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Formation of Oriented MoS2 Nanowalls by Selective Laser Ablation and Their Properties 选择性激光烧蚀制备定向二硫化钼纳米壁及其性能
IF 0.7 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-18 DOI: 10.3103/S1068335625603711
A. B. Loginov, R. R. Ismagilov, N. R. Arutyunyan, I. V. Sapkov, E. D. Obraztsova, A. N. Chulkov

Films consisting of arrays of MoS2 crystallites (nanowalls), which are oriented perpendicular to the substrate, attract the attention of researchers as a promising material for creating photonic, optoelectronic, and sensor devices. The additional ordering of the structure of such layers by orientating nanowalls along a certain direction in the substrate plane allows creation of materials with unique characteristics. For their formation, we use the method of selective laser ablation of MoS2 films formed via deposition from the vapor phase and consisting of nanowalls on the surfaces of silicon substrates. The parameters of a laser pulse, which lead to the emergence of the maximum degree of ordering of nanowalls in the film, are determined. The photoluminescence (PL) and Raman scattering (RS) have been studied. In particular, the degree of polarization of PL and RS signals was determined as a function of the angle between a selected direction in the film plane and the polarization of exciting radiation. It was revealed that exactly nanowalls are responsible for the optical properties of such films but not the underlying film. The possible applications of the materials obtained using the selective ablation method in photonics are discussed.

由垂直于衬底的二硫化钼晶体阵列(纳米壁)组成的薄膜,作为一种有前途的材料,在制造光子、光电和传感器器件方面引起了研究人员的注意。通过在衬底平面上沿一定方向定向纳米壁来对这些层的结构进行额外的排序,可以创造出具有独特特性的材料。对于它们的形成,我们使用选择性激光烧蚀的方法,由气相沉积形成的MoS2薄膜,由硅衬底表面的纳米壁组成。确定了导致薄膜中纳米壁出现最大有序度的激光脉冲参数。对其光致发光(PL)和拉曼散射(RS)进行了研究。特别地,PL和RS信号的极化程度被确定为薄膜平面上选定方向与激励辐射极化之间夹角的函数。结果表明,纳米壁对这种薄膜的光学特性起作用,而不是底层薄膜。讨论了选择性烧蚀法制备的材料在光子学中的应用前景。
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引用次数: 0
Spring Atmospheric Blockings in the Northern Hemisphere: Changes in Recent Decades (1992–2023) 北半球春季大气阻塞:近几十年的变化(1992-2023)
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-18 DOI: 10.3103/S0027134925700985
I. I. Mokhov, I. R. Eremin

This paper presents an analysis of spring atmospheric blockings (SAB) in the Northern Hemisphere (NH) for the period 1992–2023. The results of the analysis indicate a significant increase in blocking activity in the NH atmosphere in recent decades. This trend is observed against the background of a general increase in near-surface temperature in the NH during the spring seasons. The following SAB parameters were used in the study: quantity, average duration, total duration, intensity, and size. Statistically significant increases were obtained for the total duration, quantity, and size of SAB, associated with an increase in the average spring near-surface temperature in the NH.

