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Deep learning-based conjugate orbital angular momentum interferometry for in-plane displacement measurement. 基于深度学习的共轭轨道角动量干涉法面内位移测量。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.570239
Qinyu Li, Zhanwu Xie, Yuanheng Shi, Wei Xia, Dongmei Guo

A deep learning-based phase demodulation algorithm is proposed for measuring in-plane displacements in conjugate orbital angular momentum (OAM) interferometry. The phase demodulation hybrid neural network (PDHNN) is designed to directly demodulate petal-shaped interferograms in a single step. PDHNN employs a custom ResNet-transformer architecture with deformable convolutions and attention mechanisms to extract rotation-sensitive features from petal-shaped interferograms for robust phase demodulation. The algorithm has been validated using both simulated and experimental data. Experimental results show that the demodulation accuracy reaches 91.60% within an error margin of 1°, and within a 0.1° error range, the average displacement error is 0.13 nm, demonstrating high robustness and stability in noisy conditions.

提出了一种基于深度学习的相位解调算法,用于共轭轨道角动量干涉测量中面内位移的测量。设计了相位解调混合神经网络(PDHNN),用于单步直接解调花瓣型干涉图。PDHNN采用自定义resnet变压器架构,具有可变形的卷积和注意机制,从花瓣形干涉图中提取旋转敏感特征,用于鲁棒相位解调。仿真和实验数据验证了该算法的有效性。实验结果表明,在1°的误差范围内,解调精度达到91.60%,在0.1°的误差范围内,平均位移误差为0.13 nm,在噪声条件下具有较高的鲁棒性和稳定性。
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引用次数: 0
Two-dimensional light beam shape characterization using interferometric closure amplitudes. 利用干涉闭合振幅的二维光束形状表征。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.568171
Nithyanandan Thyagarajan, Bojan Nikolic, Christopher L Carilli, Laura Torino, Ubaldo Iriso

We introduce a technique using closure amplitudes, inspired by radio interferometry, to determine, with high angular resolution, the two-dimensional profile of a light beam using an interferogram from a non-redundantly masked aperture. Previous techniques required multiple interferograms or accurate estimates of the non-uniform illuminations across the aperture. In contrast, our method, using closure amplitudes, avoids the need to estimate the aperture illuminations while determining the two-dimensional beam shape from a single interferogram. The invariance of closure amplitudes to even time-varying aperture illuminations makes it suitable for longer averaging intervals, with the potential to reduce data rates and computational overheads. By using data from the ALBA synchrotron light source to validate the method and its results against existing methods, this paper represents, to our knowledge, the first real-world application of closure amplitudes to directly determine the light beam's profile using optical interferometry in the high angular resolution regime.

我们介绍了一种使用闭合振幅的技术,灵感来自无线电干涉测量,以高角分辨率确定光束的二维轮廓,使用来自非冗余掩模孔径的干涉图。以前的技术需要多个干涉图或精确估计孔径上的非均匀光照。相比之下,我们的方法,使用闭合幅度,避免了估计孔径照度的需要,同时确定二维光束形状从一个单一的干涉图。闭合幅度对时变孔径照明的不变性使其适用于较长的平均间隔,具有降低数据速率和计算开销的潜力。通过使用来自ALBA同步加速器光源的数据来验证该方法及其结果与现有方法的对比,据我们所知,本文代表了在高角分辨率下使用光学干涉测量法直接确定光束轮廓的第一个实际应用。
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引用次数: 0
Fringe visibility for pulsed digital holography with large optical path differences. 大光程差脉冲数字全息的条纹可视性。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.567877
Samuel T Thurman, Anthony C Klee

In interferometry and holography systems, the optical path difference (OPD) between the beams must be kept smaller than the source coherence length to obtain stable interference fringes. When the OPD is larger than the coherence length, the fringe phase drifts on time scales comparable to the source coherence time. This reduces fringe visibility and causes fringes to wash out completely for observation times longer than the coherence time. High fringe visibility measurements, however, can be obtained with pulsed sources (or very short detector integration times), if the pulse duration is shorter than the source coherence time, thereby limiting the amount of fringe phase drift over the pulse duration. We analyze cases where optical pulses are carved from a continuous-wave laser source. We derive an expression for the squared magnitude of the fringe visibility for pulsed interference measurements and demonstrate that high visibility fringes can be obtained even when the OPD is much longer than the source coherence length. As a rule of thumb, the source coherence time should be at least 10 times greater than the pulse duration to obtain expected fringe visibilities greater than 95% when the source laser has a Lorentzian line shape. This result is important to the design of digital holography systems for long-range remote sensing applications, where it is difficult to implement a dynamic optical delay line for path length matching with non-cooperative objects.

