Tracker-in-Calorimeter (TIC) Project: A Calorimetric New Solution for Space Experiments

Q3 Physics and Astronomy Instruments Pub Date : 2022-09-26 DOI:10.3390/instruments6040052
Gabriele Bigongiari , Oscar Adriani , Giovanni Ambrosi , Philipp Azzarello , Andrea Basti , E. Berti, Bruna Bertucci , Lorenzo Bonechi , Massimo Bongi , Sergio Bottai , Mirko Brianzi , P. Brogi, Guido Castellini , Enrico Catanzani , Caterina Checchia , Raffaello D’Alessandro , Sebastiano Detti , Matteo Duranti , Noemi Finetti , Valerio Formato , Maria Ionica , Paolo Maestro , Fernando Maletta , Pier Simone Marrocchesi , Nicola Mori , Lorenzo Pacini , Paolo Papini , S. Ricciarini, Gianluigi Silvestre , Piero Spillantini , O. Starodubtsev, F. Stolzi, Jung Eun Suh , Arta Sulaj , A. Tiberio, Elena Vannuccini 
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Abstract

A space-based detector dedicated to measurements of γ-rays and charged particles has to achieve a balance between different instrumental requirements. A good angular resolution is necessary for the γ-rays, whereas an excellent geometric factor is needed for the charged particles. The tracking reference technique of γ-ray physics is based on a pair-conversion telescope made of passive material (e.g., tungsten) coupled with sensitive layers (e.g., silicon microstrip). However, this kind of detector has a limited acceptance because of the large lever arm between the active layers, needed to improve the track reconstruction capability. Moreover, the passive material can induce fragmentation of nuclei, thus worsening charge reconstruction performances. The Tracker-In-Calorimeter (TIC) project aims to solve all these drawbacks. In the TIC proposal, the silicon sensors are moved inside a highly-segmented isotropic calorimeter with a couple of external scintillators dedicated to charge reconstruction. In principle, this configuration has a good geometrical factor, and the angle of the γ-rays can be precisely reconstructed from the lateral profile of the electromagnetic shower sampled, at different depths in the calorimeter, by silicon strips. The effectiveness of this approach has been studied with Monte Carlo simulations and validated with beam test data of a small prototype.
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跟踪量热计(TIC)项目:空间实验的量热新解决方案
专门用于测量γ射线和带电粒子的天基探测器必须在不同的仪器要求之间取得平衡。对γ射线来说,良好的角分辨率是必要的,而对带电粒子来说,则需要良好的几何因子。γ射线物理的跟踪参考技术是基于由无源材料(如钨)与敏感层(如硅微带)耦合制成的对转换望远镜。然而,由于有源层之间的杠杆臂较大,这种探测器的接受度有限,需要提高航迹重建能力。此外,钝化材料会导致原子核破碎,从而使电荷重建性能恶化。热量计跟踪器(TIC)项目旨在解决所有这些缺点。在TIC方案中,硅传感器被移动到一个高度分段的各向同性量热计中,有一对外部闪烁体专门用于电荷重建。原理上,这种结构具有良好的几何因子,可以用硅条精确地从量热计中不同深度处采样的电磁雨的侧向剖面上重建γ射线的角度。通过蒙特卡罗仿真研究了该方法的有效性,并用小型样机的波束试验数据验证了该方法的有效性。
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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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