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Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror

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Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror. / Leavey, S.; Barr, B. W.; Bell, A. S. et al.
In: Classical and Quantum Gravity, Vol. 32, No. 17, 175005, 01.09.2015.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Leavey, S, Barr, BW, Bell, AS, Gordon, N, Gräf, C, Hild, S, Huttner, SH, Kley, E-B, Kroker, S, Macarthur, J, Messenger, C, Pitkin, M, Sorazu, B, Strain, K & Tünnermann, A 2015, 'Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror', Classical and Quantum Gravity, vol. 32, no. 17, 175005. https://doi.org/10.1088/0264-9381/32/17/175005

APA

Leavey, S., Barr, B. W., Bell, A. S., Gordon, N., Gräf, C., Hild, S., Huttner, S. H., Kley, E-B., Kroker, S., Macarthur, J., Messenger, C., Pitkin, M., Sorazu, B., Strain, K., & Tünnermann, A. (2015). Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror. Classical and Quantum Gravity, 32(17), Article 175005. https://doi.org/10.1088/0264-9381/32/17/175005

Vancouver

Leavey S, Barr BW, Bell AS, Gordon N, Gräf C, Hild S et al. Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror. Classical and Quantum Gravity. 2015 Sept 1;32(17):175005. doi: 10.1088/0264-9381/32/17/175005

Author

Leavey, S. ; Barr, B. W. ; Bell, A. S. et al. / Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror. In: Classical and Quantum Gravity. 2015 ; Vol. 32, No. 17.

Bibtex

@article{19dd2c6a54494c39815e1e0622a7e175,
title = "Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror",
abstract = "Waveguide mirrors (WGMs) possess nano-structured surfaces which can potentially provide a significant reduction in thermal noise over conventional dielectric mirrors. To avoid introducing additional phase noise from the motion of the mirror transverse to the reflected light, however, they must possess a mechanism to suppress the phase effects associated with the incident light translating across the nano-structured surface. It has been shown that with carefully chosen parameters this additional phase noise can be suppressed. We present an experimental measurement of the coupling of transverse to longitudinal displacements in such a WGM designed for 1064 nm light. We place an upper limit on the level of measured transverse to longitudinal coupling of one part in seventeen thousand with 95% confidence, representing a significant improvement over a previously measured grating mirror.",
author = "S. Leavey and Barr, {B. W.} and Bell, {A. S.} and N. Gordon and C. Gr{\"a}f and S. Hild and Huttner, {S. H.} and E.-B. Kley and S. Kroker and J. Macarthur and C. Messenger and M. Pitkin and B. Sorazu and K. Strain and A. T{\"u}nnermann",
year = "2015",
month = sep,
day = "1",
doi = "10.1088/0264-9381/32/17/175005",
language = "English",
volume = "32",
journal = "Classical and Quantum Gravity",
issn = "0264-9381",
publisher = "IOP Publishing",
number = "17",

}

RIS

TY - JOUR

T1 - Upper limit to the transverse to longitudinal motion coupling of a waveguide mirror

AU - Leavey, S.

AU - Barr, B. W.

AU - Bell, A. S.

AU - Gordon, N.

AU - Gräf, C.

AU - Hild, S.

AU - Huttner, S. H.

AU - Kley, E.-B.

AU - Kroker, S.

AU - Macarthur, J.

AU - Messenger, C.

AU - Pitkin, M.

AU - Sorazu, B.

AU - Strain, K.

AU - Tünnermann, A.

PY - 2015/9/1

Y1 - 2015/9/1

N2 - Waveguide mirrors (WGMs) possess nano-structured surfaces which can potentially provide a significant reduction in thermal noise over conventional dielectric mirrors. To avoid introducing additional phase noise from the motion of the mirror transverse to the reflected light, however, they must possess a mechanism to suppress the phase effects associated with the incident light translating across the nano-structured surface. It has been shown that with carefully chosen parameters this additional phase noise can be suppressed. We present an experimental measurement of the coupling of transverse to longitudinal displacements in such a WGM designed for 1064 nm light. We place an upper limit on the level of measured transverse to longitudinal coupling of one part in seventeen thousand with 95% confidence, representing a significant improvement over a previously measured grating mirror.

AB - Waveguide mirrors (WGMs) possess nano-structured surfaces which can potentially provide a significant reduction in thermal noise over conventional dielectric mirrors. To avoid introducing additional phase noise from the motion of the mirror transverse to the reflected light, however, they must possess a mechanism to suppress the phase effects associated with the incident light translating across the nano-structured surface. It has been shown that with carefully chosen parameters this additional phase noise can be suppressed. We present an experimental measurement of the coupling of transverse to longitudinal displacements in such a WGM designed for 1064 nm light. We place an upper limit on the level of measured transverse to longitudinal coupling of one part in seventeen thousand with 95% confidence, representing a significant improvement over a previously measured grating mirror.

U2 - 10.1088/0264-9381/32/17/175005

DO - 10.1088/0264-9381/32/17/175005

M3 - Journal article

VL - 32

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

SN - 0264-9381

IS - 17

M1 - 175005

ER -