63 research outputs found

    Increased UV transmission by improving the manufacturing process for FS

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    ABSTRACT Optical designers have been designing ultraviolet (UV) systems at wavelengths in the UV region for many years. With increasing demand for deep UV applications, special considerations that are not applicable to traditional visible optics must be taken to produce the optics. Specifically as the wavelength of incident light decreases, the importance of very smooth surfaces increases. The intent of this project is to increase the performance of UV optics in a four-phase project. The first phase consists of characterizing sub-surface damage using destructive methods to enable process control, the second phase (presented here) focuses on polishing methods, the third phase will include cleaning and possible etching protocols and the fourth phase will be improving thin film coating performance. Keywords: Ultraviolet, fused silica, polishing, coating INTRODUCTION As trends in UV optical system design shift to shorter UV wavelengths, optical manufacturing has to be more conscious of the effect that subsurface damage, surface features, residual contamination from polishing and cleaning and coating have on the residual performance of the optics in their systems. For many years, researchers have tackled partial aspects of these problems. For example, Bloembergen 1 stated that cracks and pores on an optical surface will lead to laser damage (LD) when incident with a laser beam. Neauport et al. 2 spoke to two of the main damage initiators of LD, sub-surface damage (SSD) and nano-absorbing centers, focusing mainly on the latter. They used fused silica optics in high power laser applications at 351nm. Higher cerium concentration on the surfaces strongly correlated with increased damage density. Aluminum, copper and iron did not have similar correlations. Neauport et al. also tried to correlate the presence of cerium with damage morphology but the results were inconclusive. Yoshiyama et al. 3 studied the effects of polishing, etching, cleaving and water leaching on the UV damage of fused silica. The surfaces were all exposed to a Nd:YAG laser at 355nm. Micropits were found on the polished surface. Their analysis found high concentrations of Al, B, Ce and Zr. The concentrations of the Al, B and Zr all decreased rapidly to less than 10% of the maximum value at a depth of 50nm, but the Ce required ~100nm before decreasing to less than 10% of its maximum value. A second sample etched with a buffered HF solution had a lower pit density than the polished surface. The pit density decreased exponentially with the etched layer thickness indicating that the cerium is a precursor to laser damage. Micropits found on the cleaved surface indicated that cerium contamination is not the only cause of damage. It is hypothesized that damage initiated because of residual stresses and permanent mechanical damage from the cleaving process. Hydrolyzed cleaved surfaces were found to decrease the laser damage threshold. Camp et al. 4 determined that the zirconia conventionally polished surfaces have a higher laser damage threshold at 355nm compared to ceria polished surfaces. They also observed that damage typically centered around scratches or digs on the surface of the parts. Néauport et al

    Measurement of the bbb\overline{b} dijet cross section in pp collisions at s=7\sqrt{s} = 7 TeV with the ATLAS detector

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    Search for dark matter in association with a Higgs boson decaying to bb-quarks in pppp collisions at s=13\sqrt s=13 TeV with the ATLAS detector

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    Charged-particle distributions at low transverse momentum in s=13\sqrt{s} = 13 TeV pppp interactions measured with the ATLAS detector at the LHC

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    Measurement of the charge asymmetry in top-quark pair production in the lepton-plus-jets final state in pp collision data at s=8TeV\sqrt{s}=8\,\mathrm TeV{} with the ATLAS detector

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    ATLAS Run 1 searches for direct pair production of third-generation squarks at the Large Hadron Collider

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    Search for single production of vector-like quarks decaying into Wb in pp collisions at s=8\sqrt{s} = 8 TeV with the ATLAS detector

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