Thermal Noise Interferometer Update and Status

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Presentation transcript:

Thermal Noise Interferometer Update and Status Eric Black LSC Meeting March 18, 2004 Ivan Grudinin, Akira Villar, Kenneth G. Libbrecht G040156-00-R

TNI Goals Direct measurement of broadband thermal noise at lowest reasonable levels If there are any unanticipated noise sources, we want to see them in a test-bed interferometer, not in advanced LIGO. Model validation in extremely low-displacement-noise regime. Do we uncover any unexpected losses (with known noise mechanisms) at very low displacement-noise levels? Measurement of required thermal noise parameters for AdLIGO materials Core Optics: “Braginsky-noise” models need, for Sapphire Thermal-expansion coefficient a Thermal conductivity k Coatings: Structural-damping thermal noise models, for Silica-Tantala and others, need Mechanical loss angle f Loss angle is possibly anisotriopic. Ringdown measurements get value for strains parallel to coating-substrate interface, direct TN measurement gets value for perpendicular strains Coatings: Braginsky-noise models require, for Silica-Tantala and others G040156-00-R

Broadband Thermal Noise Measurements Gonzalez and Saulson Gonzalez and Saulson, J. Accoust. Soc. Am. 96, 207-212 (1994) Verified fluctuation-dissipation theorem in torsional pendulum 40-meter A. Abramovici, et al., Phys. Lett. A 218, 157-163 (1996) Claim made of observation of broadband thermal noise in compound (i.e. glued-together) optics. No analysis given. Yamamoto Yamamoto, et al., Phys. Lett. A 280, 289-296 (2001); Class. Quant. Grav. 19, 1689-1696 (2002) Verification of fluctuation-dissipation theorem, effect of inhomogeneous losses in a leaf-spring Numata Numata, et al., Phys. Rev. Lett. 91 (26), 260602 (2003) Verification of fluctuation-dissipation theorem in mirrors Selection of spot sizes, materials designed to make thermal noise relatively large, easy to measure BK7, Calcium-Fluoride substrates not suitable for AdLIGO Measured coating thermal noise in Silica-Tantala coatings on fused-silica substrates, which are candidate materials for AdLIGO G040156-00-R

Last Sensitivity Curve: 10/23/03 Coating thermal noise observed in Silica-Tantala coatings on fused-silica substrates Loss angle required to fit noise floor: 1.2e-4 Observed noise somewhat lower than predicted from ringdown measurements: Harry et al., Class. Quantum Grav. 19 (5) pp. 897-917 (2002), Penn et al., Class. Quantum Grav. 20 pp. 2917-2915 (2003) Noise level is 3x lower than previous Silica-Tantala coating noise measurement. Numata, et al., PRL 91 (26), 260602 (Dec. 31, 2003) Electronic noise limits sensitivity at lowest levels What are the levels of additional noise sources? G040156-00-R

Improved Sensitivity with Fused Silica Mirrors Photodetector electronic noise reduced by factor of 4 Additional noise sources quantified Shot Noise now dominates at high frequencies Broadband thermal noise measured at 10x better than previous BK7 measurement Noise level remains at ~3x lower level than previous measurement in same materials Silica-Tantala (isotropic) coating loss angle: f=1.2-1.8e-4 G040156-00-R

Measurement Uncertainty and Reproducibility Calibration uncertainty <10% Shot-to-shot variation in phi <5% Change in noise level after removal and reinstallation of mirrors (realignment) = 25% Change in phi = 50% Uncertainty in phi is determined by alignment, not measurement or calibration uncertainties. Does coating thermal noise vary over the face of the optic? Would it matter for the large spot sizes that will be used in AdLIGO? G040156-00-R

Sapphire Fused-silica substrates removed, sapphire installed Noise curve obtained Parameters a = 2.7e-6 K-1 k = 44 W/mK Numerical error in existing theory initially gave unexpected parameters Cerdonio, et al., Phys. Rev. D 63 (8), 082003 (2001) Braginsky model validated in Sapphire Thermoelastic-damping noise measured at 10x lower level than previous Calcium-Fluoride measurement Numata, et al., PRL 91 (26), 260602 (Dec. 31, 2003) Is this the only set of parameters that will fit the data? G040156-00-R

Conclusions The TNI is fulfilling its mission to measure broadband thermal noise at the lowest levels ever observed. The TNI is beginning to contribute to the AdLIGO effort by measuring thermal noise and extracting relevant parameters in candidate materials for optics and coatings. Existing thermoelastic-damping-noise theory (non-adiabatic-limit) must be corrected to yield correct noise floor with accepted Sapphire parameters. G040156-00-R