2024
2024
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Record 49 of
Title:Evaporation characteristics of Er3+-doped silica fiber and its application in the preparation of whispering gallery mode lasers
Author Full Names:Li, Angzhen(1); Ward, Jonathan M.(2); Tian, Ke(3,4); Yu, Jibo(5); She, Shengfei(6); Hou, Chaoqi(6); Guo, Haitao(6); Chormaic, Síle Nic(4,7); Wang, Pengfei(3)Source Title:Optics ExpressLanguage:EnglishDocument Type:Journal article (JA)Abstract:In this work, the concentration of rare-earth ions in doped silica whispering gallery lasers (WGLs) is controlled by evaporation. The fabrication of WGLs is used to experimentally evaluate the evaporation rate (mol/μm) and ratio (mol/mol) of erbium and silica lost from a doped fiber during heating. Fixed lengths of doped silica fiber are spliced to different lengths of undoped fiber and then evaporated by feeding into the focus of a CO2 laser. During evaporation, erbium ions are precipitated in the doped silica fiber to control the erbium concentration in the remaining SiO2, which is melted into a microsphere. By increasing the length of the undoped section, a critical point is reached where effectively no ions remain in the glass microsphere. The critical point is found using the spectra of the whispering gallery modes in microspheres with equal sizes. From the critical point, it is estimated that, for a given CO2 laser power, 6.36 × 10?21 mol of Er3+ is lost during the evaporation process for every cubic micron of silica fiber. This is equivalent to 1.74 × 10?7 mol of Er3+ lost per mol of SiO2 evaporated. This result facilitates the control of the doping concentration in WGLs and provides insight into the kinetics of laser-induced evaporation of doped silica. ? 2024 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement.Affiliations:(1) Tianjin Key Laboratory of Quantum Optics and Intelligent Photonics, School of Science, Tianjin University of Technology, Tianjin; 300384, China; (2) Physics Department, University College Cork, Cork, Ireland; (3) Key Laboratory of In-Fiber Integrated Optics of Ministry of Education, College of Science, Harbin Engineering University, Harbin; 150001, China; (4) Light-Matter Interactions for Quantum Technologies Unit, Okinawa Institute of Science and Technology Graduate University, Okinawa, Onna; 904-0495, Japan; (5) Xi’an Institute of Applied Optics, Xi’an; 710065, China; (6) State Key Laboratory of Transient Optics and Photonics, Xi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi’an; 710119, China; (7) Institute of Physics, Technische Universit?t Chemnitz, Chemnitz; D-09107, GermanyPublication Year:2024Volume:32Issue:3Start Page:3912-3921DOI Link:10.1364/OE.509662數(shù)據(jù)庫ID（收錄號）:20240615502598 -
Record 50 of
Title:Switchable Pancharatnam–Berry Phases in Heterogeneously Integrated THz Metasurfaces
Author Full Names:Dong, Bowen(1,2); Zhu, Shuangqi(1); Guo, Guanxuan(3); Wu, Tong(3); Lu, Xueguang(4); Huang, Wanxia(4); Ma, Hua(5); Xu, Quan(3); Han, Jiaguang(3,6); Zhang, Shuang(7); Wang, Yongtian(1); Zhang, Xueqian(3); Huang, Lingling(1)Source Title:Advanced MaterialsLanguage:EnglishDocument Type:Article in PressAbstract:The Pancharatnam–Berry (PB) phase has revolutionized the design of metasurfaces, offering a straightforward and robust method for controlling wavefronts of electromagnetic waves. However, traditional metasurfaces have fixed PB phases determined by the orientation of their individual elements. In this study, an innovative structural design and integration scheme is proposed that utilizes vanadium dioxide, a phase-change material, to achieve thermally controlled dynamic PB phase control within the metasurface. By leveraging the material's properties, this can dynamically alter the optical orientation of individual elements of the metasurface and achieve temperature-dependent local phase modulation based on the geometric phase principle. This approach, combined with advanced fabrication processing technology, paves the way for next-generation dynamic devices with customizable functions. ? 2024 Wiley-VCH GmbH.Affiliations:(1) School of Optics and Photonics, Beijing Engineering Research Center of Mixed Reality and Advanced Display, Beijing Institute of Technology, Beijing; 100081, China; (2) National Innovation Institute of Defense Technology, Academy of Military Sciences, Beijing; 100071, China; (3) Center for Terahertz waves and College of Precision Instrument and Optoelectronics Engineering, Tianjin University and the Key Laboratory of Optoelectronics Information and Technology (Ministry of Education), Tianjin; 300072, China; (4) College of Materials Science and Engineering, Sichuan University, Chengdu; 610065, China; (5) Department of Basic Sciences, Air Force Engineering University, Xian; 710038, China; (6) Guangxi Key Laboratory of Optoelectronic Information Processing, School of Optoelectronic Engineering, Guilin University of Electronic Technology, Guilin; 541004, China; (7) New Cornerstone Science Laboratory, Department of Physics, University of Hong Kong, 999077, Hong KongPublication Year:2024DOI Link:10.1002/adma.202417183數(shù)據(jù)庫ID（收錄號）:20245117545544 -
Record 51 of
Title:Scalable parallel ultrafast optical random bit generation based on a single chaotic microcomb
