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A new beam monitor at NFS/SPIRAL2 based on position-sensitive PPACs detecting fission fragments from 238U(n,f) 基于位置敏感PPACs探测238U(n,f)裂变碎片的新型NFS/SPIRAL2束流监测仪
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-31 DOI: 10.1016/j.nima.2025.171251
D. Ramos , X. Ledoux , L. Audouin , G. Fremont , P. Gangnant , J.C. Foy , C. Le Naour , M. Maloubier
A new experimental setup has been installed at the Time-Of-Flight area of the Neutrons For Science facility (NFS) at GANIL/SPIRAL2 for neutron beam monitoring. This setup consists of an array of Position-Sensitive Parallel-Plate Avalanche Counters (PS-PPACs) that detects both fission fragments in coincidence from secondary neutron-induced fission reactions in several 238U targets. The neutron energy is determined on an event-by-event basis using the Time-of-Flight method, and the reaction point within the U targets is reconstructed, enabling the measurement of the neutron beam flux and beam profile. The high transparency of the setup allows it to operate in parallel with other experiments running at NFS, thus providing an in-beam monitor of the neutron intensity. In this work, we report on the characteristics of this new setup, its operating principle, and the first results obtained using the high-intensity white-spectrum neutron beam at NFS. This beam is produced via reactions between a primary 40-MeV deuteron beam, accelerated in the SPIRAL2 LINAC, and a 8 mm-thick rotating beryllium converter target.
在GANIL/SPIRAL2的中子科学设施(NFS)的飞行时间区域安装了一个新的实验装置,用于中子束监测。该装置由一系列位置敏感平行板雪崩计数器(PS-PPACs)组成,该计数器可以在几个238U靶中检测二次中子诱导的裂变反应中同时发生的裂变碎片。利用飞行时间法逐次确定中子能量,重构U靶内的反应点,实现中子束流通量和束流剖面的测量。高透明度的设置允许它与在NFS运行的其他实验并行运行,从而提供中子强度的束内监测。在这项工作中,我们报告了这种新装置的特点,它的工作原理,以及在NFS使用高强度白谱中子束获得的第一个结果。该光束是通过在SPIRAL2直线加速器中加速的40 mev氘核束与8 mm厚的旋转铍转化器靶体之间的反应产生的。
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引用次数: 0
Characterization of FBK NUV-HD-Cryo SiPMs near LHe temperature 近LHe温度下FBK NUV-HD-Cryo SiPMs的表征
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-31 DOI: 10.1016/j.nima.2025.171256
Fengbo Gu , Junhui Liao , Jiangfeng Zhou , Meiyuanan Ma , Zhuo Liang , Guangpeng An , Zhaohua Peng , Jian Zheng , Lifeng Zhang , Lei Zhang , Yuanning Gao , Fabio Acerbi , Andrea Ficorella , Alberto Gola , Laura Parellada Monreal
Five FBK “NUV-HD-Cryo” SiPMs have been characterized at 7 K and 10 K, with 405 nm and 530 nm LED light, respectively. The dark count rate (DCR) was measured to be 1 Hz for the 100 mm2-size SiPMs, or 0.01 Hz/mm2, which is 7 orders lower than the DCR at room temperature (RT). Given the very low DCR at these cryogenic temperatures, we measured the SiPMs’ I–V curves with such a method: illuminated the SiPMs with weak light, which differs from the conventional measurements at RT. Then, we measured the photo-detection efficiency (PDE), after-pulse (AP), and cross-talk probabilities (CT) with a bias voltage ranging from overvoltage (OV) 5 to 11 V. At the OV interval (5 to 11 V), the PDE was between 20%–45%, and the AP and CT were both between 5% and 20%. With an OV higher than 10 V, the PDE would be 40%, and the AP and CT are 20%. Combining all of the measurements, we are confident that the SiPMs can be equipped as the photosensors on liquid helium detectors, including but not limited to the time projection chambers, which we have proposed in hunting for low-mass dark matter directly and beyond.
