Fulda, Paul, Kokeyama, Keiko ![]() |
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Abstract
The compatibility of higher-order Laguerre-Gauss (LG) modes with interferometric technologies commonly used in gravitational wave detectors is investigated. In this paper, we present the first experimental results concerning the performance of the LG 33 mode in optical resonators. We show that the Pound-Drever-Hall error signal for a LG 33 mode in a linear optical resonator is identical to that of the more commonly used LG 00 mode, and demonstrate the feedback control of the resonator with a LG 33 mode. We succeeded to increase the mode purity of a LG 33 mode generated using a spatial-light modulator from 51% to 99% upon transmission through a linear optical resonator. We further report the experimental verification that a triangular optical resonator does not transmit helical LG modes.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | American Physical Society |
ISSN: | 1550-7998 |
Date of First Compliant Deposit: | 19 March 2021 |
Date of Acceptance: | 22 April 2010 |
Last Modified: | 03 May 2023 18:50 |
URI: | https://orca.cardiff.ac.uk/id/eprint/139935 |
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