Optics Express_2014_High-visibility nonclassical interference of photon pairs generated in a

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三阶鬼成像的可见度研究

三阶鬼成像的可见度研究

三阶鬼成像的可见度研究于佳意;常锋;姚治海;徐聪;董博;王晓茜【摘要】Ghost imaging,also called correlation imaging,has attracted much attention in recent years. It has in estima-ble development prospects in many fields. This article put forward a new experiment scheme of third-order ghost imag-ing according to a research of third-order ghost imaging. We got the visibility range of both the original and new scheme by calculating the third-order correlation functions. Then,we compared these two kinds of schemes,and anal-ysed the similarities and differences between them. The result showed that,the new imaging scheme could improve the image quality and visibility. This conclusion was verified by numerical simulation.%鬼成像又称为关联成像,近年来受到广泛的关注,在很多领域上都具有广阔的发展前景。

通过对热光三阶鬼成像进行研究,提出一种新的三阶鬼成像实验方案。

通过计算三阶关联函数,导出三阶关联函数原始方案与新方案的可见度取值范围,将两种方案进行比较,分析它们的异同。

安迪顿克鲁斯-豪斯LED危险区域灯具说明书

安迪顿克鲁斯-豪斯LED危险区域灯具说明书

Hazardous Area LED LightingLED lighting for hazardous areas3,000 to 13,000 lumensChamp VMVL LED Safe. Reliable. Efficient.Featuring a broad range of LED luminaires for harsh, hazardous and industrial environments, Eaton Crouse-Hinds series lighting solutions are designed to perform reliably in the most extreme conditions while helping reduce energy, maintenance and manpower costs.Why LED?Why Crouse-Hinds?Useful lifeRated life is up to 60,000 hours of maintenance-free and safe operationEnergy efficiencyLED average energy consumption is significantly less than traditional fluorescent and HID fixtures Start/restart timeInstant illumination versus 10 minute restrike time for HID Light qualityHigher color rendering compared to fluorescent and HIDEnvironmental benefits Mercury-free LED eliminates disposal costs and lower energy consumption for a smaller carbon footprint Rugged designBuilt to withstand extreme temperatures, vibration, water and dustHigh efficacyUp to 127 lumens per watt (model dependent) Thermal management Effective heat sinking ensures longer lifeQuality of lightCustom optics designed to maximize light distribution and intensityVersatile mountingLED fixtures are compatible with Crouse-Hinds series HID installed base2EATON'S CROUSE-HINDS SERIESVMVL -7 vs. 175 watt HIDAssumptions: Calculations based on overall life of the LED system. Energy cost of $.09 per kilowatt; 24 hour per day operation; labor rate of $75 each for 2 workers; average time for fixture maintenance of 1 hour.TOTAL COST OF OWNERSHIP75%ENERGY EFFICIENCY77%MAINTENANCE REDUCTION100%Why choose Champ VMVL?Safe, reliable and efficient. VMVL LED luminaires are engineered to deliver high lumen output and maintenance-free long life in the toughest conditions.Simple installation and replacement:• Contractor-friendly design is ideal for both retrofit and new construction•Easy to retrofit using existing HID Champ mounting module •Available with lever lockconnectors and standard three-pole terminal blockBuilt to last:• Type 4X and IP66 rated•Impact-resistant lens sealed from the outside environment provides ingress protection against water and dust•Die cast aluminum LED housing provides efficient thermal path to heat sink assembly•Vertical fin design facilitates air flow and dust sheddingCustom optics:• Type I, III and V optics designed tomaximize light distribution and intensity** Type V optics standard.Increased efficiency:• Up to 127 lumens per watt (7L model)For more information go to:Design featuresShown with optional diffused lensShown with optional uplight refractor lens and guardMultiple lens options:• Clear glass lens standard•Uplight refractor lens provides ~5% uplight and ~16% sidelight for better visibility •Optional lenses include diffused glass, clear polycarbonate or uplight refractor3EATON'S CROUSE-HINDS SERIESTYPE ILong and rectangular for hallways, walkways, loading docks, catwalks.Ideal for:• Mining conveyor belts • Aisleways and hallways • Catwalks and walkways • Ramps and loading docks • Tunnels with overhead mountsTYPE IIIStanchion and wall mount light distribution, minimizing spillover on the wall.Ideal for:• Narrow crosswalks orpassages with wall mounted fixtures • Tunnels with wall mount • Wall or stanchion mountrequiring 180° forward throw beam patternsTYPE VRegular circular distribution pattern for high/low bay indoor and outdoor ceiling or pendant mount lighting.Ideal for:• Pendant, ceiling or stanchion mount overhead building mounts • Processing mills, industrial plants, large buildings, warehouses, etc.Type III optics minimize light spillover onto the walls and direct light to the ground.Custom opticsThree optical options to maximize light distribution and intensity4EATON'S CROUSE-HINDS SERIESLuminaire Calc. type Units Avg.Max.Min.Avg./min.Max./min.Champ VMVL Illuminance Fc 26.9136.917.4 1.55 2.12175W MHIlluminanceFc14.3218.07.91.812.28Champ VMVL w/ T ype I opticsChamp VMVL has broader coverage area, higher delivered footcandles and uniformity for a typical catwalk or conveyor application.Case study: T ype I opticsCatwalk/conveyor lightingUtilizing Eaton’s Crouse-Hinds lighting layout services, Champ VMVL luminaires with Type I optics and HID luminaires are shown installed on a catwalk to compare photometrics.ComparisonChamp T ype I LEDs have a wider linear pattern than equivalent HID luminaires and provide more efficient light dispersion, which fully illuminates the catwalk.ResultsChamp VMVL LED with T ype I optics provides superiorillumination along the conveyor and walkway safely. With no gaps in illumination, the optical pattern allows for increased spacing of fixtures and a safer conveyor system.Savings realized•Champ T ype I pattern allows for greater fixture spacing along the catwalk or conveyor system•Increased visibility with no dark spots results in safer conditions for workers •Up to 77% energy savings over the life of the fixture5EATON'S CROUSE-HINDS SERIESLED system:• High intensity discrete power emitters•Standard: cool white (5000K, 70 CRI); optional: warm white, (3000K, 80 CRI) or neutral white (4000K, 70 CRI)•Custom Type I, III and V optics available Colored LED options:• Available in green or amber*•Reduction in light polution for night space observation and sky glow due to isolating blue wavelength in red and amber colors • Wildlife-friendly•Improves visibility for telescopes in observatories during night sky space exploration*Custom optics not available with colored LEDs.•Easy installation - compact modular fixture attaches onto existing Champ mounting module•Energy-efficient technology - up to 77% energy savings over HID fixtures• Contains no mercury or other hazardous substances•Shock- and vibration-resistant solid-state luminaires have nofilaments or glass components that could break - greatly reduces the risk of premature failure • Operating ambient: -40°C to 65°C• Up to 60,000 hours lifetime at 55°C •5 year fixture warranty††Refer to page 2 of the authorized distributor price book for Crouse-Hinds standard Terms and Conditions.6EATON'S CROUSE-HINDS SERIESAdvanced scheduling control allows for improving energy efficiency during non-operational hours. Easy software control lets a user set up schedules for lights to be on and off at pre-defined times,removing the challenges of manual management.Daylight harvesting allows for use of the daylight and adjusts the light level of luminaire to maintain the desired light levels. It is best suited for outdoor environments or indoor areas where daylight is present during operational hours of a facility.Fixture grouping is an added benefit thatmaximizes control in a defined area. By grouping light fixtures, same control settings can be applied to them to increase efficiency and response time.Occupancy sensing is best used in areas that see infrequent traffic, such as storage areas ofwarehouses. Innovative occupancy sensor controls can automatically illuminate the area once presence is sensed in an area and also turn it back off when sensors stop sensing the presence.Advanced dimming controls help reduce the energy consumptions by setting dimming levels. Dimming controls could be used in conjunction with other control features, such as scheduling and occupancy sensing, to improve energy savings.Connected lighting highlights:/LEDconnectedFor more information go to:Connected lightingRemote monitoring and control for use in hazardous and hard-to-access areas.Standard materials:• Lamp housing and adapter - die cast aluminum with Corro-free™ epoxy powder coat• Lens - heat- and impact-resistant glass • Gaskets - silicone• External hardware - stainless steel •Factory-sealed, no external seals required7EATON'S CROUSE-HINDS SERIESCertifications and compliances:NEC, CEC & IEC• Class I, Division 2, Groups A, B, C, D• Class II, Groups E, F , G • Class III• Class I, Zone 2 AEx ec mb IICT*GC • Zone 21 tb IIIC • Simultaneous Presence •Wet Locations, Type 4X, IP66UL standards• UL 844 Hazardous (Classified)•UL1598 Luminaires, UL1598A MarineCSA standard• CSA C22.2 No. 137IEC/ATEX standards*• IEC 60079-0:2011, 6th Edition / EN 60079-0:2012• IEC 60079-7:2010, 5.1 Edition / EN 60079-7:2015• IEC 60079-31:2008, 2nd Edition / EN 60079-31:2014• IEC 60529:2001 / EN 60529:2001• IEC 60598-1:2008 / EN 60598-1:2008• IEC 60598-2:2008 / EN 60598-2:2008•IEC 60079-18:2017, 4.1 Edition / EN 60079-18:2015 + A1:2017Luminaire markings • IECEx UL 13.0052X• DEMKO 13 ATEX 1305741X • DEMKO 13 ATEX 1475031X100-277 VAC/127-250 VDC (UNV1 luminaire only)• II 3 G EX ec mb IIC T5 Gc -40°C to +40°C• II 3 G EX ec mb IIC T5 Gc -40°C to +55°C • II 3 G EX ec mb IIC T4 Gc -40°C to +65°C • II 2 D Ex tb IIIC T72°C Db -40°C to +40°C • II 2 D Ex tb IIIC T87°C Db -40°C to +55°C •II 2 D Ex tb IIIC T92°C Db -40°C to +65°CUplight refractor lens now available*IEC/ATEX certifications applicable for voltage ranges: 100-277VAC, 127-250 VDC.Maximize light dispersion+90°-90°0°~5% uplight~5%uplight ~16% sidelight~16% sidelight/ChampLEDFor more information go to:Weights:VMVL -9 to VMVL -13The new uplight refractor lens is perfect for low bay ceilings,suspended pendant mounts, areas with elevated infrastructure or areas which require dispersed side and uplight illumination.range, VDC127-250VT emperature codes, UNV1 driver:Temperature codes, UNV34 driver:Input power Input amps at 100-277 VMVL-13-S892Input power Input amps at 347-480 VMVL-13-S892Electrical ratings:*IEC voltage: 100-240 VAC @ 50/60 Hz. **For VMVL -3: PF>0.9 from 100-255 VAC.EMC / CE compliance:If the dimming interface of the LED driver is connected to an external dimmer which is not provided with the luminaire, a ferrite core must be used on the input and dimming lines. Approved ferrite cores are: Fair-Rite P/N 0431167281.* T -Code is T4A for VMVL -11-S892 with R1, R3 Optics* T -Code is T4A for VMVL -11 with R1, R3 Optics8EATON'S CROUSE-HINDS SERIESOrdering informationAccessories (ordered separately)VMVL -AL -GL -UNV1-DRIVER-KITD2S208 277208-277V*Available with ceiling mounted modules only.Part number example: VMVL -3-N-2A-R1-G-UNV1-S831-S891Champ VMVL, 3,000 lumens, 4000K neutral white, ¾" pendant mount, Type I optics, wire guard, 100-277 VAC driver, safety cable, diffused glass lens9EATON'S CROUSE-HINDS SERIESOptics optionsR1, R3 and BLANKType I, III and V optics with all mounts minus ceilingR1A and R3A1Type I and Type III ceiling mount onlyR1B and R3B1Type I and Type III ceiling mount onlyR3APType III wall mountR3A2Type III ceiling mount onlyR3B2Type III ceiling mount only10EATON'S CROUSE-HINDS SERIESCalculation summaryLabel Calc. type Avg.Max.Min.VMV LED grid Illuminance 0.628.00.00.250.50 1.0 5.02.5T ype I optical patternCalculation summaryLabel Calc. type Avg.Max.Min.VMV LED grid Illuminance 0.617.50.0T ype III optical patternHigher average footcandles, uniformity and distribution coverage with less than half the lumens and energy consumption compared to 175W metal halide Actual lumens †Tolerance +/- 10%.Photometric comparison at 15 ft. mounting height0.250.50 1.0 5.02.511EATON'S CROUSE-HINDS SERIESDimensionsCeiling DimensionsPendant APM2 APM3 HPM2ConeBPM2BPM3CeilingCM2CM3VMVL-*WallTWM2TWM3StanchionJ M5 PM5WallCone pendantT runnionMounting module series13EATON'S CROUSE-HINDS SERIESNotesFollow us on social media to get the latest product and support information.Eaton is a registered trademark. All other trademarks are property of their respective owners.Eaton 1000 Eaton Boulevard Cleveland, OH 44122United States © 2023 Eaton All Rights Reserved Printed in USA Publication No. 5488-0623September 2023Australia 61-2-8787-2777 FAX: 61-2-9609-2342CEASales@ IEC Electrical (CEAG products)49 (0) 6271 806-500 FAX: 49 (0) 6271 806-476*****************Haz Area Communications (MEDC, Hernis, Oxalis, FHF Sonix)44 (0) 1623 444400 FAX: 44 (0) 1623 444531*******************Process instrumentation (MTL products)44 (0) 1582 723633 FAX: 44 (0) 1582 422283********************Airport Lighting866-764-5454 ***************************China 86-21-2899-3600 FAX: 86-21-2899-4055cchsales@ Eaton Middle East 9714-8066100 FAX: 9714-8894813CHBL *************Mexico/Latin America/Caribbean 52-555-804-4000 FAX: 52-555-804-4020*************************Canada Toll Free: 800-265-0502 FAX: (800) 263-9504 FAX Orders only: (866) 653-0645U.S. (global headquarters): Eaton’s Crouse-Hinds business 1201 Wolf Street Syracuse, NY 13208(866) 764-5454 FAX: (315) 477-5179 FAX Orders Only: (866) 653-0640***************************Eaton’s B-Line business 509 West Monroe Street Highland, IL 62249800-851-7415 FAX: 618-654-1917 /b-lineseries。