5个FBK“NUV-HD-Cryo”SiPMs分别在7 K和10 K, 405 nm和530 nm LED光下进行了表征。暗计数率(DCR)测量为~ 100 mm2尺寸的SiPMs为~ 1 Hz,或0.01 Hz/mm2,比室温(RT)下的DCR低~ 7个数量级。考虑到低温下的DCR非常低,我们采用以下方法测量了SiPMs的I-V曲线:用不同于常规rt测量的弱光照射SiPMs,然后在过电压(OV) 5至11 V的偏置电压范围内测量了光探测效率(PDE)、后脉冲(AP)和串扰概率(CT)。在OV期(5 ~ 11v), PDE在20% ~ 45%之间,AP和CT均在~ 5% ~ ~ 20%之间。OV大于10 V时,PDE≥40%,AP和CT为~ 20%。综合所有的测量结果,我们相信sipm可以作为液氦探测器上的光传感器,包括但不限于时间投影室,我们已经提出了寻找低质量暗物质的直接和更远的地方。
{"title":"Characterization of FBK NUV-HD-Cryo SiPMs near LHe temperature","authors":"Fengbo Gu ,&nbsp;Junhui Liao ,&nbsp;Jiangfeng Zhou ,&nbsp;Meiyuanan Ma ,&nbsp;Zhuo Liang ,&nbsp;Guangpeng An ,&nbsp;Zhaohua Peng ,&nbsp;Jian Zheng ,&nbsp;Lifeng Zhang ,&nbsp;Lei Zhang ,&nbsp;Yuanning Gao ,&nbsp;Fabio Acerbi ,&nbsp;Andrea Ficorella ,&nbsp;Alberto Gola ,&nbsp;Laura Parellada Monreal","doi":"10.1016/j.nima.2025.171256","DOIUrl":"10.1016/j.nima.2025.171256","url":null,"abstract":"<div><div>Five FBK “NUV-HD-Cryo” SiPMs have been characterized at 7 K and 10 K, with 405 nm and 530 nm LED light, respectively. The dark count rate (DCR) was measured to be <span><math><mo>∼</mo></math></span>1 Hz for the <span><math><mo>∼</mo></math></span>100 mm<span><math><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup></math></span>-size SiPMs, or 0.01 Hz/mm<span><math><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup></math></span>, which is <span><math><mo>∼</mo></math></span>7 orders lower than the DCR at room temperature (RT). Given the very low DCR at these cryogenic temperatures, we measured the SiPMs’ I–V curves with such a method: illuminated the SiPMs with weak light, which differs from the conventional measurements at RT. Then, we measured the photo-detection efficiency (PDE), after-pulse (AP), and cross-talk probabilities (CT) with a bias voltage ranging from overvoltage (OV) 5 to 11 V. At the OV interval (5 to 11 V), the PDE was between 20%–45%, and the AP and CT were both between <span><math><mo>∼</mo></math></span>5% and <span><math><mo>∼</mo></math></span>20%. With an OV higher than 10 V, the PDE would be <span><math><mo>≥</mo></math></span> 40%, and the AP and CT are <span><math><mo>∼</mo></math></span>20%. Combining all of the measurements, we are confident that the SiPMs can be equipped as the photosensors on liquid helium detectors, including but not limited to the time projection chambers, which we have proposed in hunting for low-mass dark matter directly and beyond.</div></div>","PeriodicalId":19359,"journal":{"name":"Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment","volume":"1084 ","pages":"Article 171256"},"PeriodicalIF":1.4,"publicationDate":"2025-12-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145883483","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
Bayesian optimization of combined ballistic neutron guides for the Elastic Diffuse Scattering spectrometer at CSNS CSNS弹性漫射光谱仪组合弹道中子波导的贝叶斯优化
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-30 DOI: 10.1016/j.nima.2025.171264
Pengfei Zhou , Zhirong Zeng , Zheng He , Xiao Wang , Li Lin , Ming Tang , Arsen Goukassov , Fangwei Wang , Tianjiao Liang , Erxi Feng
Designing neutron guide systems for single-crystal time-of-flight spectrometers requires balancing neutron flux, divergence, and compatibility with polarization optics. We present an automated optimization framework that integrates Monte Carlo simulations, Bayesian optimization, and a back-tracing method to systematically explore guide geometries under realistic engineering constraints. Applied to the Elastic Diffuse Spectrometer at the China Spallation Neutron Source, the framework evaluated four candidate designs to maximize flux while meeting divergence limits imposed by polarization and resolution requirements. Among the Bayesian-optimized configurations, the straight–elliptic guide offered the best overall balance of flux, divergence, and polarization performance.