本文对1992-2023年北半球春季大气阻塞(SAB)进行了分析。分析结果表明近几十年来北半球大气中的阻塞活动显著增加。这一趋势是在春季北半球近地表温度普遍升高的背景下观测到的。研究中使用了以下SAB参数:数量、平均持续时间、总持续时间、强度和大小。在统计上,SAB的总持续时间、数量和大小都有显著增加,这与北半球春季平均近地表温度的增加有关。
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引用次数: 0
Implications of a Weakening N = 126 Shell Closure Away from Stability for r-Process Astrophysical Conditions 远离稳定的弱N = 126壳封闭对r过程天体物理条件的影响
IF 4.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-12-18 DOI: 10.1016/j.physletb.2025.140109
Mengke Li, Gail C. Mclaughlin, Rebecca Surman
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引用次数: 0
Intra-night optical polarization monitoring of blazars 夜间耀变体的光偏振监测
IF 6.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-12-18 DOI: 10.1051/0004-6361/202557558
Aristeidis Polychronakis, Ioannis Liodakis, Anastasia Glykopoulou, Dmitry Blinov, Iván Agudo, Svetlana G. Jorstad, Beatriz Agís-González, Sara Capecchiacci, Alberto Floris, Sebastian Kielhmann, John A. Kypriotakis, Dimitrios A. Langis, Nikos Mandarakas, Karan Pal, Francisco J. Aceituno, Giacomo Bonnoli, Víctor Casanova, Gabriel Emery, Juan Escudero Pedrosa, Jorge Otero-Santos, Daniel Morcuende, Alfredo Sota, Vilppu Piirola
Blazars are known for their extreme variability across the electromagnetic spectrum. Variability at very short timescales can allow us to discriminate between competing models. This is particularly true for polarization variability, which allows us to probe particle acceleration and high-energy emission models in blazars. Here we present results from the first pilot study of intra-night optical polarization monitoring conducted using RoboPol at the Skinakas Observatory; these results are supplemented by observations from the Calar Alto, Perkins, and Sierra Nevada observatories. Our results show that while variability patterns can vary widely between sources, variability on timescales as short as minutes is prevalent in blazar jets. The amplitudes of the variations are typically small, a few percent for the polarization degree and less than 20° for the polarization angle, pointing to a significant contribution to the optical emission from a turbulent magnetic field component. The overall stability of the polarization angle over time points to a preferred magnetic field orientation.
耀变体以其在电磁波谱上的极端可变性而闻名。在非常短的时间尺度上的变异性可以让我们区分不同的模型。偏振变异性尤其如此,它使我们能够探测耀变体中的粒子加速和高能发射模型。在这里,我们介绍了在斯基纳卡斯天文台使用RoboPol进行的夜间光偏振监测的第一次试点研究的结果;这些结果由Calar Alto, Perkins和Sierra Nevada天文台的观测结果补充。我们的研究结果表明,虽然不同来源的变异性模式差异很大,但短至几分钟的变异性在耀变体喷流中很普遍。这种变化的幅度通常很小,偏振度的变化幅度为几个百分点,偏振角的变化幅度小于20°,这表明湍流磁场分量对光发射有重要贡献。极化角随时间的总体稳定性指向一个首选的磁场方向。
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引用次数: 0
SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis 用于光学和近红外光谱分析的跨平台Python GUI软件
IF 1.8 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-12-18 DOI: 10.1016/j.ascom.2025.101051
D. Gasparri , L. Morelli , U. Battino , J. Méndez-Abreu , A. de Lorenzo-Cáceres
The increasing availability of high-quality optical and near-infrared spectroscopic data, as well as advances in modelling techniques, have greatly expanded the scientific potential of spectroscopic studies. However, the software tools needed to exploit this potential often remain fragmented across multiple specialised packages, requiring scripting skills and manual integration to handle complex workflows. In this paper we present SPAN (SPectral ANalysis), a cross-platform, Python-based Graphical User Interface (GUI) software that integrates the essential steps of the modern spectroscopic workflow within a single, user-friendly environment. SPAN provides a coherent framework that unifies data preparation, spectral processing, and analysis tasks, using the pPXF software as its core engine for full spectral fitting. SPAN allows users to extract 1D spectra from FITS images and datacubes, perform spectral processing (e.g. Doppler correction, continuum modelling, denoising), and carry out detailed analyses, including equivalent width measurements, stellar and gas kinematics, and stellar population studies. It runs natively on Windows, Linux, macOS, and Android, and is fully task-driven, requiring no prior coding experience. We validate SPAN by comparing its output with existing pipelines and literature studies. By offering a flexible, accessible, and well integrated environment, SPAN simplifies and accelerates the spectral analysis workflow, while maintaining scientific accuracy.
高质量的光学和近红外光谱数据的不断增加,以及建模技术的进步,极大地扩展了光谱研究的科学潜力。然而,开发这种潜力所需的软件工具通常仍然分散在多个专门的软件包中,需要脚本技能和手动集成来处理复杂的工作流。在本文中,我们介绍了SPAN(光谱分析),一个跨平台的,基于python的图形用户界面(GUI)软件,它集成了现代光谱工作流程的基本步骤,在一个单一的,用户友好的环境中。SPAN提供了一个统一的框架,将数据准备、光谱处理和分析任务统一起来,使用pPXF软件作为其全光谱拟合的核心引擎。SPAN允许用户从FITS图像和数据库中提取1D光谱,进行光谱处理(例如多普勒校正,连续统建模,去噪),并进行详细分析,包括等效宽度测量,恒星和气体运动学以及恒星群研究。它本机运行在Windows、Linux、macOS和Android上,完全是任务驱动的,不需要之前的编码经验。我们通过将SPAN的输出与现有管道和文献研究进行比较来验证SPAN。通过提供灵活、易于访问和良好集成的环境,SPAN简化并加速了光谱分析工作流程,同时保持了科学的准确性。
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引用次数: 0
Effect of Birefringence of Electromagnetic Radiation in the Field of a Relativistically Rotating Pulsar or Magnetar within the Framework of Nonlinear Vacuum Electrodynamics 非线性真空电动力学框架下相对旋转脉冲星或磁星场中电磁辐射双折射效应
IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-18 DOI: 10.3103/S0027134925701061
M. S. Seidaliyeva, V. I. Denisov, I. P. Denisova