ieee trans vehicular technology latex 模板 -回复

ieee trans vehicular technology latex 模板 -回复

ieee trans vehicular technology latex 模板-回复如何使用IEEE Transactions on Vehicular Technology LaTeX模板?第一步:下载并安装TeX发行版在使用IEEE Transactions on Vehicular Technology LaTeX模板之前,首先需要下载并安装一个TeX发行版,例如TeX Live或者MiKTeX。

这些发行版提供了TeX系统和相关的工具,使得我们能够编译和生成LaTeX文档。

第二步:获取IEEE Transactions on Vehicular Technology LaTeX模板在确认TeX发行版安装成功后,我们需要获取IEEE Transactions on Vehicular Technology LaTeX模板。

可以通过以下几种方式来获得该模板:1. 访问IEEE官方网站:IEEE提供了LaTeX模板的下载链接,我们可以通过访问IEEE Transactions on Vehicular Technology主页或者Google搜索来获取模板文件的下载链接。

2. 使用模板管理工具:有一些LaTeX发行版提供了模板管理工具,如TeX Live中的TeX Live Manager工具,我们可以使用这些工具来搜索并安装IEEE Transactions on Vehicular Technology LaTeX模板。

第三步:编写LaTeX文档一旦我们获取了IEEE Transactions on Vehicular Technology LaTeX模板,我们可以开始编写我们的文档了。

首先,我们需要创建一个新的LaTeX 源文件,以".tex"为扩展名。

我们可以使用任何文本编辑器来创建和编辑这个源文件。

在源文件中,我们需要使用指定的文档类来设置我们的文档格式,如下所示:\documentclass[journal]{IEEEtran}然后,我们需要加载所需的包和宏,如下所示:\usepackage{graphicx}\usepackage{amsmath}接下来,我们可以开始编写文档内容了。

机器学习设计知识测试 选择题 53题

机器学习设计知识测试 选择题 53题

1. 在机器学习中,监督学习的主要目标是:A) 从无标签数据中学习B) 从有标签数据中学习C) 优化模型的复杂度D) 减少计算资源的使用2. 下列哪种算法属于无监督学习?A) 线性回归B) 决策树C) 聚类分析D) 支持向量机3. 在机器学习模型评估中,交叉验证的主要目的是:A) 增加模型复杂度B) 减少数据集大小C) 评估模型的泛化能力D) 提高训练速度4. 下列哪项不是特征选择的方法?A) 主成分分析(PCA)B) 递归特征消除(RFE)C) 网格搜索(Grid Search)D) 方差阈值(Variance Threshold)5. 在深度学习中,卷积神经网络(CNN)主要用于:A) 文本分析B) 图像识别C) 声音处理D) 推荐系统6. 下列哪种激活函数在神经网络中最为常用?A) 线性激活函数B) 阶跃激活函数C) ReLUD) 双曲正切函数7. 在机器学习中,过拟合通常是由于以下哪种情况引起的?A) 模型过于简单B) 数据量过大C) 模型过于复杂D) 数据预处理不当8. 下列哪项技术用于处理类别不平衡问题?A) 数据增强B) 重采样C) 特征选择D) 模型集成9. 在自然语言处理(NLP)中,词嵌入的主要目的是:A) 提高计算效率B) 减少词汇量C) 捕捉词之间的语义关系D) 增加文本长度10. 下列哪种算法不属于集成学习方法?A) 随机森林B) AdaBoostC) 梯度提升机(GBM)D) 逻辑回归11. 在机器学习中,ROC曲线用于评估:A) 模型的准确性B) 模型的复杂度C) 模型的泛化能力D) 分类模型的性能12. 下列哪项不是数据预处理的步骤?A) 缺失值处理B) 特征缩放C) 模型训练D) 数据标准化13. 在机器学习中,L1正则化主要用于:A) 减少模型复杂度B) 增加特征数量C) 特征选择D) 提高模型精度14. 下列哪种方法可以用于处理时间序列数据?A) 主成分分析(PCA)B) 线性回归C) ARIMA模型D) 决策树15. 在机器学习中,Bagging和Boosting的主要区别在于:A) 数据处理方式B) 模型复杂度C) 样本使用方式D) 特征选择方法16. 下列哪种算法适用于推荐系统?A) K-均值聚类B) 协同过滤C) 逻辑回归D) 随机森林17. 在机器学习中,A/B测试主要用于:A) 模型选择B) 特征工程C) 模型评估D) 用户体验优化18. 下列哪种方法可以用于处理缺失数据?A) 删除含有缺失值的样本B) 使用均值填充C) 使用中位数填充D) 以上都是19. 在机器学习中,偏差-方差权衡主要关注:A) 模型的复杂度B) 数据集的大小C) 模型的泛化能力D) 特征的数量20. 下列哪种算法属于强化学习?A) Q-学习B) 线性回归C) 决策树D) 支持向量机21. 在机器学习中,特征工程的主要目的是:A) 减少数据量B) 增加模型复杂度C) 提高模型性能D) 简化数据处理22. 下列哪种方法可以用于处理多分类问题?A) 一对多(One-vs-All)B) 一对一(One-vs-One)C) 层次聚类D) 以上都是23. 在机器学习中,交叉熵损失函数主要用于:A) 回归问题B) 分类问题C) 聚类问题D) 强化学习24. 下列哪种算法不属于深度学习?A) 卷积神经网络(CNN)B) 循环神经网络(RNN)C) 随机森林D) 长短期记忆网络(LSTM)25. 在机器学习中,梯度下降算法的主要目的是:A) 减少特征数量B) 优化模型参数C) 增加数据量D) 提高计算速度26. 下列哪种方法可以用于处理文本数据?A) 词袋模型(Bag of Words)B) TF-IDFC) 词嵌入D) 以上都是27. 在机器学习中,正则化的主要目的是:A) 减少特征数量B) 防止过拟合C) 增加数据量D) 提高计算速度28. 下列哪种算法适用于异常检测?A) 线性回归B) 决策树C) 支持向量机D) 孤立森林(Isolation Forest)29. 在机器学习中,集成学习的主要目的是:A) 提高单个模型的性能B) 结合多个模型的优势C) 减少数据量D) 增加模型复杂度30. 下列哪种方法可以用于处理高维数据?A) 主成分分析(PCA)B) 特征选择C) 特征提取D) 以上都是31. 在机器学习中,K-均值聚类的主要目的是:A) 分类B) 回归C) 聚类D) 预测32. 下列哪种算法适用于时间序列预测?A) 线性回归B) ARIMA模型C) 决策树D) 支持向量机33. 在机器学习中,网格搜索(Grid Search)主要用于:A) 特征选择B) 模型选择C) 数据预处理D) 模型评估34. 下列哪种方法可以用于处理类别特征?A) 独热编码(One-Hot Encoding)B) 标签编码(Label Encoding)C) 特征哈希(Feature Hashing)D) 以上都是35. 在机器学习中,AUC-ROC曲线的主要用途是:A) 评估分类模型的性能B) 评估回归模型的性能C) 评估聚类模型的性能D) 评估强化学习模型的性能36. 下列哪种算法不属于监督学习?A) 线性回归B) 决策树C) 聚类分析D) 支持向量机37. 在机器学习中,特征缩放的主要目的是:A) 减少特征数量B) 提高模型性能C) 增加数据量D) 简化数据处理38. 下列哪种方法可以用于处理文本分类问题?A) 词袋模型(Bag of Words)B) TF-IDFC) 词嵌入D) 以上都是39. 在机器学习中,决策树的主要优点是:A) 易于理解和解释B) 计算效率高C) 对缺失值不敏感D) 以上都是40. 下列哪种算法适用于图像分割?A) 卷积神经网络(CNN)B) 循环神经网络(RNN)C) 随机森林D) 支持向量机41. 在机器学习中,L2正则化主要用于:A) 减少模型复杂度B) 增加特征数量C) 特征选择D) 提高模型精度42. 下列哪种方法可以用于处理时间序列数据的季节性?A) 移动平均B) 季节分解C) 差分D) 以上都是43. 在机器学习中,Bagging的主要目的是:A) 减少模型的方差B) 减少模型的偏差C) 增加数据量D) 提高计算速度44. 下列哪种算法适用于序列数据处理?A) 卷积神经网络(CNN)B) 循环神经网络(RNN)C) 随机森林D) 支持向量机45. 在机器学习中,AdaBoost的主要目的是:A) 减少模型的方差B) 减少模型的偏差C) 增加数据量D) 提高计算速度46. 下列哪种方法可以用于处理文本数据的情感分析?A) 词袋模型(Bag of Words)B) TF-IDFC) 词嵌入D) 以上都是47. 在机器学习中,支持向量机(SVM)的主要优点是:A) 适用于高维数据B) 计算效率高C) 对缺失值不敏感D) 以上都是48. 下列哪种算法适用于推荐系统中的用户行为分析?A) 协同过滤B) 内容过滤C) 混合过滤D) 以上都是49. 在机器学习中,交叉验证的主要类型包括:A) K-折交叉验证B) 留一法交叉验证C) 随机划分交叉验证D) 以上都是50. 下列哪种方法可以用于处理图像数据?A) 卷积神经网络(CNN)B) 循环神经网络(RNN)C) 随机森林D) 支持向量机51. 在机器学习中,梯度提升机(GBM)的主要优点是:A) 适用于高维数据B) 计算效率高C) 对缺失值不敏感D) 以上都是52. 下列哪种算法适用于异常检测中的离群点检测?A) 线性回归B) 决策树C) 支持向量机D) 孤立森林(Isolation Forest)53. 在机器学习中,特征提取的主要目的是:A) 减少特征数量B) 提高模型性能C) 增加数据量D) 简化数据处理答案:1. B2. C3. C4. C5. B6. C7. C8. B9. C10. D11. D12. C13. C14. C15. C16. B17. D18. D19. C20. A21. C22. D23. B24. C25. B26. D27. B28. D29. B30. D31. C32. B33. B34. D35. A36. C37. B38. D39. D40. A41. A42. D43. A44. B45. B46. D47. A48. D49. D50. A51. D52. D53. B。

