248 related articles for article (PubMed ID: 22540781)
1. Reduction of thermal fluctuations in a cryogenic laser interferometric gravitational wave detector.
Uchiyama T; Miyoki S; Telada S; Yamamoto K; Ohashi M; Agatsuma K; Arai K; Fujimoto MK; Haruyama T; Kawamura S; Miyakawa O; Ohishi N; Saito T; Shintomi T; Suzuki T; Takahashi R; Tatsumi D
Phys Rev Lett; 2012 Apr; 108(14):141101. PubMed ID: 22540781
[TBL] [Abstract][Full Text] [Related]
2. Alignment of an interferometric gravitational wave detector.
Fritschel P; Mavalvala N; Shoemaker D; Sigg D; Zucker M; González G
Appl Opt; 1998 Oct; 37(28):6734-47. PubMed ID: 18301487
[TBL] [Abstract][Full Text] [Related]
3. Twin mirrors for laser interferometric gravitational-wave detectors.
Sassolas B; Benoît Q; Flaminio R; Forest D; Franc J; Galimberti M; Lacoudre A; Michel C; Montorio JL; Morgado N; Pinard L
Appl Opt; 2011 May; 50(13):1894-9. PubMed ID: 21532671
[TBL] [Abstract][Full Text] [Related]
4. Mirror-orientation noise in a Fabry-Perot interferometer gravitational wave detector.
Kawamura S; Zucker ME
Appl Opt; 1994 Jun; 33(18):3912-8. PubMed ID: 20935736
[TBL] [Abstract][Full Text] [Related]
5. Calculation method for light scattering caused by multilayer coated mirrors in gravitational wave detectors.
Zeidler S; Akutsu T; Torii Y; Hirose E; Aso Y; Flaminio R
Opt Express; 2017 Mar; 25(5):4741-4760. PubMed ID: 28380744
[TBL] [Abstract][Full Text] [Related]
6. Damping and local control of mirror suspensions for laser interferometric gravitational wave detectors.
Strain KA; Shapiro BN
Rev Sci Instrum; 2012 Apr; 83(4):044501. PubMed ID: 22559557
[TBL] [Abstract][Full Text] [Related]
7. Thermoelastic-damping noise from sapphire mirrors in a fundamental-noise-limited interferometer.
Black ED; Villar A; Libbrecht KG
Phys Rev Lett; 2004 Dec; 93(24):241101. PubMed ID: 15697789
[TBL] [Abstract][Full Text] [Related]
8. Analytical model for ring heater thermal compensation in the Advanced Laser Interferometer Gravitational-wave Observatory.
Ramette J; Kasprzack M; Brooks A; Blair C; Wang H; Heintze M
Appl Opt; 2016 Apr; 55(10):2619-25. PubMed ID: 27139664
[TBL] [Abstract][Full Text] [Related]
9. Low Mechanical Loss TiO_{2}:GeO_{2} Coatings for Reduced Thermal Noise in Gravitational Wave Interferometers.
Vajente G; Yang L; Davenport A; Fazio M; Ananyeva A; Zhang L; Billingsley G; Prasai K; Markosyan A; Bassiri R; Fejer MM; Chicoine M; Schiettekatte F; Menoni CS
Phys Rev Lett; 2021 Aug; 127(7):071101. PubMed ID: 34459624
[TBL] [Abstract][Full Text] [Related]
10. Invited article: CO2 laser production of fused silica fibers for use in interferometric gravitational wave detector mirror suspensions.
Heptonstall A; Barton MA; Bell A; Cagnoli G; Cantley CA; Crooks DR; Cumming A; Grant A; Hammond GD; Harry GM; Hough J; Jones R; Kelley D; Kumar R; Martin IW; Robertson NA; Rowan S; Strain KA; Tokmakov K; van Veggel M
Rev Sci Instrum; 2011 Jan; 82(1):011301. PubMed ID: 21280809
[TBL] [Abstract][Full Text] [Related]
11. Room-temperature tests of an optical transducer for resonant gravitational wave detectors.
Pang Y; Richard JP
Appl Opt; 1995 Aug; 34(22):4982-8. PubMed ID: 21052342
[TBL] [Abstract][Full Text] [Related]
12. A step-wise steerable source of illumination for low-noise "Violin-Mode" shadow sensors, intended for use in interferometric gravitational wave detectors.