Within the framework of parameterized post-Maxwellian vacuum electrodynamics, the propagation of an X-ray and gamma radiation pulse through the electromagnetic field of a relativistically rotating pulsar is investigated. Expressions are obtained for the trajectory of this pulse and for the law of its motion from the point (mathbf{r}_{s}={x_{s},y_{s},z_{s}},) where at the moment of time (t=t_{s}) an X-ray or gamma-ray burst occurs, to the point (mathbf{r}_{d}={x_{s},y_{s},z_{d}},) where the detector of this radiation is located. In the case when the post-Maxwellian parameters of the theory differ, (eta_{1}neqeta_{2}), the time of nonlinear electrodynamic delay of electromagnetic signals carried by different normal modes is calculated. The change in the polarization state of the X-ray or gamma radiation pulse after passing through the electromagnetic field of a relativistically rotating pulsar is analyzed. The possibilities of observing the nonlinear effect of the electromagnetic field of a relativistically rotating pulsar on X-ray and gamma-ray pulses are discussed.

在参数化后麦克斯韦真空电动力学的框架下,研究了x射线和伽马辐射脉冲在相对旋转脉冲星电磁场中的传播。得到了这个脉冲的轨迹和它的运动规律的表达式,从点(mathbf{r}_{s}={x_{s},y_{s},z_{s}},),在这个时刻(t=t_{s})发生x射线或伽马射线暴,到点(mathbf{r}_{d}={x_{s},y_{s},z_{d}},),这个辐射的探测器所在的位置。在理论的后麦克斯韦参数不同的情况下,(eta_{1}neqeta_{2})计算了不同正态模态承载的电磁信号的非线性电动力延迟时间。分析了x射线或伽马射线脉冲穿过相对旋转脉冲星电磁场后偏振态的变化。讨论了观测相对旋转脉冲星电磁场对x射线和伽马射线脉冲非线性效应的可能性。
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引用次数: 0
Influence of Pumping Parameters on the Maximum Length of Unrepeatered Communication Lines with Erbium-Doped Remote Optically Pumped Amplifiers 泵送参数对远端掺铒光泵浦放大器非中继通信线路最大长度的影响
IF 0.7 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-18 DOI: 10.3103/S1068335625603723
M. O. Zhulidova, O. E. Nanii, I. I. Shikhaliev, V. N. Treschikov

The paper examines the influence of the delivery scheme and spectral characteristics of remote optically pumped amplifiers (ROPA) on the maximum length of unrepeatered communication lines. It is established that in the backward ROPA (BROPA) scheme, signal amplification due to stimulated Raman scattering (SRS) in the working telecommunication fiber causes a small shift (~5 nm) of optimal pump wavelength toward shorter wavelengths relative to the maximum gain-to-noise ratio of the erbium-doped fiber (max[GainEDFpump)/NFEDFpump)]). The pump delivery through the working fiber in the case of BROPA has been found to increase the transmission distance due to additional signal amplification caused by SRS and the absence of significant depletion of pump power delivered to the erbium-doped fiber. Conversely, when the signal and pump propagate forward (FROPA) along the working fiber, the pump power decays due to SRS, which makes its delivery via an additional fiber more efficient. It has been determined that for a pump spectral width exceeding 4 GHz, the effect of the Mandelstam-Brillouin stimulated scattering on pump power can be disregarded. Approximate formulas are derived for calculating the dependence of the BROPA gain on the microparameters of the erbium-doped fiber, the signal spectrum, and on the delivered power and pump spectrum subject to the amplified spontaneous emission.