ZEISS OPMI pico 耳鼻喉部手术镜说明书

ZEISS OPMI pico 耳鼻喉部手术镜说明书

Performance you can trustKeeping you focused on what matters mostWhether for ear, nose or laryngeal procedures, ENT specialists around theworld put their trust in the premium optical performance and proven quality they have come to expect from ZEISS for their daily work.OPMI® pico from ZEISS offers the clarity, usability and quality you require bycombining legendary ZEISS optics with user-friendly features in a compact and robust design.From examinations to minor outpatient surgery, ZEISS OPMI pico lets youfocus on what matters most – your patient.ZEISS OPMI picoPerformance you can trust2Clarity you can seeTrue colors By providing well-distributed, true-to-color light that strongly resembles natural daylight, LED illumination enables better differentiation of anatomical structures and vessels – even in deep and narrow channels – in a much brighter and clearer way than halogen illumination. Virtually maintenance-free, there is no need to replace light bulbs, thereby helping to reduce costs.ZEISS OPMI pico brings fine structuresand details into clear view. Leading-edge visualization technologies suchas LED illumination and Varioskop ® 100deliver clear visibility. More importantly,they help you to perform high-qualityexaminations, treatments and smalloutpatient surgeries with a high levelof consistency.ZEISS OPMI picoPerformance you can trustLED illumination for enhanced visibilityHalogen illumination for standardapplications4Enhanced visibilityaligned illumination help to supportenhanced visibility through narrowand deep channels. In addition, theVarioskop 100 objective lens provides alarge field of view while also enablingfine focus within the region of interest –without moving the surgical microscope.Maintain your ideal ergonomic positionby selecting a preferred workingdistance for ear, nose or laryngealprocedures using the positionableadjustment knob.Adjust the focal length during surgery with the Varioskop 1005Usability you can feelReady to use As a highly maneuverable manual surgical microscope, ZEISS OPMI pico is easy to use and position. Its simple, integrated design enables fast setup and easy maintenance. When moved from the stand-by position, the light and integrated HD camera are directly available for use.ZEISS OPMI pico is equipped with a user-optimized design and intelligent functions. Smartdesign elements such as the fully integrated HDvideo chain and a sensor-controlled stand-byposition enable a streamlined clinical workflow.Experience a compact design and ergonomicfunctions in your daily work.ZEISS OPMI picoPerformance you can trustAlways ready to go when you are6Impressive HD qualitypatients through the procedure orsimply share your expertise withcolleagues. The integrated HDvideo camera delivers 1080p high-definition images with high colorfidelity. Conveniently capture yourimages during treatments or surgicalprocedures with a foot control panelto further enhance your workflow.Share your views in high resolutionImages courtesy of:International Reference and Development Centre for Surgical Technology (IRDC), Leipzig, Germany7Maximum uptimeZEISS service agreements * encompassthe full range of support offerings toensure high device uptime and workflowconvenience. Services like a local servicehotline, quick response or preventivemaintenance ensure that you canalways focus on what you do best:caring for your patients.* S ervice offerings can vary in different countries. Please contact your local sales representative for more information.Quality you can rely onThe highest possible standards are an integralpart of any surgical microscope from ZEISS.ZEISS OPMI pico is designed to optimallysupport you for years to come. Its designallows you to easily upgrade.ZEISS OPMI picoPerformance you can trustWith its compact design, ZEISS OPMI pico is asurgical microscope you can rely on8Designed with your needs in mindMany ENT specialists around the world face a growing need to provide higherquality care at a better value. As a high-precision, high-performance instrument,the ZEISS OPMI pico offers just the right answer – delivering reliable support dayin and day out to successfully address your challenges.Shaping medical progress again and againAs one of the world‘s leading medical technology companies, ZEISS has enjoyedmore than 100 years of success marked by numerous product developments,milestones and gold standards – all in close cooperation with doctors. As a majordriving force of medical progress, ZEISS looks forward to shaping the next 100 years.9Tailor it to your needs ZEISS OPMI pico offers different mounting options to suit your specific working environment. It can be equipped with accessories and options according to your needs.Comfort T hand gripPosition your ZEISS OPMI pico with a comfortable hand grip.EndoportAttach an existing endoscope camera.Treatment unitIntegrate your ZEISS OPMI pico into atreatment unit.* 10S100 floor standTechnical dataS100 wall mountS100 ceiling mountS100 / OPMI pico from ZEISS Magnification Manual apochromatic magnification changer Eyepieces 10x wide-field eyepieces 12.5x wide-field eyepiecesTubesStraight tube, focal length f = 170 mm Tiltable tube 0-180°, f = 170 mmFoldable Tube f 170 / f 260, incl. PROMAG function for additional 50 % magnification and integrated rotate functionFocusObjective lens f = 250 mmObjective lenses from f = 200 mm to f = 400 mm, in steps of 50 mmVarioskop 100, focusable working distance 200-300 mmIllumination system 100 W halogen illumination LED illumination Hand gripComfort T hand grip Hand grips (front)Mount mobility 120° couplingStandard couplingSuspensionFloor standWall mount with long arm Ceiling mountIntegration into treatment unit *High Definition videoHD-ready 720p Full HD 1080pHD video camera live & streaming (Full HD 1080p) with recording license HD monitorsExternal video solutions Adapter SLR camera FlexioStill Adapter for digital camerasFlexioMotion Adapter for digital camcorders Endoport *AccessoriesVisionGuard ® Lens Protectors Surgical Drapes, sterile Sterilizable Asepsis Capsand hand grip coversInstrument tray on floor standStandard Option* P lease contact your local treatment unit dealer for more information.11Carl Zeiss Meditec AG Goeschwitzer Strasse 51–52 07745 JenaGermany/opmi-pico-ENT /med/contacts EN_3_1_45IVSUR.5928RevCPrintedinGermanyCZ-IV/218Thecontentsofthebrochuremaydifferfromthecurrentstatusofapprovaloftheproductorserviceofferinginyourcountry.Pleasecontactourregionalrepresentativeformoreinformation.Subjecttochangesindesignandscopeofdeliveryandduetoongoingtechnicaldevelopment.OPMI,VarioskopandVisionGuardareeithertrademarksorregisteredtrademarksofCarlZeissMeditecAGorothercompaniesoftheZEISSGroupinGermanyand/orothercountries.©CarlZeissMeditecAG,218.Allrightsreserved.。

