GEMINI: The First Underground Testbed for Seismic Isolation and Interplatform Control in Next-Generation Gravitational-Wave Detectors

Fuente: arXiv
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Auteurs principaux: Andric, Tomislav, Harms, Jan, Caravella, Ilaria, Angiolilli, Michele, Cortis, Daniele, D'Ambrosio, Nicola, De Deo, Massimiliano, D'Incecco, Marco, Di Ludovico, Antonio, Gerberding, Oliver, Lalli, Alessandro, Lantz, Brian, Leonzi, Laura, Macolino, Carla, Mittleman, Richard, Mow-Lowry, Conor, Orlandi, Donato, Pirro, Stefano, Ricci, Marco, Rollins, Jamie, Warner, Jim
Format: Preprint
Publié: 2025
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author Andric, Tomislav
Harms, Jan
Caravella, Ilaria
Angiolilli, Michele
Cortis, Daniele
D'Ambrosio, Nicola
De Deo, Massimiliano
D'Incecco, Marco
Di Ludovico, Antonio
Gerberding, Oliver
Lalli, Alessandro
Lantz, Brian
Leonzi, Laura
Macolino, Carla
Mittleman, Richard
Mow-Lowry, Conor
Orlandi, Donato
Pirro, Stefano
Ricci, Marco
Rollins, Jamie
Warner, Jim
author_facet Andric, Tomislav
Harms, Jan
Caravella, Ilaria
Angiolilli, Michele
Cortis, Daniele
D'Ambrosio, Nicola
De Deo, Massimiliano
D'Incecco, Marco
Di Ludovico, Antonio
Gerberding, Oliver
Lalli, Alessandro
Lantz, Brian
Leonzi, Laura
Macolino, Carla
Mittleman, Richard
Mow-Lowry, Conor
Orlandi, Donato
Pirro, Stefano
Ricci, Marco
Rollins, Jamie
Warner, Jim
contents GEMINI is an underground research and development facility dedicated to advancing seismic isolation and control technologies for future gravitational-wave observatories, including the Einstein Telescope (ET) and the Lunar Gravitational-Wave Antenna (LGWA). This paper presents the technical design and theoretical framework of GEMINI's active seismic isolation platforms, including detailed noise budget analyses, performance predictions, and residual platform motion evaluations. The GEMINI platforms are designed to achieve unprecedented vibration isolation, targeting motion suppression across the 10 mHz to 10 Hz frequency band, and with the goal to make them the quietest platforms of their kind. In the context of ET, GEMINI will enable the development and validation of inter-platform control strategies essential for the stabilization of auxiliary degrees of freedom of its interferometers. GEMINI will also support the testing of cryogenic payloads and ultra-sensitive inertial sensors required for LGWA. By integrating advanced cryogenic systems, precision inertial sensors, and state-of-the-art vibration isolation technologies, GEMINI will serve as a versatile testbed for next-generation ground-based gravitational-wave detectors and lunar seismometry missions.
format Preprint
id arxiv_https___arxiv_org_abs_2509_04730
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle GEMINI: The First Underground Testbed for Seismic Isolation and Interplatform Control in Next-Generation Gravitational-Wave Detectors
Andric, Tomislav
Harms, Jan
Caravella, Ilaria
Angiolilli, Michele
Cortis, Daniele
D'Ambrosio, Nicola
De Deo, Massimiliano
D'Incecco, Marco
Di Ludovico, Antonio
Gerberding, Oliver
Lalli, Alessandro
Lantz, Brian
Leonzi, Laura
Macolino, Carla
Mittleman, Richard
Mow-Lowry, Conor
Orlandi, Donato
Pirro, Stefano
Ricci, Marco
Rollins, Jamie
Warner, Jim
Instrumentation and Detectors
GEMINI is an underground research and development facility dedicated to advancing seismic isolation and control technologies for future gravitational-wave observatories, including the Einstein Telescope (ET) and the Lunar Gravitational-Wave Antenna (LGWA). This paper presents the technical design and theoretical framework of GEMINI's active seismic isolation platforms, including detailed noise budget analyses, performance predictions, and residual platform motion evaluations. The GEMINI platforms are designed to achieve unprecedented vibration isolation, targeting motion suppression across the 10 mHz to 10 Hz frequency band, and with the goal to make them the quietest platforms of their kind. In the context of ET, GEMINI will enable the development and validation of inter-platform control strategies essential for the stabilization of auxiliary degrees of freedom of its interferometers. GEMINI will also support the testing of cryogenic payloads and ultra-sensitive inertial sensors required for LGWA. By integrating advanced cryogenic systems, precision inertial sensors, and state-of-the-art vibration isolation technologies, GEMINI will serve as a versatile testbed for next-generation ground-based gravitational-wave detectors and lunar seismometry missions.
title GEMINI: The First Underground Testbed for Seismic Isolation and Interplatform Control in Next-Generation Gravitational-Wave Detectors
topic Instrumentation and Detectors
url https://arxiv.org/abs/2509.04730