Loss in long-storage-time optical cavities

Long-storage-time Fabry-Perot cavities are a core component of many precision measurement experiments. Optical loss in such cavities is a critical parameter in determining their performance; however, it is very difficult to determine a priori from independent characterisation of the individual cavit...

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Main Authors: Isogai, Tomoki, Miller, J., Kwee, Patrick, Barsotti, Lisa, Evans, M.
Other Authors: LIGO (Observatory : Massachusetts Institute of Technology)
Format: Article
Published: Optical Society of America 2019
Online Access:https://hdl.handle.net/1721.1/122799
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author Isogai, Tomoki
Miller, J.
Kwee, Patrick
Barsotti, Lisa
Evans, M.
author2 LIGO (Observatory : Massachusetts Institute of Technology)
author_facet LIGO (Observatory : Massachusetts Institute of Technology)
Isogai, Tomoki
Miller, J.
Kwee, Patrick
Barsotti, Lisa
Evans, M.
author_sort Isogai, Tomoki
collection MIT
description Long-storage-time Fabry-Perot cavities are a core component of many precision measurement experiments. Optical loss in such cavities is a critical parameter in determining their performance; however, it is very difficult to determine a priori from independent characterisation of the individual cavity mirrors. Here, we summarise three techniques for directly measuring this loss in situ and apply them to a high-finesse, near-concentric, 2 m system. Through small modifications of the cavity's length, we explore optical loss as a function of beam spot size over the 1-3 mm range. In this regime we find that optical loss is relatively constant at around 5 ppm per mirror and shows greater dependence on the positions of the beam spots on the cavity optics than on their size. These results have immediate consequences for the application of squeezed light to advanced gravitational-wave interferometers.
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spelling mit-1721.1/1227992022-09-29T23:40:16Z Loss in long-storage-time optical cavities Isogai, Tomoki Miller, J. Kwee, Patrick Barsotti, Lisa Evans, M. LIGO (Observatory : Massachusetts Institute of Technology) Long-storage-time Fabry-Perot cavities are a core component of many precision measurement experiments. Optical loss in such cavities is a critical parameter in determining their performance; however, it is very difficult to determine a priori from independent characterisation of the individual cavity mirrors. Here, we summarise three techniques for directly measuring this loss in situ and apply them to a high-finesse, near-concentric, 2 m system. Through small modifications of the cavity's length, we explore optical loss as a function of beam spot size over the 1-3 mm range. In this regime we find that optical loss is relatively constant at around 5 ppm per mirror and shows greater dependence on the positions of the beam spots on the cavity optics than on their size. These results have immediate consequences for the application of squeezed light to advanced gravitational-wave interferometers. National Science Foundation (U.S.) (Contract PHY-0757058) 2019-11-07T23:03:43Z 2019-11-07T23:03:43Z 2013-11 2019-03-19T17:40:29Z Article http://purl.org/eprint/type/JournalArticle 1094-4087 https://hdl.handle.net/1721.1/122799 Isogai, T., J. Miller, P. Kwee, L. Barsotti, and M. Evans. “Loss in Long-Storage-Time Optical Cavities.” Optics Express 21, 24 (November 2013): 30114 © 2013 Optical Society of America https://doi.org/10.1364/oe.21.030114 Optics Express Creative Commons Attribution-Noncommercial-Share Alike http://creativecommons.org/licenses/by-nc-sa/4.0/ application/pdf Optical Society of America arXiv
spellingShingle Isogai, Tomoki
Miller, J.
Kwee, Patrick
Barsotti, Lisa
Evans, M.
Loss in long-storage-time optical cavities
title Loss in long-storage-time optical cavities
title_full Loss in long-storage-time optical cavities
title_fullStr Loss in long-storage-time optical cavities
title_full_unstemmed Loss in long-storage-time optical cavities
title_short Loss in long-storage-time optical cavities
title_sort loss in long storage time optical cavities
url https://hdl.handle.net/1721.1/122799
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