OpticsExpress模版

OpticsExpress模版

OpticsExpress模版Instructions for the preparation of a manuscript for OSA Express JournalsDan McDonold1 and Theresa Miller2,3,*1Peer Review, Publications Department, Optical Society of America, 2010 Massachusetts Avenue, NW, Washington,D.C. 20036, USA2Publications Department, Optical Society of America, 2010 Massachusetts Avenue, NW, Washington, D.C. 20036,USA3Currently with the Department of Electronic Journals, Optical Society of America, 2010 Massachusetts Avenue, NW, Washington, D.C. 20036, USA*opex@/doc/529558f3fc4ffe473268abee.htmlAbstract:Updated 1 February 2016. Explicit and detailed rules are givenfor preparing a manuscript for OSA Express Journals. After a generalintroduction and a summary of the basic requirements, specific guidelinesare given for all major manuscript elements (such as abstract, headings,figures, tables, and references) to achieve optimal typographic quality. Theuse of complete and properly formatted references is particularly important.Adherence to these guidelines will significantly expedite the production ofyour paper.2016 Optical Society of AmericaOCIS codes: (000.0000) General; (000.2700) General science.References and links1.P. J. Harshman, T. K. Gustafson, and P. Kelley, ―Title of paper,‖ J. Chem. Phys. 3, (to be published).2.K. Gallo and G. Assanto, ―All-optical diode based on second-harmonic generation in an asymmetricwaveguide,‖ J. Opt. Soc. Am. B 16(2), 267–269 (1999).3. B. R. Masters, ―Three-dimensional microscopic tomographic imagings of the cataract in a human lens in vivo,‖Opt. Express 3(9), 332–338 (1998).4. D. Yelin, D. Oron, S. Thiberge, E. Moses, and Y. Silberberg, ―Multiphoton plasmon-resonance microscopy,‖Opt. Express 11(12), 1385–1391 (2003).1. IntroductionAdherence to the specifications listed in this style guide is essential for efficient review and publication of submissions. Since OSA does not routinely perform copyediting and typesetting for the express journals, the use of the macros in this style guide is critical to providing a consistent appearance.OSA Publishing’s express jou rnals create archival-quality XML along with PDF output. XML is the industry standard for producing and archiving scientific journal articles and is used in producing all other OSA journals. Having full-text XML will allow the express journals to be indexed more accurately and completely in MEDLINE, PubMed Central, and other databases; it will also allow the journal to meet its archival obligations and to prepare for new services, such as full-text semantic search and repurposing of content.OSA accepts Word and LaTeX submissions; however, we encourage authors to submit papers in MS Word. OSA will not publish the same Word file that authors submit for their final revisions, so it is imperative that authors carefully check the final version of their paper before paying the publication fee. OSA uses a Word plug-in called eXtyles to normalize, format, tag, and parse the file into full-text XML. eXtyles automatically reformats, checks, and updates the references against the CrossRef and PubMed databases. In addition to running other auto-redact editing rules, eXtyles checks all reference, figure, table and equation callouts in the text to ensure all items are cited.Except for numbering and titling of sections, which may not be desirable for short articles, the express journal style and layout rules have been followed in this guide. There is a checklist available in Section 6 that summarizes the style specifications. 2. Page layout and lengthPaper size should be U.S. Letter, 21.505 cm x 27.83 cm (8.5 in. x 11 in.). The printing area should be set to 13.28 cm x 21.54 cm (5.25 in. x 8.5 in.); margins should be set for a 2.54-cm (1 in.) top and 4.11-cm (1.625 in.) left, right, and bottom.To maintain a rapid publication cycle, the recommended page length for an express journal article is 6 pages. Higher publication fees apply to articles 7–15 pages in length. There is an additional per-page fee for manuscripts longer than 15 pages.3. SoftwareOSA Express Journals accepts Word and TeX files.4. Typographical styleAll fonts for text should be some version of Times New Roman. Text should be 10-pt., the title should be 18-pt., and the affiliation and references should be 8-pt. Do not add hyphenation at the end of a line.4.1 TitleCenter the title. The title should be in 18-pt. bold font. Use initial cap for first word in title or for proper nouns. Use lowercase following colon. Title should not begin with an article or contain the words "first," "new" or "novel."4.2 Author nameCenter author names in 10-pt. bold font. Author names should appear as used for conventional publication, with first and middle names or initials followed by surname. Every effort should be made to keep author names consistent from one paper to the next as they appear within OSA publications.4.3 Author affiliationAll authors and affiliations should be styled in the following below. If all authors share one affiliation, superscript numbers are not needed. The corresponding author will have an asterisk correlating to an email address. All authors must be grouped together using superscripts to callout each affiliation. Hard returns (Enter key) must be used to separate each individual affiliation. Abbreviations should not be used. Center the e-mail address of author(s) directly below the affiliation. Please include the country at the end of the affiliation.Dan McDonold1 and Theresa Miller2,*1Peer Review, Publications Department, Optical Society of America, Washington, D.C., 20036, USA 2Publications Department, Optical Society of America, Washington, D.C., 20036, USA*opex@/doc/529558f3fc4ffe473268abee.htmlOption 1 for affiliation line with two email addresses (only one for the corresponding author)Dan McDonold1,3 and Theresa Miller2,*1Peer Review, Publications Department, Optical Society of America, Washington, D.C., 20036, USA 2Publications Department, Optical Society of America, Washington, D.C., 20036, USA3xyz@/doc/529558f3fc4ffe473268abee.html*opex@/doc/529558f3fc4ffe473268abee.htmlOption 2 for affiliation line with two email addresses (no asterisk used to denote corresponding authorship, implying that the two email addresses share corresponding authorship equally)Dan McDonold1,3 and Theresa Miller2,41Peer Review, Publications Department, Optical Society of America, Washington, D.C., 20036, USA 2Publications Department, Optical Society of America, Washington, D.C., 20036, USA3xyz@/doc/529558f3fc4ffe473268abee.html4opex@/doc/529558f3fc4ffe473268abee.html4.4 AbstractBegin the section with the word ―Abstract:‖ in bold print followed by a colon. Indent left and right margins 1.27 cm (0.5 in.). Font size should be 10-pt. and alignment double (left and right) justified.The abstract should be limited to approximately 100 words. It should be an explicit summary of the paper that states the problem, the methods used, and the major results and conclusions. It also should contain the relevant key words that would allow it to be found in a cursory computerized search. If the work of another author is cited in the abstract, that citation should be written out without a number, [e.g., journal, volume, first page, and year (Opt. Express 22, 1234 (2014).)], and a separate citation should be included in the body of the text. The first reference cited in the main text must be [1]. Do not include numbers, bullets, or lists inside the abstract.4.5. CopyrightThe line immediately following the abstract should be2016 Optical Society of Americain 9-pt. type. Please be sure to update this line with the appropriate publication year if needed. Indentation should match the abstract, i.e., 1.27 cm (0.5 in.). Insert a 4-pt. space above and below the copyright line. See the first page of these instructions.4.6 OCIS subject classificationOptics Classification and Indexing Scheme (OCIS) subject classifications should be included at the end of the abstract. OCIS codes should be provided to help with indexing. List the OCIS code in parenthesis, followed by the term spelled out; separate OCIS terms with semicolons. Each paper must contain two to six OCIS codes. Use 8-pt. type for this line. Please avoid using OCIS codes (000.0000) General or (000.2700) General science, and instead customize these codes to best represent the topics of your manuscript.OCIS codes can be selected during upload. Follow the link for a complete listing.OCIS codes: (260.1440) Birefringence; (050.1950) Diffraction gratings4.7 Main textThe first line of the first paragraph of a section or subsection should start flush left. The first line of subsequent paragraphs within the section or subsection should be indented 0.62 cm (0.2 in.). All main text should be alignment double (left and right) justified.Section headings may be numbered consecutively and consistently throughout the paper in Arabic numbers and typed in bold. Use an initial capital letter followed by lowercase, except for proper names, abbreviations, etc. Always start headings flush left. Do not include references to the literature, illustrations, or tables in headings. Insert a 6-pt. space above and below each section heading as shown in this paper.Subsection headings may be numbered consecutively in Arabic numbers to the right of the decimal point, with the section number to the left of the decimal point as shown in this paper. Subsection headings should be in italics, with an initial capital letter followed by lowercase, except for proper names, abbreviations, etc. Start subsection headings flush left. Do not include references to the literature, illustrations, or tables in headings. Create a 6-pt. space above and below each subsection heading as shown in this paper.Numbering of section headings and subsection headings is optional but must be used consistently throughout papers in which it is applied.4.8 EquationsThe express journals do not accept equations built using the Word 2007 or 2010 Equation Builder. All display equations should be created in MathType (or the Microsoft Equation editor from Design Science). Inline equations can be created with these tools or by using keyboard and Unicode characters where needed for the best quality line spacing. We stronglyencourage authors to use MathType 6.7. Note that LaTeX users can type LaTeX code directly into MathType for rendering in Word.Equations should be centered, unless they are so long that less than 1 cm will be left between the end of the equation and the equation number, in which case they may run on to the next line. Equations should have a 6-pt. space above and below the text. Equation numbers should appear at the right-hand margin, in parenthesis. For long equations, the equation number may appear on the next line. For very long equations, the right side of the equation should be broken into approximately equal parts and aligned to the right of the equal sign. The equation number should appear only at the right hand margin of the last line of the equation:(1)All equations should be numbered in the order in which they appear and should be referenced from within the main text as Eq. (1).In-line math of simple fractions should use parentheses when necessary to avoid ambiguity; for example, to distinguish between 1/(n - 1) and 1/n - 1. Exceptions to this are the proper fractions such as ?, which are better left in this form. Summations and integrals that appear within text such as ()-1211-22n n n n =∞=∑ should have limits placed to the right of the symbol to reduce white space. Use MathType, Design Science Equation Editor, or Unicode character sets for in-text and display notation wherever possible.4.9 References and linksReferences should appear at the top of the article, below the abstract, in the order in which they are referenced in the body of the paper (see below). The font should be 8-pt. aligned left. Lines should be single-spaced. The words ―References and links ‖ should head the section (no number) in bold print followed by one blank line, directly above the first reference. Insert a 6-pt. space above the ―References and links ‖ line. All references should be indented 0.5 cm (0.2 in), with succeeding lines indented sufficiently to preserve alignment. The references section should be delimited by horizontal rules above and below the section, separated by at least 6-pts. of white space from the text.OSA Express Journals use numerical notation in brackets for bibliographic citations. At the point of citation within the main text, designate the reference by typing the number in after the last corresponding word [1]. Reference numbers should precede a comma or period [2]. Two references [3,4], should be included together, separated by a comma, while three or more consecutive references should be indicated by the bounding numbers and a dash [1–4].The express journals follow the following citation style:Journal paperFor journal articles, authors are listed first, followed by the article’s full title in quotes, the journal’s title abbreviation, the volume number in bold, the issue number in Roman and parenthesis, inclusive page numbers, and the year in parentheses. Journal titles are required. Do not include web addresses in published journal citations —these will be added post-publication.1. C. van Trigt, ―Visual s ystem-response functions and estimating reflectance,‖ J. Opt. Soc. Am. A 14(4), 741–755 (1997).2.S. Yerolatsitis, I. Gris-Sánches, and T. A. Birks, ―Adiabatically-tapered fiber mode multiplexers,‖ Opt. Express22(1), 608–617 (2014).Journal paper identified by paper numberDo not provide the number of pages; the paper number is sufficient.3.L. Rippe, B. Julsgaard, A. Walther, Y. Ying, and S. Kr?ll, ―Experimental quantum-state tomography of a solid-state qubit,‖ Phys. Rev. A 77, 022307 (2008).BookFor citation of a book as a whole or book chapter, authors or editors are listed first, followed by title in italics, and publisher and year in parenthesis. Chapter number may be added if applicable.4.T. Masters, Practical Neural Network Recipes in C++ (Academic, 1993).5. F. Ladouceur and J. D. Love, Silica-Based Buried Channel Waveguides and Devices (Chapman & Hall, 1995),Chap. 8.Article in a bookFor monographs in books, authors are listed first, followed by article’s full title in quotes, the word ―in,‖ followed by the book title in italics, the editors of the book, and the publisher and publication year in parenthesis.6. D. F. Edwards, ―Silicon (Si),‖ in Handbook of Optical Constants of Solids, E. D. Palik, ed. (Academic, 1985). Paper in published conference proceedings7.R. E. Kalman, ―Algebraic aspects of the generalized inverse of a rectangular matrix,‖ in Proceedings ofAdvanced Seminar on Generalized Inverse and Applications, M. Z. Nashed, ed. (Academic, 1976), pp. 111–124. Paper published in OSA conference proceedings8.R. Craig and B. Gignac, ―High-power 980-nm pump lasers,‖ in Optical Fiber Communication Conference, Vol.2 of 1996 OSA Technical Digest Series (Optical Society of America, 1996), paper ThG1.Paper in unpublished conference proceedings9. D. Steup and J. W einzierl, ―Resonant THz-meshes,‖ presented at the Fourth International Workshop on THz Electronics, Erlangen-Tennenlohe, Germany, 5–6 Sept. 1996.SPIE proceedingsFor later SPIE proceedings with a paper number, cite just the paper number and not any page information.10.S. K. Griebel, M. Richardson, K. E. Devenport, and H. S. Hinton, ―Experimental performance of an ATM-based buffered hyperplane CMOS-SEED smart pixel array,‖ Proc. SPIE 3005, 254–256 (1997).11.S. Gu, F. Shao, G. Jiang, F. Li, and M. Yu, ―An object ive visibility threshold measurement method forasymmetric stereoscopic images,‖ Proc. SPIE 8205, 820505 (2011).IEEE proceedings12.T. Darrel and K. Wohn, ―Pyramid based depth from focus,‖ in Proceedings of IEEE Conference on ComputerVision and Pattern Recognition (IEEE, 1988), pp. 504–509.Paper accepted for publication13. D. Piao, ―Cancelation of coherent artifacts in optical coherence tomography imaging,‖ Appl. Opt. (to be published).14. D. W. Diehl and T. D. Visser, ―Phase singularities of the longitudinal fie ld components in the focal region of ahigh-aperture optical system,‖ J. Opt. Soc. Am. A, doc. ID 56789 (posted 11 November 2005, in press).Manuscript in preparation15.J. Q. Smith, Laboratory for Laser Energetics, University of Rochester, 250 East River Road, Rochester, N.Y.14623, and K. Marshall are preparing a manuscript to be called ―Optical effects in liquid crystals.‖Personal communication 16.T. Miller, Publications Department, Optical Society of America, 2010 Massachusetts Avenue, N.W.,Washington, D.C., 20036 (personal communication, 2010).Electronic citationsInternet links may be included as references. Internet links should list the author, title (substitute file name, if needed), and thefull URL (universal resource locator). Include the date of access, if relevant.17.Extreme Networks white paper, ―Virtual metropolitan area networks,‖ (Extreme Networks, 2001),/doc/529558f3fc4ffe473268abee.html /technology/whitepapers/vMAN.asp.18. A. G. Ramm, ―Invisible obstacles,‖ /doc/529558f3fc4ffe473268abee.html /abs/math-ph/0608034.4.10 AcknowledgmentsAcknowledgments should be included at the end of the document. The section title should read ―Acknowledgments‖ in 10-pt. bold font. The section title should not follow the numbering scheme of the body of the paper. The body of the section should follow the font and layout of the body of the paper (see Subsection 4.7 above). Please identify all appropriate funding sources by name and contract number in the Acknowledgment section.OSA participates in Cross Ref’s Funding Data, a service that provides a standard way to report funding sources for published scholarly research. To ensure consistency, please be sure to add any funding sources and contract numbers from your Acknowledgments to Prism during submission, and update with any changes to your funding sources and contract numbers in Prism during any revision stages.5. Figures, supplementary materials, and tables5.1 FiguresFigures should be included directly in the document. All photographs must be in digital form and placed appropriately in the electronic document. All illustrations must be numbered consecutively (i.e., not by section) with Arabic numbers. The size of a figure should be commensurate with the amount and value of the information conveyed by the figure.Authors must use one image file per figure. Figures must be inserted as objects that are fixed and move with the text, not as floating objects. Figures should never be placed in a table environment or embedded inside the text.All the figures should be centered. No part of a figure should go beyond the typing area. Place figures as closely as possible to where they are mentioned in the text. Figures should be numbered consecutively in the order of appearance and citation in the text. Be sure to cite every figure.All figure captions should be centered beneath the figure. Longer figure captions should be centered beneath the figure and alignment double (left and right) justified, but are not to exceed the left and right edge of the figure by more than 0.5 in. The abbreviation ―Fig.‖ for figure should appear first followed by the figure number and a period. Captions should be in 8- pt. font. At least one line of space should be left before the figure and after the caption.Fig. 1. Sample figure.5.2 Supplementary materials in OSA express journalsMost OSA journals allow authors to include supplementary materials as integral parts of a manuscript. Such materials are subject to the same editorial standards and peer review procedures along with the rest of the paper and should be uploaded and described using OSA’s Prism manuscript system.Authors can submit appropriate visualizations or small data files (see details below) for OSA to host. Large datasets and code or simulation files can be included but must be placed in an appropriate archival repository and cited as described here. Table 1. Supplementary Materials Supported in OSA Journals aa Optica(see Supplementary Materials in Optica for details). For all other OSA journals, supplemental text must be included as appendices within the primary manuscript.Video visualizations (formerly media files) are the most commonly submitted type of supplementary materials for the express journals. They typically illustrate a synopsis of research results. They are integral and as such should be included only when they convey essential information beyond what can be presented within the article's PDF representation. Video visualizations should be uploaded upon submission and peer-reviewed along with the manuscript. Video files must use open compression standards for display on broadly available applications such as VLC, Apple QuickTime, or Windows Media Player. MOV, AVI, MPG, and MP4 video containers are accepted. The following video guidelines will help with the submission process:15 MB is the recommended maximum video file size.720 x 480 pixels (width by height) is the recommended screen size.If appropriate, insert a representative frame from the video in the manuscript as a figure.Minimize file size by using an acceptable codec such as QuickTime, x264, or XviD.HandBrake is an open source tool for converting video to common codecs.Videos must be playable on all platforms using QuickTime or VLC.Animations must be formatted into a standard video container.Visualizations must be associated with a figure, table, or equation OR be referenced in the results section of the manuscript. Use the label "Visualization" and the item number toidentify the visualization.Fig. 5. Three traps create three rings of magnetic nanoparticles. The rings interact with oneanother (see Visualization 3). [From Masajada et al., Opt. Lett. 38, 3910 (2013).]Please refer to the Author Guidelines for Supplementary Materials for more detailed instructions and other acceptable supplementary material types.5.3 TablesTables should be centered and numbered consecutively. Authors must use Word’s Table editor to insert tables. Authors must not import tables from Excel. All content for each table should be in a single Word table (do not split content for a single table across multiple Word tables). Tables should use horizontal lines to delimit the top and bottom of the table and column headings. Detailed explanations or table footnotes should be typed directly beneath the table, but not in a table cell. Table footnote labels should be text; numbers or special characters are not permitted. Position tables as closely as possible to where they are mentioned in the main text.Table 2. Optical Constants of Thin Films of Materials a83.4 nm 121.6 nmMaterial n K n kIr 1.182 0.865 1.450 1.040MgF2 1.584 0.487 1.682 0.0627Al 0.09874 0.1915 0.0424 1.137Mo 0.98 1.08 0.78 1.03C 1.16 1.29 1.85 1.10a From Appl. Opt. 40, 1128 (2001).6. Article thumbnail uploadAuthors have the option to upload a thumbnail image that will appear next to the published article on the Forthcoming, Current Issue, and Abstract pages. Please note that if authors do not choose a file, OSA Production Staff will choose an image from the submission. For precise representation of an article, we recommend that authors choose and upload the thumbnail image.Authors must submit a .JPG file. The image will be resized automatically to 100 x 100 pixels. For best results, authors should upload an image this size or an image with square dimensions.The 100 x 100 pixel image will be displayed on the article abstract page and a 50 x 50 pixel image will be displayed on the Table of Contents page.Fig. 3. Preview of thumbnail image display on the author submission page.7. SummaryConforming to the specifications listed above is of critical importance to the speedy publication of a manuscript. Authors should use the following style guide checklist before submitting an article.Table 3. OSA Express Journals style guide checklistAuthor Name 10 CenterEmail addressCopyright 9 0.5 in.First paragraph Subsequent paragraphs None0.2 in.subsection is not indented. Thefirst line of subsequentparagraphs is indented 0.2 in.Headings below each heading. Sectionheaders: BoldSubsection headers: Italic Equations 10 None Center Eq. Number: right tab to end oflast line of Eq., in parentheses. References and Links 8 0.2 in. Left Bold ―References and links‖.Delimit with horizontal rules.Figures Centerleft/right.Table Heads 8 None Center Long heads follow table margins.7. ConclusionAfter proofreading, the final step in submitting a manuscript to the express journals is to visit Prism, and submit your manuscript. For further instructions, please see the Optics Express, Biomedical Optics Express, or Optical Materials Express Author Information page.。