在干涉测量和全息系统中,为了获得稳定的干涉条纹,光束之间的光程差(OPD)必须小于光源相干长度。当OPD大于相干长度时,条纹相位在与源相干时间相当的时间尺度上漂移。这降低了条纹的可见度,并导致条纹在比相干时间长几倍的观测时间内完全被洗掉。然而,如果脉冲持续时间短于源相干时间,则可以使用脉冲源(或非常短的探测器积分时间)获得高条纹可见性测量,从而限制了脉冲持续时间内条纹相位漂移的量。我们分析了从连续波激光源切割光脉冲的情况。我们推导了脉冲干涉测量条纹可见度的平方量级表达式,并证明了即使OPD比源相干长度长得多,也可以获得高可见度的条纹。根据经验,当源激光具有洛伦兹线形状时,源相干时间应至少大于脉冲持续时间的10倍,以获得大于95%的预期条纹可见度。这一结果对于远程遥感应用的数字全息系统设计具有重要意义,因为在远程遥感应用中,很难实现与非合作对象进行路径长度匹配的动态光延迟线。
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引用次数: 0
High-resolution dual-band triple-grating spectrometer for atmospheric CO2 detection. 用于大气CO2探测的高分辨率双频三光栅光谱仪。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.563970
Hongling Yuan, Zhiwei Feng, Guo Xia, Hui Zhang, Yongqing Wei, Shunlong Shu

The detection of atmospheric carbon dioxide concentrations typically occurs within the near-infrared spectral band. To achieve high-precision measurements, it is essential not only to maintain high spectral resolution but also to capture spectral information across multiple wavelength ranges. Therefore, we propose a novel, to our knowledge, optical design for a high-resolution dual-band triple-grating spectrometer (DTGS). The design strategy is centered on fully utilizing the grating through simultaneous ±1st-order diffraction, enabling high-resolution acquisition of dual-band spectral information while enhancing system integration. We performed theoretical derivations and simulation validations for the initial structure of the DTGS system. The simulation results indicate that the DTGS system achieves high-resolution detection (0.072-0.075 nm spectral resolution) in near-infrared dual-band CO2 weak absorption spectra (1.556-1.576µm and 1.578-1.598µm) through a grating configuration of one 555 lines/mm and two 1100 lines/mm, overcoming the spectral resolution constraints of traditional optical systems in wide-band measurements.

大气二氧化碳浓度的检测通常发生在近红外光谱带内。为了实现高精度测量,不仅要保持高光谱分辨率,而且要捕获跨多个波长范围的光谱信息。因此,我们提出了一种新颖的,据我们所知,高分辨率双波段三光栅光谱仪(DTGS)的光学设计。设计策略以充分利用光栅为中心,通过同时±一阶衍射,在提高系统集成度的同时,实现双波段光谱信息的高分辨率采集。我们对DTGS系统的初始结构进行了理论推导和仿真验证。仿真结果表明,DTGS系统通过1条555线/mm和2条1100线/mm的光栅配置,在近红外双频CO2弱吸收光谱(1.556 ~ 1.576µm和1.578 ~ 1.598µm)中实现了0.072 ~ 0.075 nm的高分辨率检测,克服了传统光学系统在宽带测量中光谱分辨率的限制。
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引用次数: 0
Optical spatiotemporal Fourier synthesis: tutorial. 光学时空傅立叶合成:教程。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.566252
Murat Yessenov, Ayman F Abouraddy

Fourier synthesis is one of the foundations of physical optics. Spatial Fourier optics is a basis for understanding optical imaging, microscopy, and holography. In conventional Fourier optics, the complex spatial field distribution in the Fourier plane constitutes the spatial spectrum of the field to be realized in physical space. Analogously, in temporal Fourier optics, the complex temporal spectrum can be manipulated for ultrafast pulse-shaping. We present here a tutorial on the emerging field of spatiotemporal Fourier optics whereby the spatial and temporal spectra are manipulated jointly to produce spatiotemporally structured optical fields that display unique propagation characteristics. In this tutorial, we focus on a subset of the overall class of nonseparable spatiotemporally structured fields, namely cylindrically symmetric fields in which each radial spatial frequency is associated with a single wavelength. This subset of fields comprises propagation-invariant wave packets that travel rigidly in linear media at a tunable group velocity and includes space-time wave packets and other closely related structured fields. We describe a spatiotemporal Fourier synthesis system capable of preparing arbitrary optical fields belonging to this subclass.

