initial ligo upgrade to 30 w: implication for the input optics ufligo group

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Initial LIGO upgrade to 30 W: Implication for the Input Optics UFLIGO Group. Major IO components and concerns at 30 W. Electro-optic modulators Thermal lensing Degraded noise performance Long term damage? Mode cleaner Thermal lensing due to coating absorption MC_REFL beam  MC WFS - PowerPoint PPT Presentation

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