基于暗通道先验的图像去雾算法改进

基于暗通道先验的图像去雾算法改进

基于暗通道先验的图像去雾算法改进王凯;王延杰;樊博【摘要】To develop an algorithm for haze removal based on the physics model,this paper proposes an improved and fast method for single image haze removal using dark channel prior.First,we intro-duce the degraded model for describing the formation of a haze image and several algorithms based on this model.Second,we introduce the method of He’s single image haze removal using dark channel prior.The image quality of He’s method is satisfactory,but it is a time consuming method because of refining the transmission map with guide filter.We propose an optimized method based on estimating transmission by scene depth directly and the runtime of the new algorithm decreases a lot.Finally,we realize the algorithm in MATLAB and compare the runtime with the original algorithm.Results dem-onstrates that the new method provides a reliable transmission estimation and a better image quality with around 40% computation time of He’s method,and the results of haze images with sky are less halos.The optimized method execute fast and the results demonstrate the new method abilities to re-move the haze layer as well as provide a high quality transmission estimation as a byproduct of haze removal which can be used for other applications.%为了实现基于物理模型的图像复原去雾算法,文中提出了一种改进的基于暗通道先验的图像去雾算法。

物理学专业英语

物理学专业英语

华中师范大学物理学院物理学专业英语仅供内部学习参考!2014一、课程的任务和教学目的通过学习《物理学专业英语》,学生将掌握物理学领域使用频率较高的专业词汇和表达方法,进而具备基本的阅读理解物理学专业文献的能力。

通过分析《物理学专业英语》课程教材中的范文,学生还将从英语角度理解物理学中个学科的研究内容和主要思想,提高学生的专业英语能力和了解物理学研究前沿的能力。

培养专业英语阅读能力,了解科技英语的特点,提高专业外语的阅读质量和阅读速度;掌握一定量的本专业英文词汇,基本达到能够独立完成一般性本专业外文资料的阅读;达到一定的笔译水平。

要求译文通顺、准确和专业化。

要求译文通顺、准确和专业化。

二、课程内容课程内容包括以下章节:物理学、经典力学、热力学、电磁学、光学、原子物理、统计力学、量子力学和狭义相对论三、基本要求1.充分利用课内时间保证充足的阅读量(约1200~1500词/学时),要求正确理解原文。