设计单晶飞行时间光谱仪的中子导系统需要平衡中子通量、散度和与偏振光学的兼容性。我们提出了一个自动优化框架,该框架集成了蒙特卡罗模拟,贝叶斯优化和回溯方法,以系统地探索现实工程约束下的导向几何形状。应用于中国散裂中子源的弹性漫射光谱仪,该框架评估了四种候选设计,以最大限度地提高通量,同时满足极化和分辨率要求所施加的发散限制。在贝叶斯优化构型中,直椭圆导轨在通量、散度和极化性能方面的综合平衡效果最好。
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引用次数: 0
Measurement of decay heat in ISIS new-style TS-1 target ISIS新型TS-1靶体衰变热的测量
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-30 DOI: 10.1016/j.nima.2025.171263
D.J.S. Findlay, G.P. Škoro, J.P. Chapman, J.D. Moor, S.D. Gallimore
Measurements have been made of the decay heat generated within the new-style tantalum-clad ten-plate tungsten target for the First Target Station (TS-1) of the ISIS Spallation Neutron Source. The new-style target incorporates less tantalum than the old-style target, and the decay heat is correspondingly less. Measured values of decay heat agree well with values obtained from Monte Carlo calculations.
对ISIS散裂中子源第一靶站(TS-1)新型包钽十板钨靶内产生的衰变热进行了测量。新型靶材比旧式靶材含有更少的钽,相应的衰变热也更小。衰变热的测量值与蒙特卡罗计算值吻合得很好。
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引用次数: 0
Investigation of new collimator head material candidates for SuperKEKB and future electron/positron colliders SuperKEKB和未来电子/正电子对撞机新准直头材料候选材料的研究
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-30 DOI: 10.1016/j.nima.2025.171259
S. Terui , T. Ishibashi , M. Shirai , X. Jin , M. Yao , K. Shibata , T. Abe , N. Akita , A. Natochii , Q. Liu
Currently, SuperKEKB faces the challenge of sudden beam loss (SBL), which occurs with almost no prior warning, and the causes of SBL are not yet fully understood. A damaged collimator has a reduced ability to suppress beam background noise (BG) compared to an undamaged collimator. When BG suppression decreases, operation must be stopped and the collimator jaw replaced. Therefore, a robust collimator head material is required. In this study, we investigated the material properties of copper-carbide graphite (CuGr) as a candidate collimator head material for SuperKEKB and future electron/positron colliders in terms of its electrical conductivity in the high-frequency region, secondary electron yield, outgassing rate owing to photon-stimulated desorption, and amount of dust generated by the ultrasonic cleaning of CuGr. The results were compared with the simulation results of the beam background with CuGr. According to the study findings, CuGr can be effectively used as the collimator head material. Its use in SuperKEKB and future ring colliders is expected to contribute to stable accelerator operation.
