Technology for the next gravitational wave detectors

Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. S...
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Autor*in:	Mitrofanov, Valery P. [verfasserIn] Chao, Shiuh [verfasserIn] Pan, Huang-Wei [verfasserIn] Kuo, Ling-Chi [verfasserIn] Cole, Garrett [verfasserIn] Degallaix, Jerome [verfasserIn] Willke, Benno [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	gravitational waves advanced techniques thermal noise coating laser

Übergeordnetes Werk:	Enthalten in: Science in China - Heidelberg : Springer, 2003, 58(2015), 12 vom: 04. Dez.
Übergeordnetes Werk:	volume:58 ; year:2015 ; number:12 ; day:04 ; month:12

Links:	Volltext

DOI / URN:	10.1007/s11433-015-5738-8

Katalog-ID:	SPR019357621

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520			\|a Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers.
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allfields	10.1007/s11433-015-5738-8 doi (DE-627)SPR019357621 (SPR)s11433-015-5738-8-e DE-627 ger DE-627 rakwb eng 530 520 ASE 33.00 bkl 39.00 bkl Mitrofanov, Valery P. verfasserin aut Technology for the next gravitational wave detectors 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers. gravitational waves (dpeaa)DE-He213 advanced techniques (dpeaa)DE-He213 thermal noise (dpeaa)DE-He213 coating (dpeaa)DE-He213 laser (dpeaa)DE-He213 Chao, Shiuh verfasserin aut Pan, Huang-Wei verfasserin aut Kuo, Ling-Chi verfasserin aut Cole, Garrett verfasserin aut Degallaix, Jerome verfasserin aut Willke, Benno verfasserin aut Enthalten in Science in China Heidelberg : Springer, 2003 58(2015), 12 vom: 04. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:58 year:2015 number:12 day:04 month:12 https://dx.doi.org/10.1007/s11433-015-5738-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 33.00 ASE 39.00 ASE AR 58 2015 12 04 12
spelling	10.1007/s11433-015-5738-8 doi (DE-627)SPR019357621 (SPR)s11433-015-5738-8-e DE-627 ger DE-627 rakwb eng 530 520 ASE 33.00 bkl 39.00 bkl Mitrofanov, Valery P. verfasserin aut Technology for the next gravitational wave detectors 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers. gravitational waves (dpeaa)DE-He213 advanced techniques (dpeaa)DE-He213 thermal noise (dpeaa)DE-He213 coating (dpeaa)DE-He213 laser (dpeaa)DE-He213 Chao, Shiuh verfasserin aut Pan, Huang-Wei verfasserin aut Kuo, Ling-Chi verfasserin aut Cole, Garrett verfasserin aut Degallaix, Jerome verfasserin aut Willke, Benno verfasserin aut Enthalten in Science in China Heidelberg : Springer, 2003 58(2015), 12 vom: 04. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:58 year:2015 number:12 day:04 month:12 https://dx.doi.org/10.1007/s11433-015-5738-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 33.00 ASE 39.00 ASE AR 58 2015 12 04 12
allfields_unstemmed	10.1007/s11433-015-5738-8 doi (DE-627)SPR019357621 (SPR)s11433-015-5738-8-e DE-627 ger DE-627 rakwb eng 530 520 ASE 33.00 bkl 39.00 bkl Mitrofanov, Valery P. verfasserin aut Technology for the next gravitational wave detectors 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers. gravitational waves (dpeaa)DE-He213 advanced techniques (dpeaa)DE-He213 thermal noise (dpeaa)DE-He213 coating (dpeaa)DE-He213 laser (dpeaa)DE-He213 Chao, Shiuh verfasserin aut Pan, Huang-Wei verfasserin aut Kuo, Ling-Chi verfasserin aut Cole, Garrett verfasserin aut Degallaix, Jerome verfasserin aut Willke, Benno verfasserin aut Enthalten in Science in China Heidelberg : Springer, 2003 58(2015), 12 vom: 04. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:58 year:2015 number:12 day:04 month:12 https://dx.doi.org/10.1007/s11433-015-5738-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 33.00 ASE 39.00 ASE AR 58 2015 12 04 12
allfieldsGer	10.1007/s11433-015-5738-8 doi (DE-627)SPR019357621 (SPR)s11433-015-5738-8-e DE-627 ger DE-627 rakwb eng 530 520 ASE 33.00 bkl 39.00 bkl Mitrofanov, Valery P. verfasserin aut Technology for the next gravitational wave detectors 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers. gravitational waves (dpeaa)DE-He213 advanced techniques (dpeaa)DE-He213 thermal noise (dpeaa)DE-He213 coating (dpeaa)DE-He213 laser (dpeaa)DE-He213 Chao, Shiuh verfasserin aut Pan, Huang-Wei verfasserin aut Kuo, Ling-Chi verfasserin aut Cole, Garrett verfasserin aut Degallaix, Jerome verfasserin aut Willke, Benno verfasserin aut Enthalten in Science in China Heidelberg : Springer, 2003 58(2015), 12 vom: 04. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:58 year:2015 number:12 day:04 month:12 https://dx.doi.org/10.1007/s11433-015-5738-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 33.00 ASE 39.00 ASE AR 58 2015 12 04 12