Lockerbie NA; Tokmakov KV
Rev Sci Instrum; 2016 Jan; 87(1):015001. PubMed ID: 26827344
[TBL] [Abstract][Full Text] [Related]
13. Optical motion sensor for resonant-bar gravitational wave antennas.
Richard JP; Pang Y; Hamilton JJ
Appl Opt; 1992 Apr; 31(10):1641-5. PubMed ID: 20720800
[TBL] [Abstract][Full Text] [Related]
14. Investigation of mechanical properties of cryogenically treated music wire.
Heptonstall A; Waller M; Robertson NA
Rev Sci Instrum; 2015 Aug; 86(8):084501. PubMed ID: 26329213
[TBL] [Abstract][Full Text] [Related]
15. Apparatus for dimensional characterization of fused silica fibers for the suspensions of advanced gravitational wave detectors.
Cumming A; Jones R; Barton M; Cagnoli G; Cantley CA; Crooks DR; Hammond GD; Heptonstall A; Hough J; Rowan S; Strain KA
Rev Sci Instrum; 2011 Apr; 82(4):044502. PubMed ID: 21529026
[TBL] [Abstract][Full Text] [Related]
16. Optically trapped mirror for reaching the standard quantum limit.
Matsumoto N; Michimura Y; Aso Y; Tsubono K
Opt Express; 2014 Jun; 22(11):12915-23. PubMed ID: 24921489
[TBL] [Abstract][Full Text] [Related]
17. Modal frequency degeneracy in thermally loaded optical resonators.
Bullington AL; Lantz BT; Fejer MM; Byer RL
Appl Opt; 2008 May; 47(15):2840-51. PubMed ID: 18493291
[TBL] [Abstract][Full Text] [Related]
18. Enhancing the Bandwidth of Gravitational-Wave Detectors with Unstable Optomechanical Filters.
Miao H; Ma Y; Zhao C; Chen Y
Phys Rev Lett; 2015 Nov; 115(21):211104. PubMed ID: 26636839
[TBL] [Abstract][Full Text] [Related]
19. Stable operation of a 300-m laser interferometer with sufficient sensitivity to detect gravitational-wave events within our galaxy.
Ando M; Arai K; Takahashi R; Heinzel G; Kawamura S; Tatsumi D; Kanda N; Tagoshi H; Araya A; Asada H; Aso Y; Barton MA; Fujimoto MK; Fukushima M; Futamase T; Hayama K; Horikoshi G; Ishizuka H; Kamikubota N; Kawabe K; Kawashima N; Kobayashi Y; Kojima Y; Kondo K; Kozai Y; Kuroda K; Matsuda N; Mio N; Miura K; Miyakawa O; Miyama SM; Miyoki S; Moriwaki S; Musha M; Nagano S; Nakagawa K; Nakamura T; Nakao K; Numata K; Ogawa Y; Ohashi M; Ohishi N; Okutomi S; Oohara K; Otsuka S; Saito Y; Sasaki M; Sato S; Sekiya A; Shibata M; Somiya K; Suzuki T; Takamori A; Tanaka T; Taniguchi S; Telada S; Tochikubo K; Tomaru T; Tsubono K; Tsuda N; Uchiyama T; Ueda A; Ueda K; Waseda K; Watanabe Y; Yakura H; Yamamoto K; Yamazaki T;
Phys Rev Lett; 2001 Apr; 86(18):3950-4. PubMed ID: 11328068
[TBL] [Abstract][Full Text] [Related]
20. Gravitational wave detection using laser interferometry beyond the standard quantum limit.
Heurs M
Philos Trans A Math Phys Eng Sci; 2018 May; 376(2120):. PubMed ID: 29661977
[TBL] [Abstract][Full Text] [Related]
[Next] [New Search]