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.
{"title":"Deep learning-based conjugate orbital angular momentum interferometry for in-plane displacement measurement.","authors":"Qinyu Li, Zhanwu Xie, Yuanheng Shi, Wei Xia, Dongmei Guo","doi":"10.1364/JOSAA.570239","DOIUrl":"https://doi.org/10.1364/JOSAA.570239","url":null,"abstract":"<p><p>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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1376-1384"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113478","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}
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.
{"title":"Two-dimensional light beam shape characterization using interferometric closure amplitudes.","authors":"Nithyanandan Thyagarajan, Bojan Nikolic, Christopher L Carilli, Laura Torino, Ubaldo Iriso","doi":"10.1364/JOSAA.568171","DOIUrl":"https://doi.org/10.1364/JOSAA.568171","url":null,"abstract":"<p><p>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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1261-1267"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113534","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}
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.
{"title":"Fringe visibility for pulsed digital holography with large optical path differences.","authors":"Samuel T Thurman, Anthony C Klee","doi":"10.1364/JOSAA.567877","DOIUrl":"https://doi.org/10.1364/JOSAA.567877","url":null,"abstract":"<p><p>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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1403-1416"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113496","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}
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.
{"title":"High-resolution dual-band triple-grating spectrometer for atmospheric CO<sub>2</sub> detection.","authors":"Hongling Yuan, Zhiwei Feng, Guo Xia, Hui Zhang, Yongqing Wei, Shunlong Shu","doi":"10.1364/JOSAA.563970","DOIUrl":"https://doi.org/10.1364/JOSAA.563970","url":null,"abstract":"<p><p>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 ±1<i>s</i><i>t</i>-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 <i>C</i><i>O</i><sub>2</sub> weak absorption spectra (1.556-1.576µ<i>m</i> and 1.578-1.598µ<i>m</i>) 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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1276-1284"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113521","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}
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.
{"title":"Optical spatiotemporal Fourier synthesis: tutorial.","authors":"Murat Yessenov, Ayman F Abouraddy","doi":"10.1364/JOSAA.566252","DOIUrl":"https://doi.org/10.1364/JOSAA.566252","url":null,"abstract":"<p><p>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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1295-1315"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113553","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}
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}
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.
{"title":"Semi-analytic theory of high-efficiency multilayer dielectric gratings.","authors":"Lifeng Li","doi":"10.1364/JOSAA.568254","DOIUrl":"https://doi.org/10.1364/JOSAA.568254","url":null,"abstract":"<p><p>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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1385-1395"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113574","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}
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.
{"title":"Spectroscopic analysis of volumetric OCT data for the automated measurement of scatterer size.","authors":"Erin C O'Kane, Wan Wang, Robert E Highland, David A Miller, Adam Wax","doi":"10.1364/JOSAA.569122","DOIUrl":"10.1364/JOSAA.569122","url":null,"abstract":"<p><p>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 ±<i>λ</i>/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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1344-1353"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC12859759/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113566","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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.
{"title":"Borel summability of spectral nonparaxial perturbative series.","authors":"Riccardo Borghi","doi":"10.1364/JOSAA.567341","DOIUrl":"https://doi.org/10.1364/JOSAA.567341","url":null,"abstract":"<p><p>Fifty years after its introduction, the perturbative approach conceived by Lax <i>et al.</i> [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 <i>spectral series</i>. 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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 9","pages":"1268-1275"},"PeriodicalIF":1.5,"publicationDate":"2025-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145113491","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}
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.
{"title":"Scattering by nanoplasmonic mesoscale assemblies.","authors":"Md Imran Khan, Sayantani Ghosh, Arnold D Kim","doi":"10.1364/JOSAA.560629","DOIUrl":"https://doi.org/10.1364/JOSAA.560629","url":null,"abstract":"<p><p>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.</p>","PeriodicalId":17382,"journal":{"name":"Journal of The Optical Society of America A-optics Image Science and Vision","volume":"42 8","pages":"1244-1253"},"PeriodicalIF":1.5,"publicationDate":"2025-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144821898","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}