目前,SuperKEKB面临着突如其来的光束损失(SBL)的挑战,这种情况几乎没有任何预警,而且SBL的原因尚未完全清楚。与未损坏的准直器相比,损坏的准直器抑制光束背景噪声(BG)的能力降低。当BG抑制下降时,必须停止操作并更换准直钳。因此,需要一种坚固的准直头材料。在这项研究中,我们研究了CuGr作为SuperKEKB和未来电子/正电子对撞机准直头材料的材料特性,包括其高频区的电导率、二次电子产率、光子激发解吸的放气率以及超声波清洗CuGr产生的粉尘量。将模拟结果与含CuGr光束背景的模拟结果进行了比较。研究结果表明,CuGr可以有效地用作准直头材料。它在SuperKEKB和未来环形对撞机中的应用有望为稳定的加速器运行做出贡献。
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引用次数: 0
Performance evaluation of a silicon carbide semiconductor-based neutron detector for neutron-gamma discrimination 基于碳化硅半导体的中子探测器中子- γ鉴别性能评价
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-30 DOI: 10.1016/j.nima.2025.171265
Kanta Nagai , Kei Aoyama , Takahito Suzuki , Takashi Nakamura , Hiroki Tanaka , Junya Ishii , Kenji Shimazoe
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引用次数: 0
Identification and online monitoring of experimental measurement states via Cuscore statistic 采用Cuscore统计方法对实验测量状态进行识别和在线监测
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-29 DOI: 10.1016/j.nima.2025.171267
Jichao Zhang , Baohua Sun , Isao Tanihata , Zilun Shen
We present a statistical method for detecting and analysing state changes in experimental measurements using the Cuscore statistic and its special case, the Centred Cuscore statistic. These statistics are designed to identify deviations in detector responses using sequential hypothesis testing relative to a defined reference state. Applications to charge-changing reaction experiments at the FRagment Separator facility at the GSI Helmholtz Centre for Heavy Ion Research, Germany, and the Second Radioactive Ion Beam Line in Lanzhou at the Institute of Modern Physics, China, demonstrate the ability of these tools to quantify state changes, identify the change point, and classify data segments based on measured states. For long-term online monitoring, we use the exponentially weighted moving average to continuously update computations, enabling the detection of successive changes. This method supports both real-time and post-experiment diagnostics and provides a robust approach for enhancing data integrity and experimental control in nuclear physics and related fields.
我们提出了一种统计方法,用于检测和分析实验测量中的状态变化,使用Cuscore统计量及其特殊情况,即中心Cuscore统计量。这些统计数据的目的是识别偏差的探测器响应使用序贯假设检验相对于一个定义的参考状态。应用于德国GSI亥姆霍兹重离子研究中心的碎片分离器设备和中国现代物理研究所兰州第二放射性离子束线的电荷变化反应实验,证明了这些工具量化状态变化、识别变化点和基于测量状态分类数据段的能力。对于长期在线监测,我们使用指数加权移动平均来不断更新计算,从而能够检测到连续的变化。该方法支持实时和实验后诊断,为增强核物理及相关领域的数据完整性和实验控制提供了一种可靠的方法。
{"title":"Identification and online monitoring of experimental measurement states via Cuscore statistic","authors":"Jichao Zhang ,&nbsp;Baohua Sun ,&nbsp;Isao Tanihata ,&nbsp;Zilun Shen","doi":"10.1016/j.nima.2025.171267","DOIUrl":"10.1016/j.nima.2025.171267","url":null,"abstract":"<div><div>We present a statistical method for detecting and analysing state changes in experimental measurements using the Cuscore statistic and its special case, the Centred Cuscore statistic. These statistics are designed to identify deviations in detector responses using sequential hypothesis testing relative to a defined reference state. Applications to charge-changing reaction experiments at the FRagment Separator facility at the GSI Helmholtz Centre for Heavy Ion Research, Germany, and the Second Radioactive Ion Beam Line in Lanzhou at the Institute of Modern Physics, China, demonstrate the ability of these tools to quantify state changes, identify the change point, and classify data segments based on measured states. For long-term online monitoring, we use the exponentially weighted moving average to continuously update computations, enabling the detection of successive changes. This method supports both real-time and post-experiment diagnostics and provides a robust approach for enhancing data integrity and experimental control in nuclear physics and related fields.</div></div>","PeriodicalId":19359,"journal":{"name":"Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment","volume":"1084 ","pages":"Article 171267"},"PeriodicalIF":1.4,"publicationDate":"2025-12-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145883486","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
Bayesian inference for total gamma clearance monitors: Accounting for both spatial and spectral information 总伽马间隙监测器的贝叶斯推断:考虑空间和光谱信息
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-29 DOI: 10.1016/j.nima.2025.171266
Eric Laloy, Md Moudud Hasan, Bart Rogiers, Wouter Broeckx, Arne Vandenbrande, An Bielen
This work introduces a novel Bayesian approach for interpreting total gamma clearance monitoring data. The approach integrates spatial and spectral information from the measurements with a surrogate efficiency model, all within a Bayesian inference framework, to estimate the spatial activity distribution across 15 subvolumes inside a 200-liter waste drum. When the 60Co/137Cs ratio is not known a priori, it can be jointly estimated alongside other variables of interest. Virtual and real mock-up experiments demonstrate that the method accurately identifies high-activity subvolumes and reconstructs the relative spatial activity distribution. Moreover, with reliable background count estimates, the total drum activity can be determined with a relative error below 10%. Tests on two real low-level waste drums, validated against HPGe-based gamma spectrometry, confirm a maximum relative error of 10%. Regarding inference of the 60Co/137Cs ratio, the approach correctly detects drums containing only 137Cs but underestimates the 60Co fraction when 60Co is present. Our proposed approach has also some practical limitations, mainly its reliance on prior knowledge of the drum’s filling level being close to 100% and, to a lesser extent, its underlying assumption of a constant density across the drum. Future work will aim to solve that issue by incorporating filling degree into the surrogate efficiency model.
