Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005.

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Presentation transcript:

Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Contents: 1.Introduction of ARSMS 2.Scattering mapping examples 3.Comparisons between scattering and absorption 4.Conclusion 5.Acknowledgement

Stepper-motor controller box CCD camera controller box CCD camera Translation Rotation Mount Laser Sample Stepper-motor PC Experimental Set-up The ARSMS contains two subsystems: Optical imaging subsystem Mechanical motion control subsystem

Technique Parameters Translation: Resolution: 0.05 mm Rotation: Resolution: 0.3 degree (the diameter of sample is 150 mm) Scattering sensitivity: 0.5 ppm/cm (the laser power is 10 mw) Advantages High resolution 3D images Rayleigh scattering intensity Mapping large-size test masses

Measurement and Data Processing Single beam images 2D images 3D image 1 3 2

Single images and 2D images Examples:

Reconstructed 3D image Examples: Sample 2

1.The optical absorption is measured using the photothermal deflection technique at Laboratoire des Matériaux Avancés, Lyon. Typical scattering and absorption [1] maps Comparisons between scattering and absorption

High scattering correlates with higher absorption. Scattering structure is spatially displaced from a similar absorption structure.

Correlations between scattering and absorption Absorption and scattering in sample 1: In detail there is not a clear point to point correlation between scattering and absorption.

Correlations between scattering and absorption Absorption and scattering in sample 2: The spatial displacements indicate that absorption centres and scattering centres are laid down during crystal growth at different distances from the solid liquid interface.

2D and 3D scattering mappings reveal different features—the inhomogeneities and the point defects. Scattering and Absorption seem to be coming from different origins The ARSMS can ensure that an adequate low level of scattering is achieved for gravitational wave detectors and other precision applications. The ARSMS may provide data that can be utilized to improve the quality control of both single crystal and glass optical materials. Conclusions:

Acknowledgement LSC Optics Working Group VIRGO Jean-Marie Mackowski’s Group Australian Research Council ACIGA My Supervisors My fellow students and colleagues