2.泛读适量课外相关英文读物,要求基本理解原文主要内容。

3.掌握基本专业词汇(不少于200词)。

4.应具有流利阅读、翻译及赏析专业英语文献,并能简单地进行写作的能力。

四、参考书目录1 Physics 物理学 (1)Introduction to physics (1)Classical and modern physics (2)Research fields (4)V ocabulary (7)2 Classical mechanics 经典力学 (10)Introduction (10)Description of classical mechanics (10)Momentum and collisions (14)Angular momentum (15)V ocabulary (16)3 Thermodynamics 热力学 (18)Introduction (18)Laws of thermodynamics (21)System models (22)Thermodynamic processes (27)Scope of thermodynamics (29)V ocabulary (30)4 Electromagnetism 电磁学 (33)Introduction (33)Electrostatics (33)Magnetostatics (35)Electromagnetic induction (40)V ocabulary (43)5 Optics 光学 (45)Introduction (45)Geometrical optics (45)Physical optics (47)Polarization (50)V ocabulary (51)6 Atomic physics 原子物理 (52)Introduction (52)Electronic configuration (52)Excitation and ionization (56)V ocabulary (59)7 Statistical mechanics 统计力学 (60)Overview (60)Fundamentals (60)Statistical ensembles (63)V ocabulary (65)8 Quantum mechanics 量子力学 (67)Introduction (67)Mathematical formulations (68)Quantization (71)Wave-particle duality (72)Quantum entanglement (75)V ocabulary (77)9 Special relativity 狭义相对论 (79)Introduction (79)Relativity of simultaneity (80)Lorentz transformations (80)Time dilation and length contraction (81)Mass-energy equivalence (82)Relativistic energy-momentum relation (86)V ocabulary (89)正文标记说明:蓝色Arial字体(例如energy):已知的专业词汇蓝色Arial字体加下划线(例如electromagnetism):新学的专业词汇黑色Times New Roman字体加下划线(例如postulate):新学的普通词汇1 Physics 物理学1 Physics 物理学Introduction to physicsPhysics is a part of natural philosophy and a natural science that involves the study of matter and its motion through space and time, along with related concepts such as energy and force. More broadly, it is the general analysis of nature, conducted in order to understand how the universe behaves.Physics is one of the oldest academic disciplines, perhaps the oldest through its inclusion of astronomy. Over the last two millennia, physics was a part of natural philosophy along with chemistry, certain branches of mathematics, and biology, but during the Scientific Revolution in the 17th century, the natural sciences emerged as unique research programs in their own right. Physics intersects with many interdisciplinary areas of research, such as biophysics and quantum chemistry,and the boundaries of physics are not rigidly defined. New ideas in physics often explain the fundamental mechanisms of other sciences, while opening new avenues of research in areas such as mathematics and philosophy.Physics also makes significant contributions through advances in new technologies that arise from theoretical breakthroughs. For example, advances in the understanding of electromagnetism or nuclear physics led directly to the development of new products which have dramatically transformed modern-day society, such as television, computers, domestic appliances, and nuclear weapons; advances in thermodynamics led to the development of industrialization; and advances in mechanics inspired the development of calculus.Core theoriesThough physics deals with a wide variety of systems, certain theories are used by all physicists. Each of these theories were experimentally tested numerous times and found correct as an approximation of nature (within a certain domain of validity).For instance, the theory of classical mechanics accurately describes the motion of objects, provided they are much larger than atoms and moving at much less than the speed of light. These theories continue to be areas of active research, and a remarkable aspect of classical mechanics known as chaos was discovered in the 20th century, three centuries after the original formulation of classical mechanics by Isaac Newton (1642–1727) 【艾萨克·牛顿】.University PhysicsThese central theories are important tools for research into more specialized topics, and any physicist, regardless of his or her specialization, is expected to be literate in them. These include classical mechanics, quantum mechanics, thermodynamics and statistical mechanics, electromagnetism, and special relativity.Classical and modern physicsClassical mechanicsClassical physics includes the traditional branches and topics that were recognized and well-developed before the beginning of the 20th century—classical mechanics, acoustics, optics, thermodynamics, and electromagnetism.Classical mechanics is concerned with bodies acted on by forces and bodies in motion and may be divided into statics (study of the forces on a body or bodies at rest), kinematics (study of motion without regard to its causes), and dynamics (study of motion and the forces that affect it); mechanics may also be divided into solid mechanics and fluid mechanics (known together as continuum mechanics), the latter including such branches as hydrostatics, hydrodynamics, aerodynamics, and pneumatics.Acoustics is the study of how sound is produced, controlled, transmitted and received. Important modern branches of acoustics include ultrasonics, the study of sound waves of very high frequency beyond the range of human hearing; bioacoustics the physics of animal calls and hearing, and electroacoustics, the manipulation of audible sound waves using electronics.Optics, the study of light, is concerned not only with visible light but also with infrared and ultraviolet radiation, which exhibit all of the phenomena of visible light except visibility, e.g., reflection, refraction, interference, diffraction, dispersion, and polarization of light.Heat is a form of energy, the internal energy possessed by the particles of which a substance is composed; thermodynamics deals with the relationships between heat and other forms of energy.Electricity and magnetism have been studied as a single branch of physics since the intimate connection between them was discovered in the early 19th century; an electric current gives rise to a magnetic field and a changing magnetic field induces an electric current. Electrostatics deals with electric charges at rest, electrodynamics with moving charges, and magnetostatics with magnetic poles at rest.Modern PhysicsClassical physics is generally concerned with matter and energy on the normal scale of1 Physics 物理学observation, while much of modern physics is concerned with the behavior of matter and energy under extreme conditions or on the very large or very small scale.For example, atomic and nuclear physics studies matter on the smallest scale at which chemical elements can be identified.The physics of elementary particles is on an even smaller scale, as it is concerned with the most basic units of matter; this branch of physics is also known as high-energy physics because of the extremely high energies necessary to produce many types of particles in large particle accelerators. On this scale, ordinary, commonsense notions of space, time, matter, and energy are no longer valid.The two chief theories of modern physics present a different picture of the concepts of space, time, and matter from that presented by classical physics.Quantum theory is concerned with the discrete, rather than continuous, nature of many phenomena at the atomic and subatomic level, and with the complementary aspects of particles and waves in the description of such phenomena.The theory of relativity is concerned with the description of phenomena that take place in a frame of reference that is in motion with respect to an observer; the special theory of relativity is concerned with relative uniform motion in a straight line and the general theory of relativity with accelerated motion and its connection with gravitation.Both quantum theory and the theory of relativity find applications in all areas of modern physics.Difference between classical and modern physicsWhile physics aims to discover universal laws, its theories lie in explicit domains of applicability. Loosely speaking, the laws of classical physics accurately describe systems whose important length scales are greater than the atomic scale and whose motions are much slower than the speed of light. Outside of this domain, observations do not match their predictions.Albert Einstein【阿尔伯特·爱因斯坦】contributed the framework of special relativity, which replaced notions of absolute time and space with space-time and allowed an accurate description of systems whose components have speeds approaching the speed of light.Max Planck【普朗克】, Erwin Schrödinger【薛定谔】, and others introduced quantum mechanics, a probabilistic notion of particles and interactions that allowed an accurate description of atomic and subatomic scales.Later, quantum field theory unified quantum mechanics and special relativity.General relativity allowed for a dynamical, curved space-time, with which highly massiveUniversity Physicssystems and the large-scale structure of the universe can be well-described. General relativity has not yet been unified with the other fundamental descriptions; several candidate theories of quantum gravity are being developed.Research fieldsContemporary research in physics can be broadly divided into condensed matter physics; atomic, molecular, and optical physics; particle physics; astrophysics; geophysics and biophysics. Some physics departments also support research in Physics education.Since the 20th century, the individual fields of physics have become increasingly specialized, and today most physicists work in a single field for their entire careers. "Universalists" such as Albert Einstein (1879–1955) and Lev Landau (1908–1968)【列夫·朗道】, who worked in multiple fields of physics, are now very rare.Condensed matter physicsCondensed matter physics is the field of physics that deals with the macroscopic physical properties of matter. In particular, it is concerned with the "condensed" phases that appear whenever the number of particles in a system is extremely large and the interactions between them are strong.The most familiar examples of condensed phases are solids and liquids, which arise from the bonding by way of the electromagnetic force between atoms. More exotic condensed phases include the super-fluid and the Bose–Einstein condensate found in certain atomic systems at very low temperature, the superconducting phase exhibited by conduction electrons in certain materials,and the ferromagnetic and antiferromagnetic phases of spins on atomic lattices.Condensed matter physics is by far the largest field of contemporary physics.Historically, condensed matter physics grew out of solid-state physics, which is now considered one of its main subfields. The term condensed matter physics was apparently coined by Philip Anderson when he renamed his research group—previously solid-state theory—in 1967. In 1978, the Division of Solid State Physics of the American Physical Society was renamed as the Division of Condensed Matter Physics.Condensed matter physics has a large overlap with chemistry, materials science, nanotechnology and engineering.Atomic, molecular and optical physicsAtomic, molecular, and optical physics (AMO) is the study of matter–matter and light–matter interactions on the scale of single atoms and molecules.1 Physics 物理学The three areas are grouped together because of their interrelationships, the similarity of methods used, and the commonality of the energy scales that are relevant. All three areas include both classical, semi-classical and quantum treatments; they can treat their subject from a microscopic view (in contrast to a macroscopic view).Atomic physics studies the electron shells of atoms. Current research focuses on activities in quantum control, cooling and trapping of atoms and ions, low-temperature collision dynamics and the effects of electron correlation on structure and dynamics. Atomic physics is influenced by the nucleus (see, e.g., hyperfine splitting), but intra-nuclear phenomena such as fission and fusion are considered part of high-energy physics.Molecular physics focuses on multi-atomic structures and their internal and external interactions with matter and light.Optical physics is distinct from optics in that it tends to focus not on the control of classical light fields by macroscopic objects, but on the fundamental properties of optical fields and their interactions with matter in the microscopic realm.High-energy physics (particle physics) and nuclear physicsParticle physics is the study of the elementary constituents of matter and energy, and the interactions between them.In addition, particle physicists design and develop the high energy accelerators,detectors, and computer programs necessary for this research. The field is also called "high-energy physics" because many elementary particles do not occur naturally, but are created only during high-energy collisions of other particles.Currently, the interactions of elementary particles and fields are described by the Standard Model.●The model accounts for the 12 known particles of matter (quarks and leptons) thatinteract via the strong, weak, and electromagnetic fundamental forces.●Dynamics are described in terms of matter particles exchanging gauge bosons (gluons,W and Z bosons, and photons, respectively).●The Standard Model also predicts a particle known as the Higgs boson. In July 2012CERN, the European laboratory for particle physics, announced the detection of a particle consistent with the Higgs boson.Nuclear Physics is the field of physics that studies the constituents and interactions of atomic nuclei. The most commonly known applications of nuclear physics are nuclear power generation and nuclear weapons technology, but the research has provided application in many fields, including those in nuclear medicine and magnetic resonance imaging, ion implantation in materials engineering, and radiocarbon dating in geology and archaeology.University PhysicsAstrophysics and Physical CosmologyAstrophysics and astronomy are the application of the theories and methods of physics to the study of stellar structure, stellar evolution, the origin of the solar system, and related problems of cosmology. Because astrophysics is a broad subject, astrophysicists typically apply many disciplines of physics, including mechanics, electromagnetism, statistical mechanics, thermodynamics, quantum mechanics, relativity, nuclear and particle physics, and atomic and molecular physics.The discovery by Karl Jansky in 1931 that radio signals were emitted by celestial bodies initiated the science of radio astronomy. Most recently, the frontiers of astronomy have been expanded by space exploration. Perturbations and interference from the earth's atmosphere make space-based observations necessary for infrared, ultraviolet, gamma-ray, and X-ray astronomy.Physical cosmology is the study of the formation and evolution of the universe on its largest scales. Albert Einstein's theory of relativity plays a central role in all modern cosmological theories. In the early 20th century, Hubble's discovery that the universe was expanding, as shown by the Hubble diagram, prompted rival explanations known as the steady state universe and the Big Bang.The Big Bang was confirmed by the success of Big Bang nucleo-synthesis and the discovery of the cosmic microwave background in 1964. The Big Bang model rests on two theoretical pillars: Albert Einstein's general relativity and the cosmological principle (On a sufficiently large scale, the properties of the Universe are the same for all observers). Cosmologists have recently established the ΛCDM model (the standard model of Big Bang cosmology) of the evolution of the universe, which includes cosmic inflation, dark energy and dark matter.Current research frontiersIn condensed matter physics, an important unsolved theoretical problem is that of high-temperature superconductivity. Many condensed matter experiments are aiming to fabricate workable spintronics and quantum computers.In particle physics, the first pieces of experimental evidence for physics beyond the Standard Model have begun to appear. Foremost among these are indications that neutrinos have non-zero mass. These experimental results appear to have solved the long-standing solar neutrino problem, and the physics of massive neutrinos remains an area of active theoretical and experimental research. Particle accelerators have begun probing energy scales in the TeV range, in which experimentalists are hoping to find evidence for the super-symmetric particles, after discovery of the Higgs boson.Theoretical attempts to unify quantum mechanics and general relativity into a single theory1 Physics 物理学of quantum gravity, a program ongoing for over half a century, have not yet been decisively resolved. The current leading candidates are M-theory, superstring theory and loop quantum gravity.Many astronomical and cosmological phenomena have yet to be satisfactorily explained, including the existence of ultra-high energy cosmic rays, the baryon asymmetry, the acceleration of the universe and the anomalous rotation rates of galaxies.Although much progress has been made in high-energy, quantum, and astronomical physics, many everyday phenomena involving complexity, chaos, or turbulence are still poorly understood. Complex problems that seem like they could be solved by a clever application of dynamics and mechanics remain unsolved; examples include the formation of sand-piles, nodes in trickling water, the shape of water droplets, mechanisms of surface tension catastrophes, and self-sorting in shaken heterogeneous collections.These complex phenomena have received growing attention since the 1970s for several reasons, including the availability of modern mathematical methods and computers, which enabled complex systems to be modeled in new ways. Complex physics has become part of increasingly interdisciplinary research, as exemplified by the study of turbulence in aerodynamics and the observation of pattern formation in biological systems.Vocabulary★natural science 自然科学academic disciplines 学科astronomy 天文学in their own right 凭他们本身的实力intersects相交,交叉interdisciplinary交叉学科的,跨学科的★quantum 量子的theoretical breakthroughs 理论突破★electromagnetism 电磁学dramatically显著地★thermodynamics热力学★calculus微积分validity★classical mechanics 经典力学chaos 混沌literate 学者★quantum mechanics量子力学★thermodynamics and statistical mechanics热力学与统计物理★special relativity狭义相对论is concerned with 关注,讨论,考虑acoustics 声学★optics 光学statics静力学at rest 静息kinematics运动学★dynamics动力学ultrasonics超声学manipulation 操作,处理,使用University Physicsinfrared红外ultraviolet紫外radiation辐射reflection 反射refraction 折射★interference 干涉★diffraction 衍射dispersion散射★polarization 极化,偏振internal energy 内能Electricity电性Magnetism 磁性intimate 亲密的induces 诱导,感应scale尺度★elementary particles基本粒子★high-energy physics 高能物理particle accelerators 粒子加速器valid 有效的,正当的★discrete离散的continuous 连续的complementary 互补的★frame of reference 参照系★the special theory of relativity 狭义相对论★general theory of relativity 广义相对论gravitation 重力,万有引力explicit 详细的,清楚的★quantum field theory 量子场论★condensed matter physics凝聚态物理astrophysics天体物理geophysics地球物理Universalist博学多才者★Macroscopic宏观Exotic奇异的★Superconducting 超导Ferromagnetic铁磁质Antiferromagnetic 反铁磁质★Spin自旋Lattice 晶格,点阵,网格★Society社会,学会★microscopic微观的hyperfine splitting超精细分裂fission分裂,裂变fusion熔合,聚变constituents成分,组分accelerators加速器detectors 检测器★quarks夸克lepton 轻子gauge bosons规范玻色子gluons胶子★Higgs boson希格斯玻色子CERN欧洲核子研究中心★Magnetic Resonance Imaging磁共振成像,核磁共振ion implantation 离子注入radiocarbon dating放射性碳年代测定法geology地质学archaeology考古学stellar 恒星cosmology宇宙论celestial bodies 天体Hubble diagram 哈勃图Rival竞争的★Big Bang大爆炸nucleo-synthesis核聚合,核合成pillar支柱cosmological principle宇宙学原理ΛCDM modelΛ-冷暗物质模型cosmic inflation宇宙膨胀1 Physics 物理学fabricate制造,建造spintronics自旋电子元件,自旋电子学★neutrinos 中微子superstring 超弦baryon重子turbulence湍流,扰动,骚动catastrophes突变,灾变,灾难heterogeneous collections异质性集合pattern formation模式形成University Physics2 Classical mechanics 经典力学IntroductionIn physics, classical mechanics is one of the two major sub-fields of mechanics, which is concerned with the set of physical laws describing the motion of bodies under the action of a system of forces. The study of the motion of bodies is an ancient one, making classical mechanics one of the oldest and largest subjects in science, engineering and technology.Classical mechanics describes the motion of macroscopic objects, from projectiles to parts of machinery, as well as astronomical objects, such as spacecraft, planets, stars, and galaxies. Besides this, many specializations within the subject deal with gases, liquids, solids, and other specific sub-topics.Classical mechanics provides extremely accurate results as long as the domain of study is restricted to large objects and the speeds involved do not approach the speed of light. When the objects being dealt with become sufficiently small, it becomes necessary to introduce the other major sub-field of mechanics, quantum mechanics, which reconciles the macroscopic laws of physics with the atomic nature of matter and handles the wave–particle duality of atoms and molecules. In the case of high velocity objects approaching the speed of light, classical mechanics is enhanced by special relativity. General relativity unifies special relativity with Newton's law of universal gravitation, allowing physicists to handle gravitation at a deeper level.The initial stage in the development of classical mechanics is often referred to as Newtonian mechanics, and is associated with the physical concepts employed by and the mathematical methods invented by Newton himself, in parallel with Leibniz【莱布尼兹】, and others.Later, more abstract and general methods were developed, leading to reformulations of classical mechanics known as Lagrangian mechanics and Hamiltonian mechanics. These advances were largely made in the 18th and 19th centuries, and they extend substantially beyond Newton's work, particularly through their use of analytical mechanics. Ultimately, the mathematics developed for these were central to the creation of quantum mechanics.Description of classical mechanicsThe following introduces the basic concepts of classical mechanics. For simplicity, it often2 Classical mechanics 经典力学models real-world objects as point particles, objects with negligible size. The motion of a point particle is characterized by a small number of parameters: its position, mass, and the forces applied to it.In reality, the kind of objects that classical mechanics can describe always have a non-zero size. (The physics of very small particles, such as the electron, is more accurately described by quantum mechanics). Objects with non-zero size have more complicated behavior than hypothetical point particles, because of the additional degrees of freedom—for example, a baseball can spin while it is moving. However, the results for point particles can be used to study such objects by treating them as composite objects, made up of a large number of interacting point particles. The center of mass of a composite object behaves like a point particle.Classical mechanics uses common-sense notions of how matter and forces exist and interact. It assumes that matter and energy have definite, knowable attributes such as where an object is in space and its speed. It also assumes that objects may be directly influenced only by their immediate surroundings, known as the principle of locality.In quantum mechanics objects may have unknowable position or velocity, or instantaneously interact with other objects at a distance.Position and its derivativesThe position of a point particle is defined with respect to an arbitrary fixed reference point, O, in space, usually accompanied by a coordinate system, with the reference point located at the origin of the coordinate system. It is defined as the vector r from O to the particle.In general, the point particle need not be stationary relative to O, so r is a function of t, the time elapsed since an arbitrary initial time.In pre-Einstein relativity (known as Galilean relativity), time is considered an absolute, i.e., the time interval between any given pair of events is the same for all observers. In addition to relying on absolute time, classical mechanics assumes Euclidean geometry for the structure of space.Velocity and speedThe velocity, or the rate of change of position with time, is defined as the derivative of the position with respect to time. In classical mechanics, velocities are directly additive and subtractive as vector quantities; they must be dealt with using vector analysis.When both objects are moving in the same direction, the difference can be given in terms of speed only by ignoring direction.University PhysicsAccelerationThe acceleration , or rate of change of velocity, is the derivative of the velocity with respect to time (the second derivative of the position with respect to time).Acceleration can arise from a change with time of the magnitude of the velocity or of the direction of the velocity or both . If only the magnitude v of the velocity decreases, this is sometimes referred to as deceleration , but generally any change in the velocity with time, including deceleration, is simply referred to as acceleration.Inertial frames of referenceWhile the position and velocity and acceleration of a particle can be referred to any observer in any state of motion, classical mechanics assumes the existence of a special family of reference frames in terms of which the mechanical laws of nature take a comparatively simple form. These special reference frames are called inertial frames .An inertial frame is such that when an object without any force interactions (an idealized situation) is viewed from it, it appears either to be at rest or in a state of uniform motion in a straight line. This is the fundamental definition of an inertial frame. They are characterized by the requirement that all forces entering the observer's physical laws originate in identifiable sources (charges, gravitational bodies, and so forth).A non-inertial reference frame is one accelerating with respect to an inertial one, and in such a non-inertial frame a particle is subject to acceleration by fictitious forces that enter the equations of motion solely as a result of its accelerated motion, and do not originate in identifiable sources. These fictitious forces are in addition to the real forces recognized in an inertial frame.A key concept of inertial frames is the method for identifying them. For practical purposes, reference frames that are un-accelerated with respect to the distant stars are regarded as good approximations to inertial frames.Forces; Newton's second lawNewton was the first to mathematically express the relationship between force and momentum . Some physicists interpret Newton's second law of motion as a definition of force and mass, while others consider it a fundamental postulate, a law of nature. Either interpretation has the same mathematical consequences, historically known as "Newton's Second Law":a m t v m t p F ===d )(d d dThe quantity m v is called the (canonical ) momentum . The net force on a particle is thus equal to rate of change of momentum of the particle with time.So long as the force acting on a particle is known, Newton's second law is sufficient to。