这项工作引入了一种新的贝叶斯方法来解释总伽马清除率监测数据。该方法将测量的空间和光谱信息与替代效率模型结合起来,所有这些都在贝叶斯推理框架内,以估计200升废物桶内15个子体积的空间活动分布。当60Co/137Cs比率先验未知时,可以与其他感兴趣的变量一起共同估计。虚拟和真实模型实验表明,该方法能够准确识别高活度子体,并重建相对空间活度分布。此外,通过可靠的背景计数估计,可以以低于10%的相对误差确定总鼓活动。在两个真实的低放射性废物桶上进行的测试,与基于hpge的伽马能谱法进行了验证,证实了最大相对误差为10%。关于60Co/137Cs比率的推断,该方法正确地检测了仅含有137Cs的桶,但在60Co存在时低估了60Co的分数。我们提出的方法也有一些实际的局限性,主要是它依赖于对桶的填充水平接近100%的先验知识,在较小程度上,它的基本假设是桶的密度是恒定的。未来的工作将致力于通过将填充度纳入替代效率模型来解决这一问题。
{"title":"Bayesian inference for total gamma clearance monitors: Accounting for both spatial and spectral information","authors":"Eric Laloy,&nbsp;Md Moudud Hasan,&nbsp;Bart Rogiers,&nbsp;Wouter Broeckx,&nbsp;Arne Vandenbrande,&nbsp;An Bielen","doi":"10.1016/j.nima.2025.171266","DOIUrl":"10.1016/j.nima.2025.171266","url":null,"abstract":"<div><div>This work introduces a novel Bayesian approach for interpreting total gamma clearance monitoring data. The approach integrates spatial and spectral information from the measurements with a surrogate efficiency model, all within a Bayesian inference framework, to estimate the spatial activity distribution across 15 subvolumes inside a 200-liter waste drum. When the <span><math><mrow><msup><mrow></mrow><mrow><mi>60</mi></mrow></msup><mtext>Co</mtext></mrow></math></span>/<span><math><mrow><msup><mrow></mrow><mrow><mi>137</mi></mrow></msup><mtext>Cs</mtext></mrow></math></span> ratio is not known a priori, it can be jointly estimated alongside other variables of interest. Virtual and real mock-up experiments demonstrate that the method accurately identifies high-activity subvolumes and reconstructs the relative spatial activity distribution. Moreover, with reliable background count estimates, the total drum activity can be determined with a relative error below 10%. Tests on two real low-level waste drums, validated against HPGe-based gamma spectrometry, confirm a maximum relative error of 10%. Regarding inference of the <span><math><mrow><msup><mrow></mrow><mrow><mi>60</mi></mrow></msup><mtext>Co</mtext></mrow></math></span>/<span><math><mrow><msup><mrow></mrow><mrow><mi>137</mi></mrow></msup><mtext>Cs</mtext></mrow></math></span> ratio, the approach correctly detects drums containing only <span><math><mrow><msup><mrow></mrow><mrow><mi>137</mi></mrow></msup><mtext>Cs</mtext></mrow></math></span> but underestimates the <span><math><mrow><msup><mrow></mrow><mrow><mi>60</mi></mrow></msup><mtext>Co</mtext></mrow></math></span> fraction when <span><math><mrow><msup><mrow></mrow><mrow><mi>60</mi></mrow></msup><mtext>Co</mtext></mrow></math></span> is present. Our proposed approach has also some practical limitations, mainly its reliance on prior knowledge of the drum’s filling level being close to 100% and, to a lesser extent, its underlying assumption of a constant density across the drum. Future work will aim to solve that issue by incorporating filling degree into the surrogate efficiency model.</div></div>","PeriodicalId":19359,"journal":{"name":"Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment","volume":"1084 ","pages":"Article 171266"},"PeriodicalIF":1.4,"publicationDate":"2025-12-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145924696","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
Non-invasiveness evaluation of gas-sheet beam profile monitor: Observation of emittance reduction due to space-charge neutralization 气体片束剖面监测仪的非侵入性评价:由于空间电荷中和导致发射率降低的观察
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-27 DOI: 10.1016/j.nima.2025.171261
Ippei Yamada, Kunihiro Kojima, Motoki Chimura
