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LSC August 2005 1 LIGO-G050425-00-Z Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen University of Florida/LIGO Livingston

Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

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Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen University of Florida/LIGO Livingston. RFPD. Wavefront. Sensors. w. 0. flat. flat. mirror, MC1. mirror, MC3. curved mirror, MC2. Mode Cleaner. The Model (I). - PowerPoint PPT Presentation

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Page 1: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 1LIGO-G050425-00-Z

Study of thermal distortions in the Advanced LIGO mode cleaner using Melody

Ken Yoshiki Franzen

University of Florida/LIGO Livingston

Page 2: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 2LIGO-G050425-00-Z

Mode Cleaner

w0

curved mirror, MC2

flat

RFPD

mirror, MC1

flat

mirror, MC3

Wavefront Sensors

Page 3: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 3LIGO-G050425-00-Z

The Model (I)

MCellipticalcurvmm_release_2 – July 29, 2004

by Amber Lynn Bullington (Stanford University) and Ray Beausoleil (HP Laboratories)

http://www.stanford.edu/~abull/

Page 4: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 4LIGO-G050425-00-Z

The Model (II)

Melody includes: Thermal focusing Surface deformation

in coatings and substrates

New features: Elliptical beam represented Curvature mismatch operators for beam splitters

Page 5: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 5LIGO-G050425-00-Z

My job

Crash test dummy

UF group needs realistic model for design

Upper limits of coating and substrate absorption coefficients

Run the code, see what comes out…

Still some issues with Melody’s pseudo-locker and more, under discussion…

Page 6: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 6LIGO-G050425-00-Z

Parameters

Geometries as in the AdvLIGO IOO design document

Fused silica

Modulation index 0.47 (resonant), 0.10 (mode locking)

Page 7: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 7LIGO-G050425-00-Z

Output (I)

Page 8: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 8LIGO-G050425-00-Z

Output (II)

Page 9: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 9LIGO-G050425-00-Z

Reflected beam (I)

Page 10: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 10LIGO-G050425-00-Z

Reflected beam (II)

Page 11: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 11LIGO-G050425-00-Z

Reflected beam (III)

3 W into mode cleaner, coating abs. 0.6 ppm

Page 12: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 12LIGO-G050425-00-Z

Reflected beam (IV)

10 W into mode cleaner, coating abs. 0.6 ppm

Page 13: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 13LIGO-G050425-00-Z

30 W into mode cleaner, coating abs. 0.6 ppmProblem with angular control (WFS)?

Reflected beam (V)

Page 14: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 14LIGO-G050425-00-Z

150 W into mode cleaner, coating abs. 0.6 ppm

Reflected beam (VI)

Page 15: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 15LIGO-G050425-00-Z

Alternate MC geometry

Inject beam into MC2» Lower AOI

Requires some re-routing of beams in HAMs» IOT table moves to HAM2

w0

mirror, MC1

flat

mirror, MC3

flat

RFPDWavefront Sensors

Page 16: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 16LIGO-G050425-00-Z

150 W into mode cleaner, coating abs. 0.6 ppmInjected trough the curved mirror

Reflected beam (VII)

Page 17: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 17LIGO-G050425-00-Z

Reflected beam summary

Asymmetry in reflected beam at high power caused by passing through region off-center of non-spherical thermal lens…

Is this a problem?

Could be avoided by injecting beam through curved mirror instead of one of the flats

Please verify by other code

Should start to see effects above 10 W. That is soon!

Page 18: Study of thermal distortions in the Advanced LIGO mode cleaner using Melody Ken Yoshiki Franzen

LSC August 2005 18LIGO-G050425-00-Z

Conclusion

Substrate absorption not so critical

Even at 0.6 ppm coating absorption the higher order mode contamination will be more than 1%. OK?

Reflected beam will be terrible. OK? Consider alternative injection scheme.

Melody issues need to be resolved (pseudo-locker and more). Need volunteers.