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High-visibility nonclassical interferenceof photon pairs generated ina multimode nonlinear waveguideMichałJachura,1∗MichałKarpi´nski,1,2Czesław Radzewicz,1andKonrad Banaszek11Faculty of Physics,University of Warsaw,Ho˙z a69,00-681Warsaw,Poland2Clarendon Laboratory,University of Oxford,Parks Road,Oxford OX13PU,UK∗jachur@Abstract:We report measurements of two-photon interference usinga cw-pumped type-II spontaneous parametric down-conversion sourcebased on a multimode perodically poled potassium titanyl phosphate(PPKTP)waveguide.We have used the recently demonstrated technique ofcontrolling the spatial characteristics of the down-conversion process viaintermodal dispersion to generate photon pairs in fundamental transversemodes,thus ensuring their spatial indistinguishability.Good overlap ofphoton modes within the pairs has been verified using the Hong-Ou-Mandelinterferometer and the preparation of polarization entanglement in theShih-Alley configuration,yielding visibilities consistently above90%.©2014Optical Society of AmericaOCIS codes:(270.0270)Quantum optics;(190.4390)Nonlinear optics,integrated optics;(230.7370)Waveguides.References and links1.J.L.O’Brien,A.Furusawa,and J.Vuˇc kovi´c,“Photonic quantum technologies,”Nat.Photon.3,687–695(2009).2.M.˙Zukowski,A.Zeilinger,M.A.Horne,and A.K.Ekert,“‘Event-ready-detectors’Bell experiment via entan-glement swapping,”Phys.Rev.Lett.71,4287-4290(1993).3. 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A.B.U’Ren,C.Silberhorn,K.Banaszek,and I.A.Walmsley,“Efficient conditional preparation of high-fidelitysingle photon states forfiber-optic quantum networks,”Phys.Rev.Lett.93,093601(2004).7.M.Fiorentino,S.M.Spillane,R.G.Beausoleil,T.D.Roberts,P.Battle,and M.W.Munro,“Spontaneousparametric down-conversion in periodically poled KTP waveguides and bulk crystals,”Opt.Express15,7479–7488(2007).8. 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B.Brecht,A.Eckstein,A.Christ,H.Suche,and C.Silberhorn,“From quantum pulse gate to quantum pulseshaper–engineered frequency conversion in nonlinear optical waveguides,”New.J.Phys.13,065029(2011). 14.M.Karpi´n ski,C.Radzewicz,and K.Banaszek,“Dispersion-based control of modal characteristics for parametricdown-conversion in a multimode waveguide,”Opt.Lett.37,878–880(2012).15.P.J.Mosley,A.Christ,A.Eckstein,and C.Silberhorn,“Direct measurement of the spatial-spectral structure ofwaveguided parametric down-conversion,”Phys.Rev.Lett.103,233901(2009).16.M.Karpi´n ski,C.Radzewicz,and K.Banaszek,“Generation of spatially pure photon pairs in a multimode nonlin-ear waveguide using intermodal dispersion,”Proc.SPIE8518,Quantum Communications and Quantum Imaging X,85180J(2012).17. C.K.Hong,Z.Y.Ou,and L.Mandel,“Measurement of subpicosecond time intervals between two photons byinterference,”Phys.Rev.Lett.59,2044–2046(1987).18.W.P.Grice,R.Erdmann,I.A.Walmsley,and D.Branning,“Spectral distinguishability in ultrafast parametricdown-conversion,”Phys.Rev.A57,R2289–R2292(1998).19.Y.H.Shih,and C.O.Alley,“New type of Einstein-Podolsky-Rosen-Bohm experiment using pairs of light quantaproduced by optical parametric down conversion,”Phys.Rev.Lett.61,2921–2924(1988).20.M.H.Rubin“Transverse correlation in optical spontaneous parametric down-conversion,”Phys.Rev.A54,5349–5360(1996).21.J.P.Torres,K.Banaszek,and I.A.Walmsley,“Engineering nonlinear optic sources of photonic entanglement,”Progress in Optics56,227–331(2011).22.T.Zhong,X.Hu,F.N.C.Wong,K.K.Berggen,T.D.Roberts,and P.Battle,“High-qualityfiber-optics polar-ization entanglement distribution at1.3µm telecom wavelength,”Opt.Lett.35,1392–1394(2010).23.H.Herrmann,X.Yang,A.Thomas,A.Poppe,W.Sohler,and C.Silberhorn,“Post-selection free,integratedoptical source of non-degenerate,polarization entangled photon pairs,”Opt.Express21,27981–27991(2013).24. F.Steinlechner,P.Trojek,M.Jofre,H.Weier,D.Perez,T.Jennewein,R.Ursin,J.Rarity,M.W.Mitchell,J.P.Torres,H.Weinfurter,and V.Pruneri,“A high-brightness source of polarization-entangled photons optimized for applications in free space,”Opt.Express20,9640–9649(2012).1.IntroductionMultiphoton interference is a nonclassical effect widely utilized in optical realizations of quantum-enhanced technologies[1]and testing foundations of quantum mechanics.High visi-bility of multiphoton interference depends critically on the absence of distinguishing informa-tion between the interfering photons[2].While early experiments relied on spatial and spectral filtering to fulfill this requirement,a great deal of effort is currently being expended on the development of sources that guarantee suitable characteristics of the collected photons already at the production stage.Such sources can offer substantially higher brightness,compatibility with integrated optics circuits,and strong photon number correlations,the last feature needed for example in device-independent quantum cryptography and randomness generation[3,4].A promising route to photon sources with well-defined,controllable characteristics is based on spontaneous parametric down-conversion inχ(2)nonlinear waveguides[5–10].Compared to bulk crystals,the phase matching conditions that define the nonlinear process in a waveg-uide assume a different form owing to the discreteness of transverse spatial modes propagating through the structure[11,12].This opens up new possibilities to engineer properties of the pro-duced nonclassical radiation[13].In particular,generation of spatially pure photon pairs in a multimode waveguide has been recently reported in[14],with a high degree of spatial coher-ence verified via a heralded photon counting measurement of the beam quality factors based on free-space diffraction.Single spatial modes for the generated photons were selected by ex-ploiting the effects of intermodal dispersion in the down-conversion process.This technique overcomes waveguide manufacturing limitations for shorter wavelengths.Prospectively,it can also be used to produce spatial photonic entanglement[15,16].In this paper,we study experimentally two-photon interference using a periodically poled potassium titanyl phosphate(PPKTP)waveguide source of spatially pure photon pairs that #205051 - $15.00 USD Received 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014 (C) 2014 OSA7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8625Measurements performed in two configuration [18]and a visibilities consistently exceeding any spatial filtering of the generated These results provide a compelling generated photons,paving the waytowards employing them in more complex multiphoton interference experiments.This paper is organized as follows.First,in Sec.2we briefly review parametric down-conversion in a nonlinear multimode waveguide and discuss operating conditions that ensure generation of indistinguishable photon pairs.Next,Sec.3describes the experimental setup and alignment procedures.Results of two-photon interference measurements are presented and dis-cussed in Sec.4.Finally,Sec.5concludes the paper.2.MethodWe begin by reviewing the technique to control the spatial characteristics of photon pairs gen-erated in a multimode nonlinear waveguide and discussing the operation of the source that ensures high-visibility two-photon interference.The waveguide is chosen to realize a type-II down-conversion process in which a pump photon P is converted into a pair of orthogonally polarized photons H and V .The basic object in our analysis is the phase matching function,which in the quantum picture of parametric down-conversion is interpreted as the probability amplitude that a pair of photons with wavelengths λH and λV will be generated from a pump photon with the wavelength defined by energy conservation.While in a bulk medium the phase matching function depends also on continuous spatial degrees of freedom of the photons taking part in the process,parameterized for example with transverse wave vectors [20],in the case of a multimode waveguide the function depends on the specific triplet of spatial modes of the photons P ,H ,and V involved in the process.Fig.1.(a)Numerical simulations of phase matching for spontaneous parametric down-conversion in a 1mm long PPKTP waveguide analogous to the structure used in the ex-periment,with the pump field prepared in the fundamental spatial mode of the waveguide.Separate phase matching bands correspond to different combinations of the spatial modesof H and V photons.The energy conservation condition is depicted with a solid white line.(b)The joint and marginal spectra of the generated photon pairs.Application of coarsespectral filtering represented by dashed lines allows one to select the spectral region whereboth the photons are generated in the fundamental waveguide modes 00H and 00V .As illustrated in Fig.1(a),intermodal dispersion between waveguide modes makes the phase #205051 - $15.00 USDReceived 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014(C) 2014 OSA 7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8626matching condition satisfied in general at different regions of the plane spanned by the wave-lengthsλH andλV,resulting in a series of bands whose width is inversely proportional to the waveguide length.In particular,if the pump is prepared in the fundamental waveguide mode 00P,then the phase matching function for generating down-converted photons in fundamental modes00H and00V is separated from processes involving higher-order H and/or V modes, provided that the waveguide is long enough to sufficiently narrow the relevant bands.This condition is satisfied for the1mm long structure in our experiment,which was simulated in Fig.1(a).It needs to be stressed that this scheme relies critically on the pump beam prepared in the fundamental spatial mode:coupling the pump into modes other than00P generates contri-butions from phase matching bands involving higher-order spatial modes for H and V photons that overlap spectrally with the desired00P→00H+00V band.If a cw pump is employed to induce the down-conversion process,the wavelengths of the down-converted photons must satisfy the constraint of constant total energy,which is symmet-ric with respect to swappingλH andλV and for the wavelength range depicted in Fig.1(a) becomes a nearly straight line running in the antidiagonal direction with respect to the graph axes.In contrast,the slope of the phase matching bands is noticeably different,as the H and V photons are generated in the type-II process and they propagate as extraordinary and ordinary rays.Consequently,pairs of photons are produced for combinations of wavelengths that form a set of islands,shown in Fig.1(b),located at crossings of the energy conservation line with phase matching bands.The island corresponding to the process00P→00H+00V can be sepa-rated from other processes by coarse spectralfiltering of one or both of the generated photons. It is worth noting that overlap may occur between islands corresponding to generation of pho-ton pairs in higher-order spatial modes owing to approximate degeneracy with respect to their propagation constants.While the above scheme ensures generation of photons in fundamental spatial modes,two-photon interference requires also spectral indistinguishability within the produced pairs.This condition is not satisfied automatically,as the separation between the spectra of the H and V photons will vary with the wavelength of the pump photons,which shifts the energy conserva-tion line in the diagonal direction of Fig.1(a).However,the graph indicates that for a suitable pump wavelength the regime of spectral degeneracy should be achievable.Because our numer-ical simulation of the waveguide is sensitive to details of the actual refractive index profile,this regime of operation needs to be identified by experimental means.We found that a suitable procedure,described in detail in Sec.3,was to measure the individual photon spectra in the heralded regime and to carefully tune the pump wavelength until the spectral profiles of H and V photons were matched within the resolution of the measuring apparatus.3.Experimental setupThe waveguide source of photon pairs used in our experiments is shown schematically in Fig.2. Its heart was a1mm long PPKTP structure(AdvR Inc.)temperature stabilized at19.0±0.1◦C using a thermoelectric cooler.A series of waveguides localized just beneath the surface had lateral transverse dimensions of approx.2µm,effective depths of approx.5µm,and poling periods designed for efficient type-II second harmonic generation in the800nm wavelength region.At these wavelengths the waveguides supported at least8transverse spatial modes(4 for each polarization).The structure was placed between two infinity corrected50×microscope objectives with numerical apertures NA=0.55for incoupling and NA=0.8for outcoupling.A magnified image of the waveguide illuminated with incoherent white light along with measured spatial profiles of the fundamental pump,H,and V modes at their respective wavelengths is shown in Fig.3.The down-conversion process was pumped by a narrowband(linewidth<0.0011nm)cw #205051 - $15.00 USD Received 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014 (C) 2014 OSA7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8627Fig.2.The PPKTP waveguide source of photon pairs and setups for(a)characterization ofphoton spectra,(b)measurement of two-photon interference,and(c)preparation of polar-ization entanglement in Shih-Alley configuration.