傅里叶合成是物理光学的基础之一。空间傅里叶光学是理解光学成像、显微术和全息术的基础。在传统的傅里叶光学中,傅里叶平面上的复杂空间场分布构成了在物理空间中要实现的场的空间谱。类似地,在时间傅里叶光学中,可以操纵复时间谱来实现超快脉冲整形。我们在这里介绍了一个关于时空傅里叶光学新兴领域的教程,其中空间和时间光谱被联合操纵以产生时空结构的光场,显示出独特的传播特性。在本教程中,我们将重点关注不可分离时空结构场的一个子集,即每个径向空间频率与单个波长相关联的圆柱对称场。这个场子集包括以可调群速度在线性介质中严格传播的传播不变波包,包括时空波包和其他密切相关的结构化场。我们描述了一个能够制备属于该子类的任意光场的时空傅立叶合成系统。
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引用次数: 0
Generation of high-intensity 3D Gaussian-like spots via near-field diffraction from 2D orthogonally chirped structures. 通过近场衍射从二维正交啁啾结构产生高强度三维高斯样斑。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.567609
Mohammadreza Zarei, Saifollah Rasouli, Davud Hebri, Li-Gang Wang

This study presents a class of two-dimensional (2D) spatial-frequency-modulated structures with transmittance d1=0.10mm, in which the periodicity can vary along both the d2=0.30mm- and nc=1-axes. Specifically, the structure exhibits spatial frequencies nav=3 and z=0 that sinusoidally alternate between two values along both directions, with the possibility of unequal modulation in the T(x,y)- and x-axes. It is shown that y generally behaves as an almost periodic function, resulting in an impulsive spatial spectrum. However, we identify the conditions under which fx becomes periodic, and its spatial spectrum forms a lattice of impulses. When these periodicity conditions are met, we refer to the structure as a 2D spatially chirped periodic structure. These structures are characterized by four natural numbers, denoted as fy, x, y, and T(x,y), which represent the modulation in the T(x,y)- and ncx-directions, respectively, and two real parameters, named frequency modulation strengths in both the ncy- and navx-directions, denoted by navy and x, respectively. As a special case, we define a 2D spatially chirped amplitude sinusoidal structure (SCASS), based on the transmission function of a conventional 2D amplitude sinusoidal grating, where the phase of the conventional grating is replaced by a desired chirped phase. The near-field diffraction from 2D SCASSs is studied using the angular (spatial) spectrum method. The Talbot distances for these gratings are determined and verified experimentally, showing that the intensity profiles at specific Talbot distances are highly dependent on the parameters y, x, y, kx, ky, and ncx. Furthermore, we formulated the near-field diffraction of a plane wave from 2D multiplicatively separable spatially chirped amplitude sinusoidal structures, considering the variability of spatial periods in both the ncy- and navx-directions. In comparison with conventional 2D gratings, new, to our knowledge, and intriguing diffraction patterns are observed, such as sharp and smooth Gaussian-like intensity spots generated via the diffraction of the incident wave, with nearly diffraction-limited features but limited overall efficiency. These intensity spots depend on the characteristic parameters of the structure. By carefully manipulating the navy parameters, we have the ability to generate maximum intensity peaks within these 2D SCASSs, which are