A non-invasive beam profile monitor is indispensable for stable operation of a high-intensity particle accelerator. Two types based on beam-gas interaction have been developed at many institutes: the residual gas type and the gas injection type. The gas injection method enables a high-speed or accurate profile measurements due to the high secondary particle yield, in contrast to the residual gas type. However, gas injection may affect the beam quality, and a quantitative evaluation of non-invasiveness is essential. Charge exchange and phase-space distribution change of a negative hydrogen ion (H) beam induced by beam-gas interaction were quantified. The charge exchange was assessed through measurement of the beam current reduction, and the beam loss linearly increased with the injected gas flux, as consistent with the charge-exchange cross-section within a possible error range. Phase-space distributions with and without gas injection were measured, and the emittance reduced by about 5%, rather than increased due to scattering, when the beam line pressure was raised from 10−6 Pa to 10−3 Pa. An analytical approach and a particle-in-cell simulation revealed that the mitigation of the H beam’s space charge by ions generated in the beam-gas interaction induced the emittance reduction: a space-charge neutralization/compensation effect. In addition to the emittance reduction, the beam envelope exhibited a non-negligible lens effect due to the neutralization, and we devised a correction term including no arbitrariness under steady state of the neutralization.
为了保证高强度粒子加速器的稳定运行,非侵入式束流剖面监测仪是必不可少的。许多研究所发展了两种基于束气相互作用的类型:残余气型和注气型。与残余气体类型相比,由于二次颗粒产量高,注气方法可以实现高速或精确的剖面测量。然而,气体注入可能会影响光束质量,因此对非侵入性进行定量评估是必要的。定量研究了负氢离子(H -)束在束气相互作用下的电荷交换和相空间分布变化。电荷交换通过测量束流电流减少来评估,束流损耗随注入气体通量线性增加,在可能的误差范围内与电荷交换截面一致。当束线压力从10−6 Pa提高到10−3 Pa时,发射度并没有因为散射而增加,而是减少了约5%。分析方法和细胞内粒子模拟表明,在束-气相互作用中产生的离子对H -束空间电荷的减缓导致了发射度的降低:空间电荷中和/补偿效应。除了发射度降低外,由于中和,光束包络表现出不可忽略的透镜效应,我们设计了一个在中和稳态下不含任意性的校正项。
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引用次数: 0
Characterization of the light response of LYSO scintillator to α particles LYSO闪烁体对α粒子光响应的表征
IF 1.4 3区 物理与天体物理 Q3 INSTRUMENTS & INSTRUMENTATION Pub Date : 2025-12-27 DOI: 10.1016/j.nima.2025.171262
L. Gioacchini , A. Lega , R. Nicolaidis , F. Nozzoli
<div><div>Lutetium–yttrium oxyorthosilicate (LYSO) crystals are widely recognized as fast scintillators, valued for their high light output and robust mechanical properties, which make them well suited for high-energy physics and space applications despite their intrinsic radioactivity. Although the non-proportional light response of LYSO scintillators has been extensively studied, discrepancies remain among published measurements of the light-yield quenching at high ionization densities with different charged particles. We report a measurement of the light response of a LYSO scintillator to stopping <span><math><mi>α</mi></math></span> particles emitted by a <sup>241</sup>Am source performed in the laboratories of the University of Trento. A quenching factor, L/E <span><math><mo>=</mo></math></span> 0.075<span><math><mrow><mspace></mspace><mo>±</mo><mspace></mspace><mn>0</mn><mo>.</mo><mn>006</mn></mrow></math></span>, for <span><math><mrow><mn>3</mn><mo>.</mo><mn>7</mn><mspace></mspace><mspace></mspace><mi>MeV</mi></mrow></math></span> <span><math><mi>α</mi></math></span> particles has been inferred, in agreement with previous results obtained with He ions.</div><div>The time distribution of the scintillation decay has also been investigated, confirming the presence of two exponential components in the decay tail: <span><math><mrow><msub><mrow><mi>τ</mi></mrow><mrow><mtext>fast</mtext></mrow></msub><mo>=</mo><mn>23</mn><mo>.