λ/2,half-wave plate;POL,Glan-Taylorpolarizer;IF,interferencefilter;DM,dichroic mirror;PBS,polarizing beam splitter;MMF,multimodefiber;SMF,single modefiber;SPCM,single photon counting module;BSC,Babinet-Soleil compensator;BS,non-polarizing beam splitter,NDF,neutral densityfilter;CF,colorfilter.diode laser(Toptica BlueTune)beam that could be tuned around the central wavelength of 400nm.The pump beam was delivered to the setup with a single-modefiber.The pump power and polarization were controlled using a Glan-Taylor polarizer placed between two half-wave plates.Typical pump power incident on the waveguide input facet was53µW,whereas the pump power coupled into the waveguide is estimated to be at least29µW.The estimate is based on the power measured at the exit of the waveguide,assuming no propagation losses. This corresponds to coupling efficiency of at least55%,which is similar to the values reported in other experiments[9,22].Thisfigure could be improved by approx.8%by using a waveg-uide sample with anti-reflection coated facets.As preparing the pumpfield in the fundamental transverse waveguide mode was crucial for the spatial purity of the generated photons,after the outcoupling objective the remainder of the pump beam was directed with a dichroic mirror to a CCD camera.Its purpose was to monitor the quality of the pump spatial mode through a comparison with a reference profile generated beforehand in the sum-frequency process[14]. An exemplary image of the pump beam mode is shown in Fig.3(b).Although the waveguide cross section is elongated and asymmetric in the vertical direction,the fundamental pump beam mode,being well-confined within the structure,bears only a minor signature of this asymme-try.This enabled us to excite selectively the fundamental pump mode by direct coupling a laser beam spatiallyfiltered by a single modefiber and focused to an appropriate diameter with the microscope objective.An auxiliary infrared beam from a modelocked Ti:sapphire laser,coupled predominantly into the fundamental spatial mode of the waveguide at the down-conversion wavelength,was used to identify the waveguide with a suitable poling period and to align optical elements following the source.The profiles of H and V fundamental modes presented in Fig.3(c,d)were recorded with the help of this beam.In order to verify the spectral indistinguishability of the generated photon pairs,in thefirst step we measured individual spectra of heralded photons using the setup depicted in Fig.2(a). Photon pairs were sent through a colorfilter(cut-off wavelength660nm)and separated on a polarizing beam splitter.The output paths for the photons could be swapped with the help of a half-wave plate placed before the polarizing beam splitter.At the output,one photon was used #205051 - $15.00 USD Received 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014 (C) 2014 OSA7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8628Fig.3.The image of the output facet of the PPKTP waveguide illuminated with spatiallyincoherent white light(a)and transverse profiles of the fundamental P mode excited withthe pump laser(b)as well as the fundamental H mode(c)and V mode(d)excited with theauxiliary Ti:sapphire laser beam.The intensity distributions were obtained by imaging theoutput facet of the waveguide onto a CCD camera using the outcoupling objective and a200mm focal length lens.as a herald,while the second one was transmitted through a0.7nm full width at half max-imum(FWHM)interferencefilter mounted on a motorized rotation stage.The photons were subsequently coupled using11mm focal length aspheric lenses into100µm core diameter, 0.22NA multimodefibers connected to single photon counting modules(Perkin Elmer SPCM-AQRH-14-FC).Coincidence events were counted within a3ns window.The rotation angle of the interferencefilter was calibrated in terms of the transmitted central wavelength using a Ti:sapphire beam and a spectrometer.Fig.4.Heralded spectra of individual photons measured by rotating a0.7nm FWHM band-passfilter.Coincidence count rates(points,left scale)collected over5s intervals arefittedwith Gaussian functions(solid lines)assuming Poissonian errors.Experimentally obtainedspectral profiles of the interferencefilters used in measurements of two-photon interfer-ence:11nm,dashed-dotted line;3nm,dotted line(right scale).PPKTP phase matching properties make the spectral characteristics of the generated photons strongly dependent on the pump wavelength,as can be inferred from Fig.1(a).Using the over-lap of the single photon spectra as the optimization criterion,wefine-tuned the wavelength of the pump laser,obtaining the best match at400.63nm,shown in Fig.4.In the same graph, #205051 - $15.00 USD Received 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014 (C) 2014 OSA7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8629two interference filters used in measurements 4.The FWHM widths of the filters are approxi-the entire spectra of photons generated Fig.1(b),its principal role in the setup is to cut spatial modes that occur in distinct frequency regions [14,16].4.Two-photon interferenceWe have tested nonclassical interference between photons generated in the waveguide using two setups.The first one was the Hong-Ou-Mandel interferometer [17]in the common-path configuration [18]depicted in Fig.2(b).In this case,a pair of orthogonally polarized photons was rotated with a half-wave plate by 45◦and sent to a polarizing beam splitter.The time delay between the photons was adjusted using a Babinet-Soleil compensator.Zero delay was found by measuring spectral fringes with help of the Ti:sapphire beam.Photons leaving the polarizing beam splitter were coupled into multimode fibers and counted using the same configuration as before.In Fig.5we show measured coincidence rates as functions of the time delay.The depth of the Hong-Ou-Mandel dip with respect to the reference level of fully distinguishable particles,determined from Gaussian fits,is V =91.1±0.5%for 11nm filter and V =93.1±1.2%for 3nm filter.These figures confirm that the photons are highly indistinguishable in both the spectral and the spatial degrees of freedom.It is seen that the coincidence count rate is minimized for a non-zero delay of −0.08ps,which compensates the temporal walk-off within photon pairs due to waveguide birefringence.Fig.5.Coincidence count rates (points)determined over 5s intervals measured in thecommon-path Hong-Ou-Mandel interferometer as a function of the time delay for (a)11nmand (b)3nm interference filters placed at the interferometer entrance.Solid lines depictGaussian fits assuming Poissonian errors for experimental points.The second test of two-photon interference was carried out through preparation of polar-ization entanglement in the Shih-Alley configuration [19].In this setup,shown in Fig.2(c),two photons in orthogonal horizontal (H )and vertical (V )polarizations impinge on a non-polarizing beam splitter at a nearly normal incidence.Their polarizations are analyzed at the outputs using half-wave plates and polarizers.When the two photons emerge at different ports of the beam splitter,their postselected polarization state takes the maximally entangled form |HV +|V H /√2.The presence of entanglement can be verified by detecting photons in linear polarization bases.Specifically,if one of the photons is detected at 45◦,the coincidence #205051 - $15.00 USDReceived 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014(C) 2014 OSA 7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8630proportional to(1)be shown[21]that for tempo-to the depth of the Hong-Ou-Fig.6.Coincidence count rates measured over5s intervals as a function of the angleθofthe collected linear polarization,when conjugate photons were detected in horizontal(H),vertical(V),diagonal(D),and antidiagonal(A)polarizations,shown for(a)11nm and(b)3nm interferencefilters placed at the setup entrance.Before measuring polarization fringes,the Babinet-Soleil compensator placed before the non-polarizing beam splitter was set to the position that minimized the coincidence rate in the Hong-Ou-Mandel interferometer.In Fig.6we present coincidence count rates between one photon projected onto horizontal(H),vertical(V),diagonal(D),or antidiagonal(A)polariza-tion and the second photon detected in linear polarization at an angleθ.Visibilities determined from sinusoidalfits to interference fringes are collected in Tab.1.Fringe visibilities for diagonal and antidiagonal polarizations match within their uncertainties the depths of Hong-Ou-Mandel dips.Table1.Visibilities of polarization fringes obtained from measurements for multimode(MMF)and single mode(SMF)fibers in the setup for polarization entanglement prepa-ration.Absolute uncertainties of presented values are approximately1%.The last columnspecifies the source brightness for each combination of the interferencefilters and couplingfibers.Coupling Interference Fringe visibility Source brightnessfiberfilter H V D A105pairs/s/mWMMF11nm93.9%94.0%92.8%90.9% 1.463nm94.4%96.2%93.0%93.3%0.76 SMF11nm96.3%96.8%95.7%95.9% 1.283nm98.1%97.4%97.9%98.6%0.62 In order to estimate the effects of nonideal spatial overlap of the interfering photons,we repeated the measurements of polarization correlations using single modefibers to deliver pho-#205051 - $15.00 USD Received 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014 (C) 2014 OSA7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8631tons to detectors.Fringe visibilities determined from these data are also presented in Tab.1.It is seen that for measurements in the diagonal basis,fringe visibilities increased by approximately by5%.This can be mainly attributed to transverse walk-off of orthogonally polarized photons in the Babinet-Soleil compensator,a minor discrepancy between fundamental waveguide mode profiles for orthogonal polarizations that can be noticed in Fig.3(c,d),and contributions from down-conversion processes involving residually excited higher-order pump modes.The brightness of the source defined as the ratio of detected photon pairs to the pump power coupled into the waveguide is specified in the last column of Tab.1.Typical ratio of coinci-dence to single count rates in our experiments was8.9%for the11nmfilter.Although standard optical elements were antireflection-coated,contributions to non-unit transmission came from the waveguide-air interface(≈92%),outcoupling objective(≈76%),Soleil-Babinet compen-sator(≈75%),interferencefilter(≈77%),coupling into multimodefibers(≈85%)are further combined with the non-unit detector efficiency(≈45%).Other relevant effects could include intra-waveguide losses and additional parasitic down-conversion processes.It is worthwhile to note substantial improvement of indistinguishability compared to pio-neering experiments with the PPKTP nonlinear medium[7].Recently,visibilities exceeding 95%have been reported for two-photon interference experiments based on waveguide sources at1.3µm and1.5µm telecom bands[22,23],where difficulties to manufacture single-mode structures are less severe.In the800nm wavelength region,the brightness6.4×105pairs/s/mW and the average visibility above97%for photonsfiltered through a single-modefiber have been achieved in[24],where a pair of two crossed20mm long bulk PPKTP crystals was used to realize a type-0down-conversion process.5.ConclusionsWe studied experimentally distinguishability of photons generated via spontaneous paramet-ric down-conversion in a multimode nonlinear PPKTP waveguide.Measurements taken in two different setups implementing two-photon interference yielded visibilities robustly above90% without resorting to spatialfiltering.This directly demonstrates that photon sources based on exploiting intermodal dispersion in multimode structures,a key technique used in our setup,are suitable for multiphoton interference experiments.The benefits of waveguide sources in pho-tonic quantum technologies,such as high brightness and integrability,can be therefore extended also to spectral regions where single-mode structures are not readily available. AcknowledgmentsWe thank R.Demkowicz-Dobrza´n ski,P.Michelberger,K.Thyagarajan,and W.Wasilewski for insightful discussions.This work was supported by the Polish NCBiR under the ERA-NET CHIST-ERA project QUASAR and the Foundation for Polish Science TEAM project cofinanced by the EU European Regional Development Fund.#205051 - $15.00 USD Received 20 Jan 2014; revised 11 Mar 2014; accepted 11 Mar 2014; published 3 Apr 2014 (C) 2014 OSA7 April 2014 | Vol. 22, No. 7 | DOI:10.1364/OE.22.008624 | OPTICS EXPRESS 8632。

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