The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control

F. Kawazoe; G. Bergmann; A. Bertolini; M. Born; Y.B. Chen; A.V. Cummning; L. Cunningham; K. Dahl; C. Graf; G. Hammond; G. Heinzel; S. Hild; S.H. Huttner; R. Jones; S. Kohlenbeck; G. Kuhn; H. Luck; K. Mossavi; J.H. Pold; K. Somiya; A.M. van Veggel; A. Wanner; T. Westphal; B. Winke; K. Strain; S. Gossler; K. Danzmann

doi:10.1088/1742-6596/363/1/012012

The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control

F. Kawazoe^*
, G. Bergmann
, A. Bertolini
, M. Born
, Y.B. Chen
, A.V. Cummning
, L. Cunningham
, K. Dahl
, C. Graf
, G. Hammond
, G. Heinzel
, S. Hild
, S.H. Huttner
, R. Jones
, S. Kohlenbeck
, G. Kuhn
, H. Luck
, K. Mossavi
, J.H. Pold
, K. Somiya

A.M. van Veggel, A. Wanner, T. Westphal, B. Winke, K. Strain, S. Gossler, K. Danzmann

^*Corresponding author for this work

Research output: Contribution to journal › Conference article in journal › Academic › peer-review

Abstract

The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum Limit at frequencies ranging from 20 Hz to 1 kHz with a 10 m arm-length Michelson interferometer named the sub-SQL interferometer. The frequency control system uses a 20 m optical path length triangular suspended cavity named the reference cavity, with the goal of suppressing frequency noise of the input laser to a level of similar to 10(-4) Hz/root Hz at 20 Hz rolling off to below 6 x 10(-6) Hz/root Hz above 1 kHz. It is expected that tight angular control of the reference cavity''s mirrors is necessary to reach this stringent requirement.

Original language	English
Article number	012012
Number of pages	7
Journal	Journal of Physics: Conference Series
Volume	363
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/363/1/012012
Publication status	Published - 2012
Externally published	Yes

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Kawazoe, F., Bergmann, G., Bertolini, A., Born, M., Chen, Y. B., Cummning, A. V., Cunningham, L., Dahl, K., Graf, C., Hammond, G., Heinzel, G., Hild, S., Huttner, S. H., Jones, R., Kohlenbeck, S., Kuhn, G., Luck, H., Mossavi, K., Pold, J. H., ... Danzmann, K. (2012). The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control. Journal of Physics: Conference Series, 363(1), Article 012012. https://doi.org/10.1088/1742-6596/363/1/012012

@article{b23cf2b765a64a2189f4532f84de5434,

title = "The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control",

abstract = "The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum Limit at frequencies ranging from 20 Hz to 1 kHz with a 10 m arm-length Michelson interferometer named the sub-SQL interferometer. The frequency control system uses a 20 m optical path length triangular suspended cavity named the reference cavity, with the goal of suppressing frequency noise of the input laser to a level of similar to 10(-4) Hz/root Hz at 20 Hz rolling off to below 6 x 10(-6) Hz/root Hz above 1 kHz. It is expected that tight angular control of the reference cavity''s mirrors is necessary to reach this stringent requirement.",

author = "F. Kawazoe and G. Bergmann and A. Bertolini and M. Born and Y.B. Chen and A.V. Cummning and L. Cunningham and K. Dahl and C. Graf and G. Hammond and G. Heinzel and S. Hild and S.H. Huttner and R. Jones and S. Kohlenbeck and G. Kuhn and H. Luck and K. Mossavi and J.H. Pold and K. Somiya and \{van Veggel\}, A.M. and A. Wanner and T. Westphal and B. Winke and K. Strain and S. Gossler and K. Danzmann",

year = "2012",

doi = "10.1088/1742-6596/363/1/012012",

language = "English",

volume = "363",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

number = "1",

}

Kawazoe, F, Bergmann, G, Bertolini, A, Born, M, Chen, YB, Cummning, AV, Cunningham, L, Dahl, K, Graf, C, Hammond, G, Heinzel, G, Hild, S, Huttner, SH, Jones, R, Kohlenbeck, S, Kuhn, G, Luck, H, Mossavi, K, Pold, JH, Somiya, K, van Veggel, AM, Wanner, A, Westphal, T, Winke, B, Strain, K, Gossler, S & Danzmann, K 2012, 'The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control', Journal of Physics: Conference Series, vol. 363, no. 1, 012012. https://doi.org/10.1088/1742-6596/363/1/012012

TY - JOUR

T1 - The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control

AU - Kawazoe, F.

AU - Bergmann, G.

AU - Bertolini, A.

AU - Born, M.

AU - Chen, Y.B.

AU - Cummning, A.V.

AU - Cunningham, L.

AU - Dahl, K.

AU - Graf, C.

AU - Hammond, G.

AU - Heinzel, G.

AU - Hild, S.

AU - Huttner, S.H.

AU - Jones, R.

AU - Kohlenbeck, S.

AU - Kuhn, G.

AU - Luck, H.

AU - Mossavi, K.

AU - Pold, J.H.

AU - Somiya, K.

AU - van Veggel, A.M.

AU - Wanner, A.

AU - Westphal, T.

AU - Winke, B.

AU - Strain, K.

AU - Gossler, S.

AU - Danzmann, K.

PY - 2012

Y1 - 2012

N2 - The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum Limit at frequencies ranging from 20 Hz to 1 kHz with a 10 m arm-length Michelson interferometer named the sub-SQL interferometer. The frequency control system uses a 20 m optical path length triangular suspended cavity named the reference cavity, with the goal of suppressing frequency noise of the input laser to a level of similar to 10(-4) Hz/root Hz at 20 Hz rolling off to below 6 x 10(-6) Hz/root Hz above 1 kHz. It is expected that tight angular control of the reference cavity''s mirrors is necessary to reach this stringent requirement.

AB - The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum Limit at frequencies ranging from 20 Hz to 1 kHz with a 10 m arm-length Michelson interferometer named the sub-SQL interferometer. The frequency control system uses a 20 m optical path length triangular suspended cavity named the reference cavity, with the goal of suppressing frequency noise of the input laser to a level of similar to 10(-4) Hz/root Hz at 20 Hz rolling off to below 6 x 10(-6) Hz/root Hz above 1 kHz. It is expected that tight angular control of the reference cavity''s mirrors is necessary to reach this stringent requirement.

U2 - 10.1088/1742-6596/363/1/012012

DO - 10.1088/1742-6596/363/1/012012

M3 - Conference article in journal

SN - 1742-6588

VL - 363

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012012

ER -

The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control

Abstract

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