</mo><mn>3</mn><mspace></mspace><mo>±</mo><mspace></mspace><mn>0</mn><mo>.</mo><msup><mrow><mn>7</mn></mrow><mrow><mrow><mo>(</mo><mtext>stat.</mtext><mo>)</mo></mrow></mrow></msup><mo>±</mo><mn>0</mn><mo>.</mo><msup><mrow><mn>8</mn></mrow><mrow><mrow><mo>(</mo><mtext>syst.</mtext><mo>)</mo></mrow></mrow></msup><mspace></mspace><mspace></mspace><mi>ns</mi></mrow></math></span> and <span><math><mrow><msub><mrow><mi>τ</mi></mrow><mrow><mtext>slow</mtext></mrow></msub><mo>=</mo><mn>43</mn><mo>.</mo><mn>9</mn><mspace></mspace><mo>±</mo><mspace></mspace><mn>0</mn><mo>.</mo><msup><mrow><mn>5</mn></mrow><mrow><mrow><mo>(</mo><mtext>stat.</mtext><mo>)</mo></mrow></mrow></msup><mspace></mspace><mo>±</mo><mspace></mspace><mn>2</mn><mo>.</mo><msup><mrow><mn>3</mn></mrow><mrow><mrow><mo>(</mo><mtext>syst.</mtext><mo>)</mo></mrow></mrow></msup><mspace></mspace><mspace></mspace><mi>ns</mi></mrow></math></span>. The current measurement revealed that <span><math><mi>α</mi></math></span> scintillation pulses are faster than <span><math><mrow><mi>β</mi><mo>/</mo><mi>γ</mi></mrow></math></span> ones. This behavior is quantitatively parameterized by a difference in the amplitude of the two scintillation components: <span><math><mrow><msubsup><mrow><mi>A</mi></mrow><mrow><mtext>slow</mtext></mrow><mrow><mi>α</mi></mrow></msubsup><mo>=</mo><mrow><mo>(</mo><mn>48</mn><mo>.</mo><mn>7</mn><mspace></mspace><mo>±</mo><mspace></mspace><mn>3</mn><mo>.</mo><msup><mrow><mn>3</mn></mrow><mrow><mrow><mo>(</mo><mtext>stat.</mtext><mo>)</mo></mrow></mrow></ms
氧化硅酸镥钇(LYSO)晶体被广泛认为是快速闪烁体,因其高光输出和强大的机械性能而受到重视,这使得它们非常适合高能物理和空间应用,尽管它们具有固有的放射性。虽然LYSO闪烁体的非比例光响应已被广泛研究,但在不同带电粒子的高电离密度下,发表的光产率猝灭测量结果仍然存在差异。我们报道了在特伦托大学的实验室中进行的LYSO闪烁体对阻止241Am源发射的α粒子的光响应的测量。本文推导出3.7MeV α粒子的猝灭因子L/E = 0.075±0.006,与先前用He离子得到的结果一致。我们还研究了闪烁衰减的时间分布,证实了在衰减尾部存在两个指数分量:τfast=23.3±0.7(stat.)±0.8(syst.)ns和τslow=43.9±0.5(stat.)±2.3(syst.)ns。目前的测量表明,α闪烁脉冲比β/γ闪烁脉冲快。这种行为是由两个闪烁分量的振幅差异定量参数化的:Aslowα=(48.7±3.3(stat.)±15(syst.))%,显著小于Aslowβ/γ=(72.9±1.3(stat.)±3.5(system .))%。最后,建立最小线性模型Aslow=A0+A1LE,其中A0=(42±4(stat.)±4(syst.))%, A1=(35±5(stat.)±4(system .))%,被认为是为了验证用α和β/γ事件测量的LYSO光衰减时间的差异与闪烁猝灭效应有关的假设。
{"title":"Characterization of the light response of LYSO scintillator to α particles","authors":"L. Gioacchini ,&nbsp;A. Lega ,&nbsp;R. Nicolaidis ,&nbsp;F. Nozzoli","doi":"10.1016/j.nima.2025.171262","DOIUrl":"10.1016/j.nima.2025.171262","url":null,"abstract":"&lt;div&gt;&lt;div&gt;Lutetium–yttrium oxyorthosilicate (LYSO) crystals are widely recognized as fast scintillators, valued for their high light output and robust mechanical properties, which make them well suited for high-energy physics and space applications despite their intrinsic radioactivity. Although the non-proportional light response of LYSO scintillators has been extensively studied, discrepancies remain among published measurements of the light-yield quenching at high ionization densities with different charged particles. We report a measurement of the light response of a LYSO scintillator to stopping &lt;span&gt;&lt;math&gt;&lt;mi&gt;α&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; particles emitted by a &lt;sup&gt;241&lt;/sup&gt;Am source performed in the laboratories of the University of Trento. A quenching factor, L/E &lt;span&gt;&lt;math&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;/math&gt;&lt;/span&gt; 0.075&lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;mn&gt;006&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;, for &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mn&gt;3&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;mn&gt;7&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mi&gt;MeV&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; &lt;span&gt;&lt;math&gt;&lt;mi&gt;α&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; particles has been inferred, in agreement with previous results obtained with He ions.