本文研究了远程光泵浦放大器(ROPA)的传输方案和频谱特性对非中继通信线路最大长度的影响。在反向ROPA (BROPA)方案中,由于受激拉曼散射(SRS)在工作的电信光纤中引起的信号放大,导致最佳泵浦波长相对于掺铒光纤的最大增益噪声比(max[GainEDF(λ泵浦)/NFEDF(λ泵浦)]向较短波长偏移较小(~5 nm)。在BROPA的情况下,通过工作光纤的泵送已经被发现增加了传输距离,因为SRS引起了额外的信号放大,并且泵送到掺铒光纤的功率没有明显的损耗。相反,当信号和泵浦沿着工作光纤向前传播(FROPA)时,由于SRS,泵浦功率会衰减,这使得其通过额外的光纤传输更有效。对于超过4 GHz的泵浦谱宽,可以忽略曼德尔斯塔姆-布里渊受激散射对泵浦功率的影响。导出了计算BROPA增益与掺铒光纤微参数、信号频谱、输出功率和自发发射放大后的泵浦光谱的关系的近似公式。
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引用次数: 0
Low-stress MOCVD-grown 15 μm GaN layers on 200 mm engineered substrates with minimal wafer bow 低应力mocvd生长的15 μm GaN层在200毫米的工程衬底上以最小的晶圆弯曲
IF 4 2区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2025-12-18 DOI: 10.1063/5.0312962
Kwang Jae Lee, Jawad Hadid, Sourish Banerjee, Thomas Nuytten, Ravikiran Lingaparthi, Herwig Hahn, Sebastian M. J. Beer, Md Arif Khan, Karen Geens, Stefaan Decoutere, Robert Langer, Anurag Vohra
Gallium nitride is increasingly recognized as a leading material for power and radio frequency applications, due to its unique electronic properties. However, the phenomenon of wafer bow and warpage during GaN growth on heterogeneous substrates presents significant challenges for vertical-type GaN devices with increasing drift layer thickness (for high voltage applications, 1200 V and above) and substrate diameters scaling to 200 mm. In this study, we introduce a growth scheme in the metalorganic chemical vapor deposition of GaN on 200 mm “engineered” substrates from Qromis substrate technology, specifically to minimize the wafer bow for vertical GaN metal-oxide-semiconductor field-effect transistors featuring an 11.5 μm-thick drift layer, with an overall GaN stack of ∼15 μm. By systematically reducing the pressure during the growth of unintentionally doped GaN from 300 to 150 mbar on an Al0.3Ga0.7N buffer layer, the tensile stress induced during cooldown could be effectively compensated. This yields an overall low residual stress of the thick ∼15 μm epitaxially grown GaN layers on the engineered Qromis substrate technology® substrate.
氮化镓由于其独特的电子特性,越来越被认为是电力和射频应用的主要材料。然而,在异质衬底上生长GaN时,晶圆弯曲和翘曲现象对垂直型GaN器件提出了重大挑战,因为漂移层厚度(用于高压应用,1200v及以上)和衬底直径缩放到200mm。在这项研究中,我们介绍了一种在200毫米Qromis衬底技术的“工程”衬底上金属有机化学气相沉积GaN的生长方案,特别是为了最小化具有11.5 μm厚漂移层的垂直GaN金属氧化物半导体场效应晶体管的晶圆弯曲,总体GaN堆叠为~ 15 μm。通过在Al0.3Ga0.7N缓冲层上系统地将无意掺杂GaN生长过程中的压力从300降低到150 mbar,可以有效地补偿冷却过程中引起的拉应力。这在工程Qromis衬底技术®衬底上产生了厚~ 15 μm外延生长GaN层的整体低残余应力。
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引用次数: 0
Thick brane in Palatini formalism with a non-minimally coupled bulk scalar field 具有非最小耦合本体标量场的Palatini形式中的厚膜
IF 3.5 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-12-18 DOI: 10.1088/1361-6382/ae272f
Tahereh Azizi and Mojtaba Alimoradi
We study a thick brane scenario within the Palatini formulation of gravity, where the metric and affine connection are treated as independent variables. By introducing a non-minimal coupling between a bulk scalar field and the Ricci scalar, we obtain analytic solutions under a flat, four-dimensional Poincaré-invariant metric with a kink-like scalar configuration. The warp factor exhibits a bell-shaped profile, while the scalar potential forms a symmetric volcano-like structure, characteristic of a finite-thickness brane. The corresponding energy density is regular and localized, featuring a central peak with symmetrically placed negative minima. Through the analysis of linear tensor perturbations, we derive a Schrödinger-like equation with supersymmetric factorization, ensuring the absence of tachyonic modes and thus the stability of the background configuration. The effective potential also takes a volcano-like form that supports a localized graviton zero mode, confirming the recovery of four-dimensional gravity on the brane. A numerical study of the massive Kaluza–Klein spectrum reveals the progressive delocalization of massive modes into the bulk. Our results demonstrate a stable and physically consistent thick brane configuration within the Palatini gravity framework, offering new insights into gravity localization and braneworld phenomenology.
我们研究了帕拉蒂尼重力公式中的厚膜场景,其中度规和仿射连接被视为独立变量。通过引入量标量场与Ricci标量之间的非极小耦合,我们得到了具有弯曲标量形的平面四维poincar不变度量下的解析解。经度因子呈钟形轮廓,而标量势形成对称的火山状结构,具有有限厚度膜的特征。相应的能量密度是规则的和局域的,具有中心峰和对称放置的负极小值。通过对线性张量微扰的分析,导出了一个超对称分解的Schrödinger-like方程,保证了超对称模的不存在,从而保证了背景构型的稳定性。有效势也采取类似火山的形式,支持局域引力子零模式,证实了膜上四维引力的恢复。对质量Kaluza-Klein谱的数值研究揭示了质量模态向体的逐步离域。我们的研究结果在Palatini重力框架内展示了一个稳定的、物理上一致的厚膜结构,为重力局域化和膜世界现象学提供了新的见解。
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引用次数: 0
Absolute measurement of absorbed dose in water for 125I brachytherapy seeds 125I近距离放射治疗种子在水中吸收剂量的绝对测量
IF 2.2 3区 物理与天体物理 Q2 NUCLEAR SCIENCE & TECHNOLOGY Pub Date : 2025-12-18 DOI: 10.1016/j.radmeas.2025.107594
Zhong-Bin Hang , Chuan-Feng Liu , Yan Zhang , Zi-Wei Liang , Hai Hu , Tian-Tian Zhang , Yun-Tao Liu , Ming-Zhe Song , Ke-Xin Wei , Lin Qin , Xi-Mei Wang , Zuo-Xiang He

