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Related papers: The 10m AEI prototype facility A brief overview

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At present a 10\,m prototype interferometer facility is being set up at the AEI Hannover. One unique feature of the prototype will be the suspension platform interferometer (SPI). The purpose of the SPI is to monitor and stabilise the…

The 10m Prototype facility at the Albert-Einstein-Institute (AEI) in Hanover, Germany, employs three large seismic attenuation systems to reduce mechanical motion. The AEI Seismic-Attenuation-System (AEI-SAS) uses mechanical anti-springs in…

Recent advances in atom interferometry have led to the development of quantum inertial sensors with outstanding performance in terms of sensitivity, accuracy, and long-term stability. For ground-based implementations, these sensors are…

This Technical Design Report presents AION-10, a 10-meter atom interferometer to be located at Oxford University using ultracold strontium atoms to make precision measurements of fundamental physics. AION-10 serves as both a prototype for…

The Einstein Telescope (ET) will be the next generation gravitational wave observatory in Europe with a sensitivity reaching beyond the CMB into the dark era of the Universe. Each corner of the triangular baseline design is the center of…

Instrumentation and Methods for Astrophysics · Physics 2025-08-25 Thomas Höhn , Adrian Schwenck , Thomas Thümmler , Joachim Wolf , Ralph Engel , Andreas Haungs , Einstein Telescope Pathfinder , collaboration

The AION project has built a tabletop prototype of a single-photon long-baseline atom interferometer using the 87Sr clock transition - a type of quantum sensor designed to search for dark matter and gravitational waves. Our prototype…

The third-generation of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer (CE), aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current…

Instrumentation and Methods for Astrophysics · Physics 2022-10-05 A. Utina , A. Amato , J. Arends , C. Arina , M. de Baar , M. Baars , P. Baer , N. van Bakel , W. Beaumont , A. Bertolini , M. van Beuzekom , S. Biersteker , A. Binetti , H. J. M. ter Brake , G. Bruno , J. Bryant , H. J. Bulten , L. Busch , P. Cebeci , C. Collette , S. Cooper , R. Cornelissen , P. Cuijpers , M. van Dael , S. Danilishin , D. Dixit , S. van Doesburg , M. Doets , R. Elsinga , V. Erends , J. van Erps , A. Freise , H. Frenaij , R. Garcia , M. Giesberts , S. Grohmann , H. Van Haevermaet , S. Heijnen , J. V. van Heijningen , E. Hennes , J. -S. Hennig , M. Hennig , T. Hertog , S. Hild , H. -D. Hoffmann , G. Hoft , M. Hopman , D. Hoyland , G. A. Iandolo , C. Ietswaard , R. Jamshidi , P. Jansweijer , A. Jones , P. Jones , N. Knust , G. Koekoek , X. Koroveshi , T. Kortekaas , A. N. Koushik , M. Kraan , M. van de Kraats , S. L. Kranzhoff , P. Kuijer , K. A. Kukkadapu , K. Lam , N. Letendre , P. Li , R. Limburg , F. Linde , J. -P. Locquet , P. Loosen , H. Lueck , M. Martınez , A. Masserot , F. Meylahn , M. Molenaar , C. Mow-Lowry , J. Mundet , B. Munneke , L. van Nieuwland , E. Pacaud , D. Pascucci , S. Petit , Z. Van Ranst , G. Raskin , P. M. Recaman , N. van Remortel , L. Rolland , L. de Roo , E. Roose , J. C. Rosier , D. Ryckbosch , K. Schouteden , A. Sevrin , A. Sider , A. Singha , V. Spagnuolo , A. Stahl , J. Steinlechner , S. Steinlechner , B. Swinkels , N. Szilasi , M. Tacca , H. Thienpont , A. Vecchio , H. Verkooijen , C. H. Vermeer , M. Vervaeke , G. Visser , R. Walet , P. Werneke , C. Westhofen , B. Willke , A. Xhahi , T. Zhang

Long-baseline laser-interferometer gravitational-wave detectors are operating at a factor of 10 (in amplitude) above the standard quantum limit (SQL) within a broad frequency band. Such a low classical noise budget has already allowed the…

The second generation of large scale interferometric gravitational wave detectors will be limited by quantum noise over a wide frequency range in their detection band. Further sensitivity improvements for future upgrades or new detectors…

We propose two distinct atom interferometer gravitational wave detectors, one terrestrial and another satellite-based, utilizing the core technology of the Stanford 10 m atom interferometer presently under construction. Each configuration…

General Relativity and Quantum Cosmology · Physics 2009-01-07 Savas Dimopoulos , Peter W. Graham , Jason M. Hogan , Mark A. Kasevich , Surjeet Rajendran

We propose an atom interferometer gravitational wave detector in low Earth orbit (AGIS-LEO). Gravitational waves can be observed by comparing a pair of atom interferometers separated over a ~30 km baseline. In the proposed configuration,…

Current gravitational-wave detectors have achieved remarkable sensitivity around 100 Hz, enabling ground-breaking discoveries. Enhancing sensitivity at higher frequencies in the kilohertz (kHz) range promises access to rich physics,…

Homodyne Quadrature Interferometers (HoQIs) are compact, low noise and high dynamic range displacement sensors designed for use in gravitational wave observatories. Their lower noise compared to the displacement sensors used at present…

Atom interferometry represents a quantum leap in the technology for the ultra-precise monitoring of accelerations and rotations and, therefore, for all the science that relies on the latter quantities. These sensors evolved from a new kind…

Recently, the design study `Einstein gravitational wave Telescope' (ET) has been funded within the European FP7 framework. The ambitious goal of this project is to provide a conceptual design of a detector with a hundred times better…

General Relativity and Quantum Cosmology · Physics 2008-11-24 Stefan Hild , Simon Chelkowski , Andreas Freise

We present results from exploratory studies, supported by the Physics Beyond Colliders (PBC) Study Group, of the suitability of a CERN site and its infrastructure for hosting a vertical atom interferometer (AI) with a baseline of about 100…

We propose two distinct atom interferometer gravitational wave detectors, one terrestrial and another satellite-based, utilizing the core technology of the Stanford $10 \text{m}$ atom interferometer presently under construction. The…

General Relativity and Quantum Cosmology · Physics 2009-06-22 Savas Dimopoulos , Peter W. Graham , Jason M. Hogan , Mark A. Kasevich , Surjeet Rajendran

Atom interferometer (AI) experiments offer interesting prospects for searches for the interactions of ultralight bosonic dark matter with Standard Model particles as well as detection of gravitational waves in a frequency band inaccessible…

Absolute gravimeters (AG) are used in geodesy, geophysics, and physics for a wide spectrum of applications. Stable gravimetric measurements over timescales from several days to decades are required to provide relevant insight into…

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