Author Full Names:Li, Pu(1,2,3); Li, Qizhi(4); Tang, Wenye(4); Wang, Weiqiang(5); Zhang, Wenfu(5); Little, Brent E.(5); Chu, Sai Tek(6); Shore, K. Alan(7); Qin, Yuwen(1,2,3); Wang, Yuncai(1,2,3)Source Title:Light: Science and ApplicationsLanguage:EnglishDocument Type:Journal article (JA)Abstract:Random bit generators are critical for information security, cryptography, stochastic modeling, and simulations. Speed and scalability are key challenges faced by current physical random bit generation. Herein, we propose a massively parallel scheme for ultrafast random bit generation towards rates of order 100 terabit per second based on a single micro-ring resonator. A modulation-instability-driven chaotic comb in a micro-ring resonator enables the simultaneous generation of hundreds of independent and unbiased random bit streams. A proof-of-concept experiment demonstrates that using our method, random bit streams beyond 2 terabit per second can be successfully generated with only 7 comb lines. This bit rate can be easily enhanced by further increasing the number of comb lines used. Our approach provides a chip-scale solution to random bit generation for secure communication and high-performance computation, and offers superhigh speed and large scalability. ? The Author(s) 2024.Affiliations:(1) Institute of Advanced Photonics Technology, School of Information Engineering, Guangdong University of Technology, Guangzhou; 51006, China; (2) Key Laboratory of Photonic Technology for Integrated Sensing and Communication, Ministry of Education of China, Guangdong University of Technology, Guangzhou; 51006, China; (3) Guangdong Provincial Key Laboratory of Information Photonics Technology, Guangdong University of Technology, Guangzhou; 51006, China; (4) Key Laboratory of Advanced Transducers and Intelligent Control System, Ministry of Education, Taiyuan University of Technology, Taiyuan; 030024, China; (5) State Key Laboratory of Transient Optics and Photonics, Xi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi’an; 710119, China; (6) Department of Physics and Materials Science, City University of Hong Kong, Hong Kong; (7) School of Electronic Engineering, Bangor University, Wales, Bangor; LL57 1UT, United KingdomPublication Year:2024Volume:13Issue:1Article Number:66DOI Link:10.1038/s41377-024-01411-7數(shù)據(jù)庫ID（收錄號）:20241015704601 -
Record 52 of
Title:Polarization-Based Enhancement for Oceanic Constituents and Inherent Optical Properties (Iops) Retrieval from Multi-Angular Polarimetric Measurements Over Global Oceans
Author Full Names:Liu, Jia(1,2,3,4); Li, Chunxia(5); He, Xianqiang(3); Chen, Tieqiao(2); Jia, Xinyin(2); Bai, Yan(3); Liu, Dong(6); Liu, Yupeng(1); Yang, Wentao(7); Wang, Yihao(2); Zhang, Geng(2); Li, Siyuan(2); Hu, Bingliang(2); Pan, Delu(3)Source Title:SSRNLanguage:EnglishDocument Type:Preprint (PP)Abstract:Multi-angle polarization characteristics of water-leaving radiation, which contain rich information on oceanic constituents and inherent optical properties (IOPs), have often been neglected. In this study, global radiative transfer (RT) simulations for the polarization characteristics of water-leaving radiance (Lw) were performed using the vector radiative transfer model for a coupled ocean-atmosphere system (PCOART). And, a global polarization-based algorithm for retrieving oceanic constituents and inherent optical properties (IOPs) was developed, employing the Fully Connected U-Net (FCUN). The retrieval performance of the algorithm was then analyzed using in-situ measurements collected during the Qiandao Lake field campaign. Results indicated that the low degrees of polarization (DOP) at short blue bands at solar zenith angle of 0° predominantly occurred in the tropical and subtropical oceans, with the lowest DOP value of 0.0176 observed in the extra oligotrophic subtropical gyres. The global mean absolute percentage error (MAPE) of the FCUN predictions compared to RT simulations for oceanic constituents (Chla, ag(443), NAP) and IOPs (a, b, aph, bph, aNAP, bNAP, bb, bbph, bbNAP) at 443 nm were 6.24%, 3.90%, 10.65%, 2.85%, 3.15%, 3.79%, 4.42%, 3.90%, 3.90%, 3.13%, 4.44%, and 3.90%, respectively, with mean global MAPE values of 4.52%. Additionally, the FCUN model’s predictions were consistent with RT simulation inputs under various random instrument noise conditions, with mean global MAPE values of 6.74% and 8.84% for those 12 retrieved parameters, respectively. Moreover, the retrieval performance analysis of FCUN on the in-situ measurements was performed with MAPE for Chla, a, aph, bb at 443 nm of 31.80%, 29.65%, 34.87%, and 43.04%, respectively. The importance of multi-angles polarization observations of Lw for ocean constituents and IOPs retrieval were also examined with the global mean MAPE decreasing from 16.91% to 1.48% as the observation angles increasing. Overall, the global polarization-based inversion model exhibited substantial potential for the oceanic constituents and IOPs retrieval of using multi-angle polarimetry. ? 2024, The Authors. All rights reserved.Affiliations:(1) State Key Laboratory of Tropical Oceanography, South China Sea Institute of Oceanology, Chinese Academy of Sciences, Guangzhou; 510301, China; (2) Key Laboratory of Spectral Imaging Technology of CAS, Xi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi’an; 710119, China; (3) State Key Laboratory of Satellite Ocean Environment Dynamics, Second Institute of Oceanography, Ministry of Natural Resources, Hangzhou; 310012, China; (4) University of Chinese Academy of Sciences, Beijing; 100049, China; (5) School of Human Settlements and Civil Engineering, Xi’an Jiaotong University, Xi’an; 710049, China; (6) Key Laboratory of Watershed Geographic Sciences, Nanjing Institute of Geography and Limnology, Chinese Academy of Sciences, Nanjing; 210008, China; (7) National-local Joint Engineering Laboratory of Geospatial Information Technology, Hunan University of Science and Technology, Xiangtan; 411201, ChinaPublication Year:2024DOI Link:10.2139/ssrn.4803997數(shù)據(jù)庫ID（收錄號）:20240169237 -
