Feasibility study of beam-expanding telescopes in the interferometer arms for the Einstein Telescope
Samuel Rowlinson (1), Artemiy Dmitriev (1), Aaron Jones (2), Teng, Zhang (1), Andreas Freise (1, 3, 4) ((1) School of Physics and, Astronomy, and Institute of Gravitational Wave Astronomy, (2) OzGrav,, University of Western Australia, (3) Department of Physics, Astronomy, VU

TL;DR
This paper explores the potential use of beam-expander telescopes in the Einstein Telescope's interferometer arms, demonstrating their feasibility and ability to optimize optical mode matching in the detector design.
Contribution
It presents a feasibility analysis and an example implementation of beam-expander telescopes in the Einstein Telescope, enhancing optical layout flexibility and mode matching capabilities.
Findings
Beam-expander telescopes can be integrated into the ET design.
Tuning beam-expander telescopes can compensate for mode mismatches.
The proposed implementation aligns with the 2020 ET design update.
Abstract
The optical design of the Einstein Telescope (ET) is based on a dual-recycled Michelson interferometer with Fabry-Perot cavities in the arms. ET will be constructed in a new infrastructure, allowing us to consider different technical implementations beyond the constraints of the current facilities. In this paper we investigate the feasibility of using beam-expander telescopes in the interferometer arms. We provide an example implementation that matches the optical layout as presented in the ET design update 2020. We further show that the beam-expander telescopes can be tuned to compensate for mode mismatches between the arm cavities and the rest of the interferometer.
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