A dual tunnel structure for the Einstein Telescope
Riccardo DeSalvo, Emerald Gingell, Jes\'us Leonardo Gonz\'alez L\'opez, Nelson Leon, Marina Mondin, Harry Themann, Fabi\'an Erasmo Pe\~na Arellano

TL;DR
This paper proposes a new dual tunnel architecture for the Einstein Telescope that significantly reduces excavation volume and enhances seismic isolation, stability, and geophysical monitoring capabilities for gravitational wave detection.
Contribution
It introduces a novel dual tunnel design with integrated seismic isolation systems and real-time rock motion monitoring, improving performance and maintenance over traditional approaches.
Findings
Reduces excavation volume by an order of magnitude.
Enhances seismic isolation and stability of the interferometers.
Provides real-time rock motion monitoring for improved noise cancellation.
Abstract
We present a novel tunnel architecture for the Einstein Telescope that departs from the traditional large-cavern approach and reduces the excavated volume by an order of magnitude. In the proposed design, all seismic isolation systems are housed in raise-bore wells drilled upward from the main tunnel toward an upper service tunnel. The pre-isolators for the most sensitive optics are located in the service tunnel, seating directly on strong and compact rock, while the other filters are distributed along the wells within compact, side-access vacuum chambers. Shorter, separate wells accommodate the seismic isolation systems for less demanding optics. This configuration provides substantial advantages: easier lock acquisition and improved robustness of the interferometers, lower-frequency pendulum stages, reduced congestion around the test masses, simplified installation and maintenance,…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Sensor Technology · Advanced Frequency and Time Standards
