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Design and sensitivity of a 6-axis seismometer for gravitational wave observatories

Leonid Prokhorov1,*, Sam Cooper1, Amit Singh Ubhi1, Conor Mow-Lowry1,2,3, John Bryant1, Artemiy Dmitriev1, Chiara Di Fronzo1, Christopher J. Collins1, Alex Gill1 et al.

Alexandra Mitchell2,3, Joscha Heinze1, Jiri Smetana1, Tianliang Yan1, Alan V. Cumming4, Giles Hammond4, and Denis Martynov1

  • 1Institute for Gravitational Wave Astronomy, School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT, United Kingdom
  • 2Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV, Amsterdam, Netherlands
  • 3Dutch National Institute for Subatomic Physics, Nikhef, 1098 XG, Amsterdam, Netherlands
  • 4Institute for Gravitational Wave Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom

  • *l.g.prokhorov@bham.ac.uk

Phys. Rev. D 109, 042007 – Published 20 February, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.042007

Abstract

We present the design, control system, and noise analysis of a 6-axis seismometer comprising a mass suspended by a single fused silica fiber. We utilize custom-made, compact Michelson interferometers for the readout of the mass motion relative to the table and successfully overcome the sensitivity of existing commercial seismometers by over an order of magnitude in the angular degrees of freedom. We develop the sensor for gravitational-wave observatories, such as LIGO, Virgo, and KAGRA, to help them observe intermediate-mass black holes, increase their duty cycle, and improve localization of sources. Our control system and its achieved sensitivity makes the sensor suitable for other fundamental physics experiments, such as tests of semiclassical gravity, searches for bosonic dark matter, and studies of the Casimir force.

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