&lt;/div&gt;&lt;div&gt;The time distribution of the scintillation decay has also been investigated, confirming the presence of two exponential components in the decay tail: &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;τ&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mtext&gt;fast&lt;/mtext&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;23&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;mn&gt;3&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mn&gt;7&lt;/mn&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mtext&gt;stat.&lt;/mtext&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mn&gt;8&lt;/mn&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mtext&gt;syst.&lt;/mtext&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mi&gt;ns&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; and &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;τ&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mtext&gt;slow&lt;/mtext&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;43&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;mn&gt;9&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mn&gt;5&lt;/mn&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mtext&gt;stat.&lt;/mtext&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mn&gt;3&lt;/mn&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mtext&gt;syst.&lt;/mtext&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mi&gt;ns&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;. The current measurement revealed that &lt;span&gt;&lt;math&gt;&lt;mi&gt;α&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; scintillation pulses are faster than &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;β&lt;/mi&gt;&lt;mo&gt;/&lt;/mo&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; ones. This behavior is quantitatively parameterized by a difference in the amplitude of the two scintillation components: &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;msubsup&gt;&lt;mrow&gt;&lt;mi&gt;A&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mtext&gt;slow&lt;/mtext&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;α&lt;/mi&gt;&lt;/mrow&gt;&lt;/msubsup&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mn&gt;48&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;mn&gt;7&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mn&gt;3&lt;/mn&gt;&lt;mo&gt;.&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mn&gt;3&lt;/mn&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mtext&gt;stat.&lt;/mtext&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;/ms","PeriodicalId":19359,"journal":{"name":"Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment","volume":"1084 ","pages":"Article 171262"},"PeriodicalIF":1.4,"publicationDate":"2025-12-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145883485","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}
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Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment
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