Record 53 of
Title:Dark gap soliton families in coupled nonlinear Schr?dinger equations with linear lattices
Author Full Names:Chen, Junbo(1); Mihalache, Dumitru(2); Beli?, Milivoj R.(3); Qin, Wenqiang(4,5,6); Zhu, Danfeng(1); Zhu, Xing(7); Zeng, Liangwei(7)Source Title:Nonlinear DynamicsLanguage:EnglishDocument Type:Article in PressAbstract:We demonstrate that two types of dark gap soliton families, the fundamental dark solitons and the dark soliton clusters, can be stabilized in coupled nonlinear Schr?dinger equations (NLSEs) with linear lattices. Two types of coupled NLSEs are investigated, those with identical lattices and those with different lattices. In the latter case, one component features a monochromatic linear lattice, while the other features a bichromatic linear lattice. For coupled NLSEs with the same lattices, the soliton profiles are nearly identical, with both components exhibiting monochromatic backgrounds. In contrast, for coupled NLSEs with different lattices, the profiles differ significantly: one component has a monochromatic background, while the other has a bichromatic background. The stability domains of these dark soliton families are determined by the method of linear stability analysis, and also confirmed by direct numerical simulations. ? The Author(s), under exclusive licence to Springer Nature B.V. 2024.Affiliations:(1) School of Physics and Electronic Engineering, Jiaying University, Meizhou; 514015, China; (2) Horia Hulubei National Institute of Physics and Nuclear Engineering, Magurele, Bucharest; 077125, Romania; (3) College of Sciences and Engineering, Hamad Bin Khalifa University, Doha; 23874, Qatar; (4) Key Laboratory for Physical Electronics and Devices of the Ministry of Education, Shaanxi Key Lab of Information Photonic Technique, School of Electronic Science and Engineering, Xi’an Jiaotong University, Xi’an; 710049, China; (5) Key Laboratory of Ultra-fast Photoelectric Diagnostics Technology of CAS, Xi’an Institute of Optics and Precision Mechanics of Chinese Academy of Sciences, Xi’an; 710119, China; (6) University of Chinese Academy of Sciences, Beijing; 100049, China; (7) School of Arts and Sciences, Guangzhou Maritime University, Guangzhou; 510725, ChinaPublication Year:2024Article Number:213001DOI Link:10.1007/s11071-024-10788-4數(shù)據(jù)庫ID（收錄號）:20245217571754 -
Record 54 of
Title:Enhancing the spatial resolution of time-of-flight based non-line-of-sight imaging via instrument response function deconvolution
Author Full Names:Wang, Dingjie(1,2); Hao, Wei(1,3,4); Tian, Yuyuan(1,2); Xu, Weihao(1,2); Tian, Yuan(1,2); Cheng, Haihao(2,5); Chen, Songmao(1,3,4); Zhang, Ning(6); Zhu, Wen Hua(7); Su, Xiuqin(1,3,4)Source Title:Optics ExpressLanguage:EnglishDocument Type:Journal article (JA)Abstract:Non-line-of-sight (NLOS) imaging retrieves the hidden scenes by utilizing the signals indirectly reflected by the relay wall. Benefiting from the picosecond-level timing accuracy, time-correlated single photon counting (TCSPC) based NLOS imaging can achieve theoretical spatial resolutions up to millimeter level. However, in practical applications, the total temporal resolution (also known as total time jitter, TTJ) of most current TCSPC systems exceeds hundreds of picoseconds due to the combined effects of multiple electronic devices, which restricts the underlying spatial resolution of NLOS imaging. In this paper, an instrument response function deconvolution (IRF-DC) method is proposed to overcome the constraints of a TCSPC system s TTJ on the spatial resolution of NLOS imaging. Specifically, we model the transient measurements as Poisson convolution process with the normalized IRF as convolution kernel, and solve the inverse problem with iterative deconvolution algorithm, which significantly improves the spatial resolution of NLOS imaging after reconstruction. Numerical simulations show that the IRF-DC facilitates light-cone transform and frequency-wavenumber migration solver to achieve successful reconstruction even when the system s TTJ reaches 1200 ps, which is equivalent to what was previously possible when TTJ was about 200 ps. In addition, the IRF-DC produces satisfactory reconstruction outcomes when the signal-To-noise ratio (SNR) is low. Furthermore, the effectiveness of the proposed method has also been experimentally verified. The proposed IRF-DC method is highly applicable and efficient, which may promote the development of high-resolution NLOS imaging. ? 2024 Optica Publishing Group (formerly OSA). All rights reserved.Affiliations:(1) Key Laboratory of Space Precision Measurement Technology, Xi an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi an; 710719, China; (2) University of Chinese Academy of Science, Beijing; 100049, China; (3) Center for Shared Technologies and Facilities, Xi an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi an; 710119, China; (4) Pilot National Laboratory for Marine Science and Technology (Qingdao), Qingdao; 266237, China; (5) State Key Laboratory of Transient Optics and Photonics, Xi an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi an; 710119, China; (6) Key Laboratory of Spectral Imaging Technology, Xi an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi an; 710119, China; (7) School of Electronic and Information Engineering, Jiujiang University, Jiujiang; 332005, ChinaPublication Year:2024Volume:32Issue:7Start Page:12303-12317DOI Link:10.1364/OE.518767數(shù)據(jù)庫ID（收錄號）:20241415837517 -
