Thermal noise caused by an inhomogeneous loss in the mirrors used in the gravitational wave detector

Physics Letters, Section A: General, Atomic and Solid State Physics

Volumn 305, Issue 1-2, 2002, Pages 18-25

  Yamamoto, Kazuhiro ^a   Ando, Masaki ^a   Kawabe, Keita ^a,b   Tsubono, Kimio ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b ALBERT EINSTEIN INSTITUT   (Germany)

Author keywords

Direct approach; Inhomogeneous loss; Interferometric gravitational wave detector; Modal expansion; Thermal noise of mirror

Indexed keywords

ELECTRIC CURRENT CONTROL; GRAVITATIONAL EFFECTS; INTERFEROMETRY; LASER BEAMS; MIRRORS; MODAL ANALYSIS; SIGNAL DETECTION; THERMAL NOISE;

BEAM SPOT; DIRECT APPROACH; ESTIMATION METHODS; GRAVITATIONAL WAVE DETECTORS; MODAL EXPANSION; TYPICAL MODEL;

GRAVITY WAVES;

ARTICLE; CALCULATION; GRAVITY; ILLUMINATION; LASER; NOISE; RELIABILITY; SURFACE PROPERTY;

EID: 0037175599     PISSN: 03759601     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0375-9601(02)01389-0     Document Type: Article

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