Background:

In the clinical application of brachytherapy, the relevant quantities of brachytherapy seed strength must be converted into absorbed dose at a reference depth of 1 cm in water. The current method of obtaining the absorbed dose in water is based on the air kerma strength and dose rate constant, which has an uncertainty of more than 10% (k=2), potentially affecting cancer treatment outcomes.

Purpose:

To ensure accurate dosimetry for 125I brachytherapy seeds, an extrapolation chamber embedded in the water-equivalent material was designed and manufactured to measure the absorbed dose in water directly.

Methods:

The mathematical model for determining the absorbed dose in water is based on radiation transport theory, where the key term conversion factor C(xi+1,xi) is determined using the Monte Carlo (MC) methods. In this paper, the basic structure, the measurement method, and the MC simulation of the extrapolation chamber are described. The dose rate constant of the model 6711 125I brachytherapy seed was obtained using three methods (experimental measurement, MC simulation, and AAPM recommended values), and the results was compared and analyzed.

Results:

The absorbed dose in water of the model 6711 125I brachytherapy seed was determined, and after repeated measurements and uncertainty evaluation, the result was 12.39 mGy/h, with an uncertainty of 3.5% (k=2). In addition, the brachytherapy seed was calibrated using an absolute measurement device for the air kerma strength, and its dose rate constant was calculated, which was in good agreement with both the AAPM-recommended values and MC simulated values.

Conclusions:

We successfully developed an absolute measurement device for the absorbed dose in water, which reduced the measurement uncertainty for 125I brachytherapy seeds and achieved dose accuracy for external radiotherapy. This study contributes to the establishment of primary standards for the absorbed dose in water of 125I brachytherapy seeds.
背景:在近距离放射治疗的临床应用中,必须在水中参考深度1cm处将相关量的近距离放射治疗种子强度转换为吸收剂量。目前获取水中吸收剂量的方法是基于空气可汗强度和剂量率常数,其不确定度大于10% (k=2),可能影响癌症治疗效果。目的:为保证125I近距离放射治疗种子剂量测定的准确性,设计并制造了嵌入水当量材料的外推室,用于直接测量125I近距离放射治疗种子在水中的吸收剂量。方法:确定水中吸收剂量的数学模型基于辐射输运理论,其中关键项转换因子C(xi+1,xi)采用蒙特卡罗(MC)方法确定。本文介绍了外推室的基本结构、测量方法和MC模拟。采用实验测量、MC模拟和AAPM推荐值三种方法获得6711 125I型近距离放射治疗种子的剂量率常数,并对结果进行比较分析。结果:测定了6711 125I模型近距离放疗种子在水中的吸收剂量,经过反复测量和不确定度评定,结果为12.39 mGy/h,不确定度为3.5% (k=2)。此外,使用空气粒子强度绝对测量装置对近距离治疗粒子进行校准,并计算其剂量率常数,与aapm推荐值和MC模拟值吻合较好。结论:研制成功的水中吸收剂量绝对测量装置,降低了125I近距离放射治疗粒子的测量不确定度,达到了体外放疗的剂量准确性。本研究有助于建立125I近距离放射治疗种子在水中吸收剂量的初步标准。
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引用次数: 0
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