Record 55 of
Title:200 mm optical synthetic aperture imaging over 120 meters distance via macroscopic Fourier ptychography
Author Full Names:Zhang, Qi(1,2,3); Lu, Yuran(4); Guo, Yinghui(1,2,3,5,6); Shang, Yingjie(1,2,3,5); Pu, Mingbo(1,2,3,5); Fan, Yulong(1,2,3); Zhou, Rui(4); Li, Xiaoyin(1,2,3); Pan, An(7); Zhang, Fei(1,2,3); Xu, Mingfeng(1,2,3); Luo, Xiangang(1,2,3,5)Source Title:Optics ExpressLanguage:EnglishDocument Type:Journal article (JA)Abstract:Fourier ptychography (FP) imaging, drawing on the idea of synthetic aperture, has been demonstrated as a potential approach for remote sub-diffraction-limited imaging. Nevertheless, the farthest imaging distance is still limited to around 10 m, even though there has been a significant improvement in macroscopic FP. The most severe issue in increasing the imaging distance is the field of view (FoV) limitation caused by far-field conditions for diffraction. Here, we propose to modify the Fourier far-field condition for rough reflective objects, aiming to overcome the small FoV limitation by using a divergent beam to illuminate objects. A joint optimization of pupil function and target image is utilized to attain the aberration-free image while estimating the pupil function simultaneously. Benefiting from the optimized reconstruction algorithm, which effectively expands the camera’s effective aperture, we experimentally implement several FP systems suited for imaging distances of 12 m, 65 m, and 120 m with the maximum synthetic aperture of 200 mm. The maximum synthetic aperture is thus improved by more than one order of magnitude of the state-of-the-art works from the furthest distance, with an over fourfold improvement in the resolution compared to a single aperture. Our findings demonstrate significant potential for advancing the field of macroscopic FP, propelling it into a new stage of development. ? 2024 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement.Affiliations:(1) National Key Laboratory of Optical Field Manipulation Science and Technology, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu; 610209, China; (2) State Key Laboratory of Optical Technologies on Nano-Fabrication and Micro-Engineering, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu; 610209, China; (3) Research Center on Vector Optical Fields, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu; 610209, China; (4) Tianfu Xinglong Lake Laboratory, Chengdu; 610299, China; (5) College of Materials Sciences and Opto-Electronic Technology, University of Chinese Academy of Sciences, Beijing; 100049, China; (6) Sichuan Provincial Engineering Research Center of Digital Materials, Chengdu; 610299, China; (7) State Key Laboratory of Transient Optics and Photonics, Xi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi’an; 710119, ChinaPublication Year:2024Volume:32Issue:25Start Page:44252-44264DOI Link:10.1364/OE.533063數(shù)據(jù)庫ID（收錄號）:20244917491979 -
Record 56 of
Title:PneumoLLM: Harnessing the power of large language model for pneumoconiosis diagnosis
Author Full Names:Song, Meiyue(1,2); Wang, Jiarui(3); Yu, Zhihua(4); Wang, Jiaxin(5); Yang, Le(6); Lu, Yuting(3); Li, Baicun(7); Wang, Xue(8,9); Wang, Xiaoxu(3); Huang, Qinghua(10); Li, Zhijun(11,12); Kanellakis, Nikolaos I.(13,14,15); Liu, Jiangfeng(1,16,17); Wang, Jing(1,2); Wang, Binglu(3); Yang, Juntao(1,16,17)Source Title:Medical Image AnalysisLanguage:EnglishDocument Type:Journal article (JA)Abstract:The conventional pretraining-and-finetuning paradigm, while effective for common diseases with ample data, faces challenges in diagnosing data-scarce occupational diseases like pneumoconiosis. Recently, large language models (LLMs) have exhibits unprecedented ability when conducting multiple tasks in dialogue, bringing opportunities to diagnosis. A common strategy might involve using adapter layers for vision–language alignment and diagnosis in a dialogic manner. Yet, this approach often requires optimization of extensive learnable parameters in the text branch and the dialogue head, potentially diminishing the LLMs’ efficacy, especially with limited training data. In our work, we innovate by eliminating the text branch and substituting the dialogue head with a classification head. This approach presents a more effective method for harnessing LLMs in diagnosis with fewer learnable parameters. Furthermore, to balance the retention of detailed image information with progression towards accurate diagnosis, we introduce the contextual multi-token engine. This engine is specialized in adaptively generating diagnostic tokens. Additionally, we propose the information emitter module, which unidirectionally emits information from image tokens to diagnosis tokens. Comprehensive experiments validate the superiority of our methods. ? 