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

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Page 1: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Rayleigh Scattering Mapping System

School of Physics, University of Western Australia

Australia – Italy Workshop on GW Detection 2005

Page 2: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Contents:

1.Introduction of ARSMS2.Scattering mapping examples3.Comparisons between scattering and absorption4.Conclusion5.Acknowledgement

Page 3: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

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

Page 4: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

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

Page 5: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Measurement and Data Processing

Single beam images

2D images

3D image

13

2

Page 6: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Single images and 2D images

Examples:

Page 7: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Reconstructed 3D image

Examples:

Sample 2

Page 8: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

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

Page 9: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Comparisons between scattering and absorption

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

Page 10: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

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.

Page 11: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

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.

Page 12: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

•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:

Page 13: Rayleigh Scattering Mapping System School of Physics, University of Western Australia Australia – Italy Workshop on GW Detection 2005

Acknowledgement

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