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Overview of coating research Stuart Reid On behalf of the coating subgroup LSC/VIRGO meeting, September 2008, Amsterdam G080468-00-R
Program Overview ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Coating sensitivity impact ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],Narrowband Advanced LIGO sensitivity Wideband Advanced LIGO sensitivity (assuming Advanced LIGO baseline values)
Advanced LIGO developments ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Brownian noise ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],Mirror suspension, with HR coating on front face
[object Object],[object Object],[object Object],[object Object],[object Object],Glasgow (I. Martin et al) low T dissipation in single-layers Ta 2 O 5  and SiO 2
Glasgow (I. Martin et al)  Heat treatment of un-doped tantala films ,[object Object],[object Object],Above: Electron diffraction measurement of Ta 2 O 5  heat treated at (i)  600  ° C,  showing amorphous structure and (ii)  800   ° C, showing crystalline structure. Left: Loss at 1.9 kHz of 0.5 mm Ta 2 O 5  coatings heat treated at  (a) 600 ,   (b) 300  and  (c) 800   ° C  (i) (ii) (c) (a) (b) Temperature (K) Loss of coated cantilever 0 50 100 300 150 200 250 1E-5 1E-4
Glasgow (E. Chalkley et al) Other ongoing coating R&D ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],HfO 2
Hobart and William Smith Colleges (S. Penn et al)   Mechanical loss is silica thin-films ,[object Object],[object Object],[object Object],[object Object],[object Object]
Caltech TNI update (G. Olgin, E. Black et al) ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Caltech Photothermal experiment (G. Olgin et al) ,[object Object],Expansion Reflection Phase ,[object Object]
Sannio University (I. Pinto et al) Optimised coatings ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],(Sannio Coating Team: Giuseppe Castaldi, Vincenzo Galdi, Vincenzo Pierro, Innocenzo M. Pinto, Maria Principe)
Thermo-optic noise - update ,[object Object],[object Object],[object Object],»  thermoelastic noise »  thermorefractive noise ,[object Object], T  T Thermorefractive contribution somewhat higher than thermoelastic contribution but same order of magnitude.
Embry-Riddle - Thermo-optic noise (A. Gretarsson, G. Ogin et al) ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
MIT - Cancellation of thermo-optic noises? (M. Evans et al) ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
MIT - Cancellation of thermo-optic noises? (M. Evans et al)  contd ,[object Object],[object Object]
Stanford - Effect of First Contact & UV (A. Markosyan, K. Sun et al) Effect of First Contact application to UV exposure was studied on a 1” LIGO mirror with baseline absorption value    0.3 ppm.   Measurements were carried out along the red line (2 mm above center) at ambient atmosphere. Areas 1 and 2 were subjected to the following procedures  i)                  Absorption measurement ii)               Area 2 was covered by FC, left for 48 hours iii)             Areas 1 and 2 were UV illuminated for 24 hours iv)             FC was peeled off v)                 Absorption measurement vi)             Annealed for 2 hour at c.a. 350  C vii)             Absorption measurement UV source:    = 255nm with several nm FWHM,       3.5 mm. Power density is  ~ 6   W / cm 2 , so 24 hours gives total irradiation flux of  ~ 0.5 J /cm 2 1 2 Central line (x-direction)
Fig. 1. A reference scan over the sample surface (blue):  Alpha = 0.32 ppm The black line shows the same data with spikes removed (for the sake of clarity) Stanford - Effect of First Contact & UV  contd (A. Markosyan, K. Sun et al)
Fig. 2. Comparison between three different scans (all spikes are  removed in order to simplify the presentation): before UV exposure (black line), after UV exposure (blue), after heat treatment (red). Area 2 shows smaller increase presumably because of protection by FC. The excess absorption caused by UV exposure is totally  reversible  by  annealing  2 hrs@350  C 1 2 UV beam position Stanford - Effect of First Contact & UV  contd (A. Markosyan, K. Sun et al)
Stanford - absorption of TNI optic (optimised coating)  (A. Markosyan, K. Sun et al) ,[object Object],[object Object],[object Object],[object Object],[object Object]
Syracuse - Scatter studies after different cleaning techniques (J. Smith et al) ,[object Object],[object Object],[object Object],[object Object],[object Object],Drag wiped Std First Contact Carbon Nano Tube First Contact As part of the overall coating plan, we also intend to study  scatter  vs  annealing .
Caltech - Scatter  contd (Liyuan Zhang) ,[object Object]
Other developments ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Summary ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]

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G080468 00

  • 1. Overview of coating research Stuart Reid On behalf of the coating subgroup LSC/VIRGO meeting, September 2008, Amsterdam G080468-00-R
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  • 17. Stanford - Effect of First Contact & UV (A. Markosyan, K. Sun et al) Effect of First Contact application to UV exposure was studied on a 1” LIGO mirror with baseline absorption value  0.3 ppm.   Measurements were carried out along the red line (2 mm above center) at ambient atmosphere. Areas 1 and 2 were subjected to the following procedures i)                 Absorption measurement ii)               Area 2 was covered by FC, left for 48 hours iii)             Areas 1 and 2 were UV illuminated for 24 hours iv)             FC was peeled off v)                Absorption measurement vi)             Annealed for 2 hour at c.a. 350  C vii)            Absorption measurement UV source:  = 255nm with several nm FWHM,   3.5 mm. Power density is ~ 6  W / cm 2 , so 24 hours gives total irradiation flux of ~ 0.5 J /cm 2 1 2 Central line (x-direction)
  • 18. Fig. 1. A reference scan over the sample surface (blue): Alpha = 0.32 ppm The black line shows the same data with spikes removed (for the sake of clarity) Stanford - Effect of First Contact & UV contd (A. Markosyan, K. Sun et al)
  • 19. Fig. 2. Comparison between three different scans (all spikes are removed in order to simplify the presentation): before UV exposure (black line), after UV exposure (blue), after heat treatment (red). Area 2 shows smaller increase presumably because of protection by FC. The excess absorption caused by UV exposure is totally reversible by annealing 2 hrs@350  C 1 2 UV beam position Stanford - Effect of First Contact & UV contd (A. Markosyan, K. Sun et al)
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