2024 Elsevier B.V.Affiliations:(1) Institute of Basic Medical Sciences Chinese Academy of Medical Sciences, School of Basic Medicine Peking Union Medical College, Beijing; 100005, China; (2) State Key Laboratory of Respiratory Health and Multimorbidity, Beijing; 100005, China; (3) School of Automation, Northwestern Polytechnical University, Shaanxi, Xi'an; 710072, China; (4) Jinneng Holding Coal Industry Group Co. Ltd Occupational Disease Precaution Clinic, Shanxi; 037001, China; (5) School of Medicine, Tsinghua University, Beijing; 100084, China; (6) School of Electronics and Control Engineering, Chang'an University, Shaanxi, Xi'an; 710064, China; (7) Center of Respiratory Medicine, China-Japan Friendship Hospital, National Center for Respiratory Medicine, Institute of Respiratory Medicine, Chinese Academy of Medical Sciences, National Clinical Research Center for Respiratory Diseases, Beijing; 100020, China; (8) Department of Respiratory, the Second Affiliated Hospital of Harbin Medical University, Harbin, Heilongjiang; 150086, China; (9) Internal Medicine, Harbin Medical University, Harbin, Heilongjiang; 150081, China; (10) School of Artificial Intelligence, OPtics and ElectroNics (iOPEN), Northwestern Polytechnical University, Xi'an; 710072, China; (11) Translational Research Center, Shanghai YangZhi Rehabilitation Hospital (Shanghai Sunshine Rehabilitation Center), Shanghai; 201619, China; (12) School of Mechanical Engineering, Tongji University, Shanghai; 201804, China; (13) Laboratory of Pleural and Lung Cancer Translational Research, CAMS Oxford Institute, Nuffield Department of Medicine, University of Oxford, Oxford, United Kingdom; (14) Oxford Centre for Respiratory Medicine, Churchill Hospital, Oxford University Hospitals NHS Foundation Trust, Oxford, United Kingdom; (15) National Institute for Health Research Oxford Biomedical Research Centre, University of Oxford, Oxford, United Kingdom; (16) Plastic Surgery Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing; 100144, China; (17) State Key Laboratory of Common Mechanism Research for Major Diseases, Beijing; 100005, ChinaPublication Year:2024Volume:97Article Number:103248DOI Link:10.1016/j.media.2024.103248數(shù)據(jù)庫ID（收錄號）:20242616508439 -
Record 57 of
Title:On-chip generation and processing of ultrafast time-entangled photonic qudits for quantum communications
Author Full Names:Sciara, Stefania(1); Yu, Hao(1,2); Chemnitz, Mario(1,3); Montaut, Nicola(1); Fischer, Bennet(1,3); Helsten, Robin(1); Crockett, Benjamin(1); Wetzel, Benjamin(4); Goebel, Thorsten A.(5); Kr?mer, Ria G.(5); Little, Brent E.(6); Chu, Sai T.(7); Nolte, Stefan(5,8); Munro, William J.(9); Moss, David J.(10); Aza?a, José(1); Wang, Zhiming(2); Morandotti, Roberto(1,2)Source Title:2024 Conference on Lasers and Electro-Optics, CLEO 2024Language:EnglishDocument Type:Conference article (CA)Conference Title:2024 Conference on Lasers and Electro-Optics, CLEO 2024Conference Date:May 7, 2024 - May 10, 2024Conference Location:Charlotte, NC, United statesConference Sponsor:American Elements; American Physical Society, Division of Laser Science; et al.; IEEE Photonics Society; IPG Photonics; LIGENTECAbstract:We present a photonic platform for the generation and processing of picosecond-spaced time entangled qudits, based on on-chip interferometers and a spiral waveguide. We utilize these qudits to implement quantum communications over standard optical fibers. ? Optica Publishing Group 2024 ? 2024 The Author (s)Affiliations:(1) Institut national de la recherche scientifique - Centre énergie, Matériaux et Télécommunications (INRS-EMT), Varennes; J3X 1S2, Canada; (2) Institute of Fundamental and Frontier Sciences, University of Science and Technology of China, Chendu; 610054, China; (3) Leibniz Institute of Photonic Technology, Albert-Einstein Strasse 9, Jena; 07745, Germany; (4) XLIM Research Institute, CNRS, UMR 7252, Université de Limoges, Limoges; 87060, France; (5) Friedrich Schiller University Jena, Abbe Center of Photonics, Institute of Applied Physics, Albert-Einstein-Strasse 15, Jena; 07745, Germany; (6) QXP Technology Inc., Xi'an, China; (7) Department of Physics, City University of Hong Kong, Hong Kong, Hong Kong; (8) Fraunhofer Institute for Applied Optics and Precision Engineering IOF, Center of Excellence in Photonics, Albert-Einstein-Strasse 7, Jena; 07745, Germany; (9) Okinawa Institute of Science and Technology Graduate University, Okinawa, Onna-son; 904-0495, Japan; (10) Optical Sciences Centre, Swinburne University of Technology, Hawthorn; VIC; 3122, AustraliaPublication Year:2024DOI Link:10.1364/cleo_fs.2024.ftu4f.6數(shù)據(jù)庫ID（收錄號）:20244917467986 -
Record 58 of
Title:On-chip generation and processing of ultrafast time-entangled photonic qudits for quantum communications
