Environmental Noise Challenges for the Einstein Telescope - A Review
Abstract
Einstein Telescope (ET) will be a next-generation ground based interferometric gravitational-wave detector designed to explore the Universe to an unprecedented depth and detail. With its 10-15 km long arms, underground infrastructure, and advanced cryogenic technologies to suppress thermal noise, ET aims at achieving a sensitivity up to eight orders of magnitude better than current detectors such as Virgo, LIGO, and KAGRA. The coverage of the low-frequency band, starting at 2 Hz, will enable the observation of earlier inspiral phases of compact binary coalescences, enhancing early-warning capabilities and improving multi-messenger follow-up. However, this increased sensitivity also implies a higher susceptibility to environmental disturbances, particularly in the 2-10 Hz range where anthropogenic, seismic and infrastructural noise noise are most relevant. Therefore, understanding and mitigating environmental contributions are essential to fully exploit the scientific potential of ET. This chapter reviews the ongoing studies on environmental noise for ET, summarizes the main challenges related to site characterization and infrastructure design and outlines the strategies currently under development to ensure optimal detector performance.
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BibTeX
@misc{giovanni2026environmental,
title = {{Environmental Noise Challenges for the Einstein Telescope - A Review}},
author = {Matteo Di Giovanni},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2608.07633},
eprint = {2608.07633},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2608.07633},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Environmental Noise Challenges for the Einstein Telescope - A Review
AU - Matteo Di Giovanni
PY - 2026
DA - 2026/10/29
PB - arXiv
DO - 10.48550/arxiv.2608.07633
UR - https://arxiv.org/abs/2608.07633
AB - Einstein Telescope (ET) will be a next-generation ground based interferometric gravitational-wave detector designed to explore the Universe to an unprecedented depth and detail. With its 10-15 km long arms, underground infrastructure, and advanced cryogenic technologies to suppress thermal noise, ET aims at achieving a sensitivity up to eight orders of magnitude better than current detectors such as Virgo, LIGO, and KAGRA. The coverage of the low-frequency band, starting at 2 Hz, will enable the observation of earlier inspiral phases of compact binary coalescences, enhancing early-warning capabilities and improving multi-messenger follow-up. However, this increased sensitivity also implies a higher susceptibility to environmental disturbances, particularly in the 2-10 Hz range where anthropogenic, seismic and infrastructural noise noise are most relevant. Therefore, understanding and mitigating environmental contributions are essential to fully exploit the scientific potential of ET. This chapter reviews the ongoing studies on environmental noise for ET, summarizes the main challenges related to site characterization and infrastructure design and outlines the strategies currently under development to ensure optimal detector performance.
ER -