allfieldsSound	10.1007/s11433-015-5738-8 doi (DE-627)SPR019357621 (SPR)s11433-015-5738-8-e DE-627 ger DE-627 rakwb eng 530 520 ASE 33.00 bkl 39.00 bkl Mitrofanov, Valery P. verfasserin aut Technology for the next gravitational wave detectors 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers. gravitational waves (dpeaa)DE-He213 advanced techniques (dpeaa)DE-He213 thermal noise (dpeaa)DE-He213 coating (dpeaa)DE-He213 laser (dpeaa)DE-He213 Chao, Shiuh verfasserin aut Pan, Huang-Wei verfasserin aut Kuo, Ling-Chi verfasserin aut Cole, Garrett verfasserin aut Degallaix, Jerome verfasserin aut Willke, Benno verfasserin aut Enthalten in Science in China Heidelberg : Springer, 2003 58(2015), 12 vom: 04. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:58 year:2015 number:12 day:04 month:12 https://dx.doi.org/10.1007/s11433-015-5738-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 33.00 ASE 39.00 ASE AR 58 2015 12 04 12
language	English
source	Enthalten in Science in China 58(2015), 12 vom: 04. Dez. volume:58 year:2015 number:12 day:04 month:12
sourceStr	Enthalten in Science in China 58(2015), 12 vom: 04. Dez. volume:58 year:2015 number:12 day:04 month:12
format_phy_str_mv	Article
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topic_facet	gravitational waves advanced techniques thermal noise coating laser
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container_title	Science in China
authorswithroles_txt_mv	Mitrofanov, Valery P. @@aut@@ Chao, Shiuh @@aut@@ Pan, Huang-Wei @@aut@@ Kuo, Ling-Chi @@aut@@ Cole, Garrett @@aut@@ Degallaix, Jerome @@aut@@ Willke, Benno @@aut@@
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author	Mitrofanov, Valery P.
spellingShingle	Mitrofanov, Valery P. ddc 530 bkl 33.00 bkl 39.00 misc gravitational waves misc advanced techniques misc thermal noise misc coating misc laser Technology for the next gravitational wave detectors
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topic_title	530 520 ASE 33.00 bkl 39.00 bkl Technology for the next gravitational wave detectors gravitational waves (dpeaa)DE-He213 advanced techniques (dpeaa)DE-He213 thermal noise (dpeaa)DE-He213 coating (dpeaa)DE-He213 laser (dpeaa)DE-He213
topic	ddc 530 bkl 33.00 bkl 39.00 misc gravitational waves misc advanced techniques misc thermal noise misc coating misc laser
topic_unstemmed	ddc 530 bkl 33.00 bkl 39.00 misc gravitational waves misc advanced techniques misc thermal noise misc coating misc laser
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title	Technology for the next gravitational wave detectors
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title_full	Technology for the next gravitational wave detectors
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author_browse	Mitrofanov, Valery P. Chao, Shiuh Pan, Huang-Wei Kuo, Ling-Chi Cole, Garrett Degallaix, Jerome Willke, Benno
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title_sort	technology for the next gravitational wave detectors
title_auth	Technology for the next gravitational wave detectors
abstract	Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers.
abstractGer	Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers.
abstract_unstemmed	Abstract This paper reviews some of the key enabling technologies for advanced and future laser interferometer gravitational wave detectors, which must combine test masses with the lowest possible optical and acoustic losses, with high stability lasers and various techniques for suppressing noise. Sect. 1 of this paper presents a review of the acoustic properties of test masses. Sect. 2 reviews the technology of the amorphous dielectric coatings which are currently universally used for the mirrors in advanced laser interferometers, but for which lower acoustic loss would be very advantageous. In sect. 3 a new generation of crystalline optical coatings that offer a substantial reduction in thermal noise is reviewed. The optical properties of test masses are reviewed in sect. 4, with special focus on the properties of silicon, an important candidate material for future detectors. Sect. 5 of this paper presents the very low noise, high stability laser technology that underpins all advanced and next generation laser interferometers.
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title_short	Technology for the next gravitational wave detectors
url	https://dx.doi.org/10.1007/s11433-015-5738-8
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