Author Full Names:Sciara, Stefania(1); Yu, Hao(1,2); Chemnitz, Mario(1,3); Montaut, Nicola(1); Fischer, Bennet(1,3); Helsten, Robin(1); Crockett, Benjamin(1); Wetzel, Benjamin(4); Goebel, Thorsten A.(5); Kr?mer, Ria G.(5); Little, Brent E.(6); Chu, Sai T.(7); Nolte, Stefan(5,8); Munro, William J.(9); Moss, David J.(10); Aza?a, José(1); Wang, Zhiming(2); Morandotti, Roberto(1,2)Source Title:CLEO: Fundamental Science, CLEO:FS 2024 in Proceedings CLEO 2024 - Part of Conference on Lasers and Electro-OpticsLanguage:EnglishDocument Type:Conference article (CA)Conference Title:CLEO: Fundamental Science, CLEO:FS 2024 - Part of Conference on Lasers and Electro-Optics, CLEO 2024Conference Date:May 5, 2024 - May 10, 2024Conference Location:Charlotte, NC, United statesAbstract:We present a photonic platform for the generation and processing of picosecond-spaced time entangled qudits, based on on-chip interferometers and a spiral waveguide. We utilize these qudits to implement quantum communications over standard optical fibers. ? Optica Publishing Group 2024 ? 2024 The Author(s)Affiliations:(1) Institut National de la Recherche Scientifique - Centre énergie, Matériaux et Télécommunications (INRS-EMT), Varennes; J3X 1S2, Canada; (2) Institute of Fundamental and Frontier Sciences, University of Science and Technology of China, Chendu; 610054, China; (3) Leibniz Institute of Photonic Technology, Albert-Einstein Strasse 9, Jena; 07745, Germany; (4) XLIM Research Institute, CNRS, UMR 7252, Université de Limoges, Limoges; 87060, France; (5) Friedrich Schiller University Jena, Abbe Center of Photonics, Institute of Applied Physics, Albert-Einstein-Strasse 15, Jena; 07745, Germany; (6) QXP Technology Inc., Xi'an, China; (7) Department of Physics, City University of HongKong, Hong Kong, Hong Kong; (8) Fraunhofer Institute for Applied Optics and Precision Engineering IOF, Center of Excellence in Photonics, Albert-Einstein-Strasse 7, Jena; 07745, Germany; (9) Okinawa Institute of Science and Technology, Graduate University, Okinawa, Onna-son; 904-0495, Japan; (10) Optical Sciences Centre, Swinburne University of Technology, Hawthorn; VIC; 3122, AustraliaPublication Year:2024DOI Link:10.1364/cleo_fs.2024.ftu4f.6數(shù)據(jù)庫ID（收錄號）:20244217221602 -
Record 59 of
Title:New Upper Limit on the Axion-Photon Coupling with an Extended CAST Run with a Xe-Based Micromegas Detector
Author Full Names:Altenmüller, K.(1); Anastassopoulos, V.(2); Arguedas-Cuendis, S.(3); Aune, S.(4); Baier, J.(5); Barth, K.(3); Br?uninger, H.(6); Cantatore, G.(7); Caspers, F.(3,8); Castel, J.F.(1); ?etin, S.A.(9); Christensen, F.(10); Cogollos, C.(1,11); Dafni, T.(1); Davenport, M.(3); Decker, T.A.(12); Desch, K.(13); Díez-Ibá?ez, D.(1); D?brich, B.(3); Ferrer-Ribas, E.(4); Fischer, H.(5); Funk, W.(3); Galán, J.(1); García, J.A.(1); Gardikiotis, A.(14); Giomataris, I.(4); Golm, J.(3,15); Hailey, C.H.(16); Hasinoff, M.D.(17); Hoffmann, D.H.H.(18); Irastorza, I.G.(1); Jacoby, J.(5); Jakobsen, A.C.(10); Jakov?i?, K.(19); Kaminski, J.(13); Karuza, M.(20,21); Kostoglou, S.(3); Krieger, C.(22); Laki?, B.(19); Laurent, J.M.(3); Luzón, G.(1); Malbrunot, C.(3); Margalejo, C.(1); Maroudas, M.(23); Miceli, L.(24); Mirallas, H.(1); Navarro, P.(25); Obis, L.(1); ?zbey, A.(9,26); ?zbozduman, K.(9,27); Papaevangelou, T.(4); Pérez, O.(1); Pivovaroff, M.J.(12); Rosu, M.(28); Ruiz-Chóliz, E.(1); Ruz, J.(1,12); Schmidt, S.(13); Schumann, M.(5); Semertzidis, Y.K.(24,29); Solanki, S.K.(30); Stewart, L.(3); Vafeiadis, T.(3); Vogel, J.K.(1,12); Zioutas, K.(2,3)Source Title:Physical Review LettersLanguage:EnglishDocument Type:Journal article (JA)Abstract:Hypothetical axions provide a compelling explanation for dark matter and could be emitted from the hot solar interior. The CERN Axion Solar Telescope has been searching for solar axions via their back conversion to x-ray photons in a 9-T 10-m long magnet directed toward the Sun. We report on an extended run with the International Axion Observatory pathfinder detector, doubling the previous exposure time. The detector was operated with a xenon-based gas mixture for part of the new run, providing technical insights for future configurations. No counts were detected in the 95% signal-encircling region during the new run, while 0.75 were expected. The new data improve the axion-photon coupling limit to 5.8×10-11 GeV-1 at 95% CL (for ma0.02 eV), the most restrictive experimental limit to date. ? 2024 authors. Published by the American Physical Society.Affiliations:(1) Centro de Astropartículas y Física de Altas Energías (CAPA), Departamento de Física Teórica, University de Zaragoza, Zaragoza; 50009, Spain; (2) Physics Department, University of Patras, Patras, Greece; (3) European Organization for Nuclear Research (CERN), Geneva 23; 1211, Switzerland; (4) IRFU, CEA, Université Paris-Saclay, Gif-sur-Yvette; 91191, France; (5) Physikalisches Institut, Albert-Ludwigs-Universit?t Freiburg, Freiburg; 79104, Germany; (6) Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany; (7) University of Trieste and Instituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste, Trieste, Italy; (8) European Scientific Institute, Archamps, France; (9) Istinye University, Institute of Sciences, Sariyer, Istanbul; 34396, Turkey; (10) DTU Space, National Space Institute, Technical University of Denmark, Lyngby; 2800, Denmark; (11) Institut de Ciències Del Cosmos, Universitat de Barcelona (UB-IEEC), Catalonia, Barcelona, Spain; (12) Lawrence Livermore National Laboratory, Livermore; CA; 94550, United States; (13) Physikalisches Institut, University of Bonn, Bonn; 53115, Germany; (14) Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Padova, Padova; 