本文提出了一类二维(2D)空间调频结构,其透过率d1=0.10mm,其周期性可以沿d2=0.30mm-和nc=1轴变化。具体来说,该结构的空间频率nav=3和z=0沿两个方向在两个值之间正弦交替,并可能在T(x,y)和x轴上进行不等调制。结果表明,y一般表现为近似周期函数,产生脉冲空间谱。然而,我们确定了fx成为周期性的条件,其空间频谱形成脉冲的晶格。当满足这些周期性条件时,我们将该结构称为二维空间啁啾周期结构。这些结构的特征是四个自然数,分别表示为fy, x,y和T(x,y),分别表示T(x,y)和ncx方向的调制,以及两个实参数,分别表示ncy和navx方向的频率调制强度,分别表示为navy和x。作为一种特殊情况,我们基于传统二维振幅正弦光栅的传输函数定义了二维空间啁啾振幅正弦结构(SCASS),其中传统光栅的相位被所需的啁啾相位所取代。利用角(空间)谱方法研究了二维scass近场衍射。这些光栅的塔尔博特距离是确定和实验验证,表明强度分布在特定的塔尔博特距离高度依赖于参数y, x, y, kx, ky,和ncx。此外,考虑到空间周期在近方向和中方向上的可变性,我们从二维乘分空间啁啾振幅正弦结构中推导出平面波的近场衍射。与传统的二维光栅相比,新的,据我们所知,有趣的衍射模式被观察到,如通过入射波的衍射产生的尖锐和光滑的类高斯强度斑,具有几乎衍射有限的特征,但有限的整体效率。这些强度点取决于结构的特征参数。通过仔细操纵海军参数,我们有能力在这些2D scass中产生最大强度峰值,这是入射光强度的22倍。将这些最大强度峰与它们的一维啁啾对应物进行比较,可以发现显著的差异。我们展示了一个有趣的结果:一维啁啾结构和二维scass的塔尔博特地毯中的高强度斑点出现在不同的传播平面上,而这些斑点精确地位于一维和二维二元光栅的塔尔博特和半塔尔博特平面上。另一个有趣的结果表明,在一维和二维二元光栅的自成像区前后,沿传播方向的强度分布的下降发生在两个紧密间隔的强度最大值附近。对于一维啁啾结构和二维scass,强度点在传播方向和横向上都表现出类似高斯的斑点分布,使得这些空间点适合于三维阵列中粒子的三维捕获,而不需要外部成像系统。
{"title":"Generation of high-intensity 3D Gaussian-like spots via near-field diffraction from 2D orthogonally chirped structures.","authors":"Mohammadreza Zarei, Saifollah Rasouli, Davud Hebri, Li-Gang Wang","doi":"10.1364/JOSAA.567609","DOIUrl":"https://doi.org/10.1364/JOSAA.567609","url":null,"abstract":"<p><p>This study presents a class of two-dimensional (2D) spatial-frequency-modulated structures with transmittance <i>d</i><sub>1</sub>=0.10<i>m</i><i>m</i>, in which the periodicity can vary along both the <i>d</i><sub>2</sub>=0.30<i>m</i><i>m</i>- and <i>n</i><sub>c</sub>=1-axes. Specifically, the structure exhibits spatial frequencies <i>n</i><sub><i>a</i><i>v</i></sub>=3 and <i>z</i>=0 that sinusoidally alternate between two values along both directions, with the possibility of unequal modulation in the <i>T</i>(<i>x</i>,<i>y</i>)- and <i>x</i>-axes. It is shown that <i>y</i> generally behaves as an almost periodic function, resulting in an impulsive spatial spectrum. However, we identify the conditions under which <i>f</i><sub>x</sub> becomes periodic, and its spatial spectrum forms a lattice of impulses. When these periodicity conditions are met, we refer to the structure as a 2D spatially chirped periodic structure. These structures are characterized by four natural numbers, denoted as <i>f</i><sub>y</sub>, <i>x</i>, <i>y</i>, and <i>T</i>(<i>x</i>,<i>y</i>), which represent the modulation in the <i>T</i>(<i>x</i>,<i>y</i>)- and <i>n</i><sub><i>c</i><i>x</i></sub>-directions, respectively, and two real parameters, named frequency modulation strengths in both the <i>n</i><sub><i>c</i><i>y</i></sub>- and <i>n</i><sub><i>a</i><i>v</i><i>x</i></sub>-directions, denoted by <i>n</i><sub><i>a</i><i>v</i><i>y</i></sub> and <i>x</i>, respectively. As a special case, we define a 2D spatially chirped amplitude sinusoidal structure (SCASS), based on the transmission function of a conventional 2D amplitude sinusoidal grating, where the phase of the conventional grating is replaced by a desired chirped phase. The near-field diffraction from 2D SCASSs is studied using the angular (spatial) spectrum method. The Talbot distances for these gratings are determined and verified experimentally, showing that the intensity profiles at specific Talbot distances are highly dependent on the parameters <i>y</i>, <i>x</i>, <i>y</i>, <i>k</i><sub>x</sub>, <i>k</i><sub>y</sub>, and <i>n</i><sub><i>c</i><i>x</i></sub>. Furthermore, we formulated the near-field diffraction of a plane wave from 2D multiplicatively separable spatially chirped amplitude sinusoidal structures, considering the variability of spatial periods in both the <i>n</i><sub><i>c</i><i>y</i></sub>- and <i>n</i><sub><i>a</i><i>v</i><i>x</i></sub>-directions. In comparison with conventional 2D gratings, new, to our knowledge, and intriguing diffraction patterns are observed, such as sharp and smooth Gaussian-like intensity spots generated via the diffraction of the incident wave, with nearly diffraction-limited features but limited overall efficiency. These intensity spots depend on the characteristic parameters of the structure. By carefully manipulating the <i>n</i><sub><i>a</i><i>v</i><i>y</i></sub> parameters, we have the ability to generate maximum intensity peaks within these 2D SCASSs, which are ","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1434-1448"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113469","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Semi-analytic theory of high-efficiency multilayer dielectric gratings. 高效多层介质光栅的半解析理论。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.568254
Lifeng Li

