Thermal-noise-limited underground interferometer CLIO

被引：14

作者：

Agatsuma, Kazuhiro ^{[1
]}

Arai, Koji ^{[2
]}

Fujimoto, Masa-Katsu ^{[2
]}

Kawamura, Seiji ^{[2
]}

Kuroda, Kazuaki ^{[1
]}

Miyakawa, Osamu ^{[1
]}

Miyoki, Shinji ^{[1
]}

Ohashi, Masatake ^{[1
]}

Suzuki, Toshikazu ^{[3
]}

Takahashi, Ryutaro ^{[2
]}

Tatsumi, Daisuke ^{[2
]}

Telada, Souichi ^{[4
]}

Uchiyama, Takashi ^{[1
]}

Yamamoto, Kazuhiro ^{[5
,6
]}

机构：

[1] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan

[2] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[3] High Energy Accelerator Org, Tsukuba, Ibaraki 3050801, Japan

[4] Natl Inst Adv Ind Sci & Technol, Tsukuba, Ibaraki 3058563, Japan

[5] Leibniz Univ Hannover, Inst Gravitat Phys, D-30167 Hannover, Germany

[6] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

来源：

CLASSICAL AND QUANTUM GRAVITY | 2010年 / 27卷 / 08期

关键词：

FREQUENCY STABILIZATION; LASER; VIBRATION;

D O I：

10.1088/0264-9381/27/8/084022

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report on the current status of CLIO (Cryogenic Laser Interferometer Observatory), which is a prototype interferometer for LCGT (large scale cryogenic gravitational-wave telescope). LCGT is a Japanese next-generation interferometric gravitational-wave detector featuring the use of cryogenic mirrors and a quiet underground site. The main purpose of CLIO is to demonstrate a reduction of the mirror thermal noise by cooling the sapphire mirrors. CLIO is located in an underground site of the Kamioka mine, 1000 m deep from the mountain top, to verify its advantages. After a few years of commissioning work, we have achieved a thermal-noise-limited sensitivity at room temperature. One of the main results of noise hunting was the elimination of thermal noise caused by a conductive coil holder coupled with a pendulum through magnets.

引用

页数：10

共 50 条

[1] Thermal-noise-limited optical cavity
Webster, S. A.
Pugla, S.
Millo, J.
Oxborrow, M.
Gill, P.
2008 CONFERENCE ON PRECISION ELECTROMAGNETIC MEASUREMENTS DIGEST, 2008, : 58 - +
[2] Thermal-noise-limited optical cavity
Webster, S. A.
Oxborrow, M.
Pugla, S.
Millo, J.
Gill, P.
PHYSICAL REVIEW A, 2008, 77 (03):
[3] THERMAL-NOISE-LIMITED OPERATION OF DYNAMICAL GRAVITATIONAL DETECTORS
FORWARD, RL
BERMAN, D
MILLER, LR
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1968, 13 (03): : 513 - &
[4] Underground Cryogenic Laser Interferometer CLIO
Miyoki, Shinji
TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP2009), 2010, 203
[5] Thermal-noise-limited higher-order mode locking of a reference cavity
Zeng, X. Y.
Ye, Y. X.
Shi, X. H.
Wang, Z. Y.
Deng, K.
Zhang, J.
Lu, Z. H.
OPTICS LETTERS, 2018, 43 (08) : 1690 - 1693
[6] Compact, thermal-noise-limited reference cavity for ultra-low-noise microwave generation
Davila-Rodriguez, J.
Baynes, F. N.
Ludlow, A. D.
Fortier, T. M.
Leopardi, H.
Diddams, S. A.
Quinlan, F.
OPTICS LETTERS, 2017, 42 (07) : 1277 - 1280
[7] Thermal-noise-limited ultra-stable laser operated at 698 nm
Zhang, Lin-Bo
Chen, Long
Dong, Rui-Fang
Liu, Tao
Zhang, Shou-Gang
PHYSICA SCRIPTA, 2024, 99 (07)
[8] THERMAL-NOISE-LIMITED TRANSDUCTION OBSERVED IN MECHANOSENSORY RECEPTORS OF THE INNER-EAR
DENK, W
WEBB, WW
PHYSICAL REVIEW LETTERS, 1989, 63 (02) : 207 - 210
[9] Compact, portable, thermal-noise-limited optical cavity with low acceleration sensitivity
Kelleher, Megan L.
Mclemore, Charles A.
Lee, Dahyeon
Davila-Rodriguez, Josue
Diddams, Scott A.
Quinlan, Franklyn
OPTICS EXPRESS, 2023, 31 (07) : 11954 - 11965
[10] Thermal-noise-limited crystalline whispering-gallery-mode resonator for laser stabilization
Alnis, J.
Schliesser, A.
Wang, C. Y.
Hofer, J.
Kippenberg, T. J.
Haensch, T. W.
PHYSICAL REVIEW A, 2011, 84 (01):

← 1 2 3 4 5 →