使用量热法和深度学习的ASTRA增强质子跟踪

Q3 Physics and Astronomy Instruments Pub Date : 2022-10-08 DOI:10.3390/instruments6040058
C. Jesús-Valls, M. Granado-González, T. Lux, T. Price, Federico Sánchez
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引用次数: 0

摘要

最近,我们提出了一个新的测距仪概念,名为ASTRA。ASTRA经过优化,可以在非常高的O(100MHz)速率下精确测量(优于1%)动能在几十到几百MeV范围内的质子的残余能量。这些综合性能旨在实现快速、高质量的质子计算机断层扫描(pCT),这对于正确评估质子束治疗中的治疗计划至关重要。尽管ASTRA是一台测距望远镜,但它也是一台量热计,为基于深度学习的增强跟踪可能性打开了大门。在这里,我们回顾了ASTRA的概念,并研究了一种利用量热法的替代跟踪方法。特别是,我们研究了ASTRA通过一种基于语义分割的新型跟踪方法来处理堆积质子的潜力,语义分割是一种在像素级执行分类的深度学习网络架构。
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Enhanced Proton Tracking with ASTRA Using Calorimetry and Deep Learning
Recently, we proposed a novel range detector concept named ASTRA. ASTRA is optimized to accurately measure (better than 1%) the residual energy of protons with kinetic energies in the range from tens to a few hundred MeVs at a very high rate of O(100 MHz). These combined performances are aimed at achieving fast and high-quality proton Computerized Tomography (pCT), which is crucial to correctly assessing treatment planning in proton beam therapy. Despite being a range telescope, ASTRA is also a calorimeter, opening the door to enhanced tracking possibilities based on deep learning. Here, we review the ASTRA concept, and we study an alternative tracking method that exploits calorimetry. In particular, we study the potential of ASTRA to deal with pile-up protons by means of a novel tracking method based on semantic segmentation, a deep learning network architecture that performs classification at the pixel level.
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来源期刊
Instruments
Instruments Physics and Astronomy-Instrumentation
CiteScore
2.60
自引率
0.00%
发文量
70
审稿时长
11 weeks
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