A semi-analytic theory of multilayer dielectric gratings (MLDGs) is presented. Analytic formulas for the -1st-order diffraction efficiency of an MLDG being 100% and greater than a preset value are given in terms of the scattering matrix elements of the top surface-relief grating (TG). The important role of the combined reflection phases is highlighted. The need to secure high reflectances of the multilayer stack at the two angles of incidence below the TG and the need to supply a sufficient number of aperiodic layers in the multilayer substrate for phase matching are emphasized. Three numerical examples of 100% efficient MLDGs, obtained without optimizing the TG, are presented, illustrating the accuracy and generality of the theory.

提出了多层介质光栅(mldg)的半解析理论。根据顶面缓释光栅(TG)的散射矩阵元素,给出了MLDG -1级衍射效率为100%且大于预设值的解析公式。强调了组合反射相位的重要作用。强调了在TG以下的两个入射角处确保多层堆叠的高反射率的必要性,以及在多层衬底中提供足够数量的非周期层以进行相位匹配的必要性。本文给出了三个在不优化热重的情况下获得100%效率的mldg的数值例子,说明了该理论的准确性和通用性。
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引用次数: 0
Spectroscopic analysis of volumetric OCT data for the automated measurement of scatterer size. 用于散射体尺寸自动测量的体积OCT数据的光谱分析。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.569122
Erin C O'Kane, Wan Wang, Robert E Highland, David A Miller, Adam Wax

Spectroscopic optical coherence tomography enables an accurate estimation of scatterer size by computing the correlation distance (CD) function. For calibration and accuracy verification, polystyrene spheres are commonly used as size standards. However, anomalies have been observed when using the CD function to analyze spherical scatterers, which we link to multiple scattering. We have developed a robust, automated algorithm to calculate the size of hundreds of scatterers within a volumetric OCT image while accounting for the effects of multiple scattering. We measured 5.1, 7.7, and 11.3 µm polystyrene beads suspended in collagen hydrogel, agarose, and polydimethylsiloxane, which resulted in average diameters in agreement with the theoretical size to within ±λ/2, using this analysis approach. Accurately accounting for these multiple scattering effects is crucial for a robust calibration, and these measurements point the way toward analyzing the nuclear size of cells throughout a 3D tissue volume.

光谱光学相干层析成像可以通过计算相关距离(CD)函数来精确估计散射体的大小。为了校准和精度验证,通常使用聚苯乙烯球作为尺寸标准。然而,当使用CD函数分析球面散射体时,发现了异常现象,我们将其与多重散射联系起来。我们开发了一种鲁棒的自动化算法来计算体积OCT图像中数百个散射体的大小,同时考虑多重散射的影响。我们测量了悬浮在胶原蛋白水凝胶、琼脂糖和聚二甲基硅氧烷中的5.1、7.7和11.3µm聚苯乙烯微球,结果表明平均直径与理论尺寸一致,在±λ/2范围内。准确地计算这些多重散射效应对于稳健的校准至关重要,这些测量为分析整个3D组织体积中细胞的核大小指明了方向。
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引用次数: 0
Borel summability of spectral nonparaxial perturbative series. 谱非旁轴摄动级数的Borel可和性。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-09-01 DOI: 10.1364/JOSAA.567341
Riccardo Borghi