35131, Italy; (15) Institute for Optics and Quantum Electronics, Friedrich Schiller University Jena, Jena, Germany; (16) Physics Department and Columbia Astrophysics Laboratory, Columbia University, New York; NY; 10027, United States; (17) Department of Physics and Astronomy, University of British Columbia, Vancouver; BC, Canada; (18) Xi'An Jiaotong University, School of Science, Xi'An; 710049, China; (19) Rudjer Bo?kovi? Institute, Zagreb, Croatia; (20) Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste, Trieste, Italy; (21) Faculty of Physics, Center for Micro and Nano Sciences and Technologies, University of Rijeka, Rijeka; 51000, Croatia; (22) Universit?t Hamburg, Hamburg, Germany; (23) Institute of Experimental Physics, University of Hamburg, Hamburg; 22761, Germany; (24) Center for Axion and Precision Physics Research, Institute for Basic Science (IBS), Daejeon; 34141, Korea, Republic of; (25) Department of Information and Communications Technologies, Technical University of Cartagena, Murcia; 30203, Spain; (26) Istanbul University-Cerrahpasa, Department of Mechanical Engineering, Avcilar, Istanbul, Turkey; (27) Bo?azi?i University, Physics Department, Bebek, Istanbul, Turkey; (28) Extreme Light Infrastructure - Nuclear Physics (ELI-NP), Magurele; 077125, Romania; (29) Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon; 34141, Korea, Republic of; (30) Max-Planck-Institut für Sonnensystemforschung, G?ttingen; 37077, GermanyPublication Year:2024Volume:133Issue:22Article Number:221005DOI Link:10.1103/PhysRevLett.133.221005數(shù)據(jù)庫ID（收錄號）:20244817454689 -
Record 60 of
Title:The scintillating-fiber tracker (FIT) of the HERD space mission from design to performance
Author Full Names:Adriani, O.(1,2); Alemanno, F.(3,4); Altomare, C.(5); Ambrosi, G.(6); Antonelli, M.(7); Bai, X.H.(9); Bai, Y.L.(9); Bao, T.W.(10); Barbanera, M.(6); Barbato, F.C.T.(3,4); Bernard, F.(11); Bernardini, P.(12,13); Berti, E.(2); Bertucci, B.(6,14); Betti, P.(1,2); Bi, X.J.(10,15); Bigongiari, G.(16,17); Blanch, O.(18); Boix, J.(18); Bongi, M.(1,2); Bonvicini, V.(7); Bottai, S.(2); Brogi, P.(16,17); Brugnoni, C.(6,14); Cadoux, F.(8); Cagnoli, I.(3,4); Cai, H.Y.(10,15); Campana, D.(19); Cao, W.W.(9); Cardiel-Sas, L.(18); Casaus, J.(20); Casilli, E.(12,13); Catala, R.(21); Catanzani, E.(6,14); Cattaneo, P.W.(22); Cerasole, D.(5,23); Chang, L.(24); Chen, H.(10,15); Chen, K.(25); Chen, L.(26); Chen, M.L.(10); Chen, P.D.(27); Chen, R.(25); Cheng, Y.D.(10,15); Cianetti, F.(6,14); Comerma, A.(28); Cong, X.Q.(29); Coppin, P.(8); Cui, X.Z.(10); D'Alessandro, R.(1,2); D'Urso, D.(6,30); Díaz, C.(20); Dai, C.(31); De Mitri, I.(3,4); de Palma, F.(12,13); De Vecchi, C.(22); Di Felice, V.(32); Di Giovanni, A.(3,4); Di Santo, M.(3,4); Di Venere, L.(5); Dong, Y.W.(10); Donvito, G.(5); Du, Y.J.(33); Duranti, M.(6); Espinya, A.(21); Fang, K.(10); Fari?a, L.(18); Favre, Y.(8); Feng, H.B.(31); Fernandez Alonso, M.(3,4); Finetti, N.(2,34); Fontanella, G.(3,4); Formato, V.(32); Frieden, J.M.(11); Fu, Y.(33); Fusco, P.(5,23); Gao, J.R.(9); Gargano, F.(5); Gascón, D.(21,35); Gasparrini, D.(32); Ghose, E.(12,13,48); Giovacchini, F.(20); Gómez, S.(21,28); Gong, K.(10); Gu, M.H.(10); Guberman, D.(21); Guerrisi, C.(5,23); Guida, R.(36); Guo, D.Y.(10); Guo, J.H.(37); He, H.L.(10,15); Hu, H.(10); Hu, H.J.(31); Hu, Y.M.(37); Hu, Z.X.(29); Huang, G.S.(27); Huang, W.H.(38); Huang, X.T.(38); Huang, Y.G.(33); Ionica, M.(6); Jia, F.(31); Jia, J.S.(33); Jiang, F.(31); Jiang, X.W.(10); Jiang, Y.(6,14); Jiao, P.(33); Kotenko, A.(8); Kyratzis, D.(3,4); La Marra, D.(8); Lathika, K.R.(18); Li, L.(10); Li, M.J.(38); Li, M.X.(25); Li, Q.Y.(39); Li, Q.Y.(40); Li, R.(9); Li, S.L.(10,15); Li, T.(29); Li, T.(38); Li, X.Q.(10); Li, X.Q.(41); Li, Y.Y.(39); Li, Z.H.(10,15); Liang, M.J.(10,15); Liang, X.Z.(9); Liao, C.L.(10,15); Licciulli, F.(5); Lin, Y.J.(29); Liu, B.H.(24); Liu, D.(38); Liu, H.(26); Liu, H.B.(31); Liu, H.W.(10); Liu, X.(10,15); Liu, X.J.(10); Liu, X.W.(31); Liu, Y.Q.(10); Loparco, F.(5,23); Loporchio, S.(5,23); Lorusso, L.(5,23); Lu, B.(10); Lu, R.S.(10,15); Lu, Y.P.(10); Lucchetta, G.(18); Lv, J.G.(10); Lv, L.W.(9); Maestro, P.(16,17); Mancini, E.(6); Manera, R.(21); Marin, J.(20); Marrocchesi, P.S.(16,17); Marsella, G.(42,43); Martinez, G.(20); Martinez, M.(18); Mauricio, J.(21); Mazziotta, M.N.(5); Morettini, G.(6,14); Mori, N.(2); Mussolin, L.(6,14); Nicotri, S.(5); Niu, Y.(38); Oliva, A.(44); Orlandi, D.(4); Orta, M.(21,35)Source Title:Proceedings of ScienceLanguage:EnglishDocument Type:Conference article (CA)Conference Title:38th International Cosmic Ray Conference, ICRC 2023Conference Date:July 26, 2023 - August 3, 2023Conference Location:Nagoya, JapanConference Sponsor:et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya UniversityAbstract:The High Energy cosmic-Radiation Detection facility (HERD) will be a calorimetric experiment on board the China Space Station. Starting from 2027, HERD will perform the first direct measurement of cosmic rays in the PeV region and the gamma-ray full-sky survey from 100 MeV. The detector will be equipped with a scintillating-fiber tracker (FIT) read out with silicon photomultipliers. A miniature of a FIT sector, called MiniFIT, was designed, built and tested with particle beams at CERN. The FIT design, together with the design and physics performance