the Draghi government mandated the president of INFN Antonio Zoccoli to proceed with the creation of Italy's candidacy dossier,[17][18] confirming the 350 million euro of economic commitment already allocated by the Sardinia Region.[19]
^Stefan Hild; Simon Chelkowski; Andreas Freise (2008-11-24), Pushing towards the ET sensitivity using 'conventional' technology, arXiv:0810.0604, Bibcode:2008arXiv0810.0604H