Fifty years after its introduction, the perturbative approach conceived by Lax et al. [Phys. Rev. A11, 1365 (1975)10.1103/PhysRevA.11.1365] to solve Maxwell's equations remains widely used, despite its inherent divergence in the physical space. Through a vectorial analysis of the LLM algorithm carried out within the spatial frequency domain, it is here shown how each single term of the asymptotic expansion of a free-space propagated coherent light field represents the outcome of a suitable linear filter fed by the boundary field. In this way, since the Fourier transform operator naturally uncouples the roles of the boundary condition and of the propagation process, the decoding mechanism of the LLM scheme can be clearly unveiled. To this end, our main task is the exploration of the convergence features of the so-called spectral series. This is the spectral counterpart of the asymptotic series representation (in the physical space) provided by the LLM algorithm. Through a delicate asymptotic analysis, it is proved that the spectral series is uniformly convergent, within the homogeneous portion of the angular spectrum, to the Fourier transform of the coherent free-space propagator. On employing Borel summation together with analytical continuation, such a fundamental connection is then extended to the remaining evanescent part of the spectrum. In this way, it is rigorously proven that (i) exact free-space solutions of Maxwell's equations are completely encoded within their paraxial approximations and (ii) the Rayleigh-Sommerfeld coherent propagator is the generating function for all nonparaxial corrections iteratively obtained by the LLM algorithm, irrespective of the boundary condition.

在引入微扰方法50年后,Lax等人设想的微扰方法。尽管麦克斯韦方程组在物理空间中存在固有的发散性,但求解麦克斯韦方程组的方法仍然被广泛使用。通过在空间频域内进行的LLM算法的矢量分析,这里显示了自由空间传播相干光场的渐近展开的每一项如何表示由边界场馈送的合适线性滤波器的结果。这样,由于傅里叶变换算子自然地解耦了边界条件和传播过程的作用,可以清楚地揭示LLM方案的解码机制。为此,我们的主要任务是探索所谓谱级数的收敛性特征。这是LLM算法提供的(在物理空间中)渐近级数表示的谱对应。通过细致的渐近分析,证明了谱级数在角谱的齐次部分内一致收敛于相干自由空间传播子的傅里叶变换。在使用Borel求和和解析延拓的同时,这种基本联系被推广到谱的剩余倏逝部分。通过这种方式,严格证明了(i)麦克斯韦方程组的精确自由空间解完全编码在其近轴近似内,(ii) Rayleigh-Sommerfeld相干传播子是由LLM算法迭代获得的所有非近轴修正的生成函数,而与边界条件无关。
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引用次数: 0
Scattering by nanoplasmonic mesoscale assemblies. 纳米等离子体中尺度组件的散射。
IF 1.5 3区 物理与天体物理 Q3 OPTICS Pub Date : 2025-08-01 DOI: 10.1364/JOSAA.560629
Md Imran Khan, Sayantani Ghosh, Arnold D Kim

The flexibility and versatility of nano-assembled plasmonic structures provide platforms for mesoscale tunable optical modulation. Our recently developed model for these nano-assembled plasmonic structures is composed of a dielectric spherical core surrounded by a concentric spherical shell containing a random distribution of gold nanoparticles (AuNPs). This model provides a useful platform for studying the role of a controlled amount of disorder on scattering by a particle. In that context, we explore the angular distribution of scattered light for different sizes (5-20 nm) and filling fractions (0.1-0.3) of the AuNPs in the coatings. The simulations reveal that the coating of AuNPs redistributes power in a way that suppresses angular side lobes, thereby guiding the scattered power preferentially in the forward direction. These results highlight that, with the ability to tune both the spatial and spectral aspects of the scattering profile, these coated structures may serve as a platform for a variety of applications, including passive cloaking and high-resolution imaging.

纳米组装等离子体结构的灵活性和多功能性为中尺度可调谐光调制提供了平台。我们最近开发的这些纳米组装等离子体结构模型是由一个介电球核和一个含有随机分布的金纳米颗粒(AuNPs)的同心球壳包围组成的。该模型为研究受控无序量对粒子散射的作用提供了一个有用的平台。在此背景下,我们研究了涂层中不同尺寸(5-20 nm)和填充分数(0.1-0.3)的aunp的散射光角分布。模拟结果表明,纳米纳米粒子的涂层以抑制角侧叶的方式重新分配功率,从而优先引导散射功率向前方向。这些结果强调,由于能够调整散射剖面的空间和光谱方面,这些涂层结构可以作为各种应用的平台,包括被动隐身和高分辨率成像。
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引用次数: 0
期刊
Journal of The Optical Society of America A-optics Image Science and Vision
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