of MiniFIT will be presented in this contribution. ? Copyright owned by the author(s) under the terms of the Creative Commons.Affiliations:(1) Department of Physics, University of Florence, Via Sansone 1, Sesto Fiorentino, Firenze; I-50019, Italy; (2) Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Sesto Fiorentino, Via Sansone 1, Firenze; I-50019, Italy; (3) Gran Sasso Science Institute (GSSI), Viale Crispi 7, L'Aquila; I-67100, Italy; (4) Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso, Via Acitelli 22, Assergi, L'Aquila; I-67100, Italy; (5) Istituto Nazionale di Fisica Nucleare, Sezione di Bari, via Orabona 4, Bari; I-70126, Italy; (6) Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Via Alessandro Pascoli 23c, Perugia; I-06123, Italy; (7) Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, via A. Valerio 2, Trieste; I-34127, Italy; (8) Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, 24 quai Ernest-Ansermet, 4, Genève; CH-1211, Switzerland; (9) Xi'an Institute of Optics and Precision Mechanics, CAS, No.17 Xinxi Road, New Industrial Park, Xi'an Hi-Tech Industrial Development Zone, Xi'an; 710019, China; (10) Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Shijingshan District, Beijing; 100049, China; (11) Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Batiment PH, Station 3, Lausanne; CH-1015, Switzerland; (12) Dipartimento di Matematica e Fisica 'E. De Giorgi', Università del Salento, Lecce; I-73100, Italy; (13) Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Via per Arnesano, Lecce; I-73100, Italy; (14) Università degli Studi di Perugia, Piazza Università 1, Perugia; I-06123, Italy; (15) University of Chinese Academy of Sciences, No.1 Yanqihu East Rd, Huairou District, Beijing; 101408, China; (16) Department of Physical Sciences, Earth and Environment, University of Siena, via Roma 56, Siena; I-53100, Italy; (17) Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Largo B. Pontecorvo 3, Pisa; I-56127, Italy; (18) Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), Bellaterra, Barcelona; E-08193, Spain; (19) Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Via Cintia, Napoli; I-80126, Italy; (20) Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid; E-28040, Spain; (21) Departament de Física Quàntica i Astrofísica (FQA), Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), Barcelona; E-08028, Spain; (22) Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, Via Bassi 6, Pavia; I-27100, Italy; (23) Dipartimento di Fisica, 'M. Merlin' dell'Università e del Politecnico di Bari, via Amendola 173, Bari; I-70126, Italy; (24) North Night Vision Technology Co., Ltd., Hongwai Road 5, Kunming; 650217, China; (25) PLAC, Key Laboratory of Quark & Lepton Physics (MOE), Central China Normal University, Wuhan; 430079, China; (26) School of Physical Science and Technology, Southwest Jiaotong University, No.999, Xi'an Road, Chengdu; 611756, China; (27) Department of Modern Physics, University of Science and Technology of China, Hefei; 230026, China; (28) Polytechnic University of Catalonia (UPC), Electronics Department, Barcelona; E-08019, Spain; (29) North Night Vision Science & Technology (Nanjing) Research Institute Co., Ltd, Kangping Street 2, Nanjing; 211100, China; (30) Università degli Studi di Sassari, Piazza Università 21, Sassari; I-07100, Italy; (31) Guangxi Key Laboratory for Relativistic Astrophysics, Guangxi University, Daxue East Road 100, Nanning; 530004, China; (32) Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, via della Ricerca Scientifica 1, Roma; I-00133, Italy; (33) Institute of Special Glass Fiber & Optoelectronic Functional Materials, China Building Materials Academy, Guanzhuang Dongli 1, Chaoyang district, Beijing; 100024, China; (34) Department of Physical and Chemical Sciences, University of L'Aquila, Via Vetoio, Coppito, L'Aquila; I-67100, Italy; (35) Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona; E-08034, Spain; (36) Dipartimento di Ingegneria Industriale, Università degli Studi di Napoli Federico II, P.le Tecchio 80, Napoli; I-80125, Italy; (37) Purple Mountain Observatory, CAS, No.10 Yuanhua Road, Qixia District, Nanjing; 210023, China; (38) Shandong University (SDU), 72 Binhai Road, Qingdao, Jimo; 266237, China; (39) Shandong University (SDU), 27 Shanda Nanlu, Shandong, Jinan; 250100, China; (40) Shandong Institute of Advanced Technology (SDIAT), 1501, Panlong Road, Shandong, Jinan; 250100, China; (41) Institute of Modern Physics, CAS, 509 Nanchang Rd., Lanzhou; 730000, China; (42) Dipartimento di Fisica e Chimica, 'E. Segrè', Università degli Studi di Palermo, via delle Scienze, Palermo; I-90128, Italy; (43) Istituto Nazionale di Fisica Nucleare, Sezione di Catania, Via Santa Sofia 64, Catania; I-95123, Italy; (44) Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Viale C. Berti Pichat 6/2, Bologna; I-40127, Italy; (45) Università di Napoli Federico II, Dipartimento di Fisica 'Ettore Pancini', Via Cintia, Napoli; I-80126, Italy; (46) Agenzia Spaziale Italiana, via del Politecnico s.n.c., Roma; I-00133, Italy; (47) Département d'Astronomie, Université de Genève, Chemin d'Ecogia 16, Versoix; CH-1290, Switzerland; (48) Dipartimento di Fisica, Università di Trento, via Sommarive 14, Trento; I-38123, ItalyPublication Year:2024Volume:444Article Number:147數(shù)據(jù)庫ID（收錄號）:20245117556256