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Compton polarimeter as a focal plane detector for hard X-ray telescope: sensitivity estimation with Geant4 simulations

机译:康普顿旋光仪作为硬X射线望远镜的焦平面检测器:Geant4模拟的灵敏度估计

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X-ray polarimetry can be an important tool for investigating various physical processes as well as their geometries at the celestial X-ray sources. However, X-ray polarimetry has not progressed much compared to the spectroscopy, timing and imaging mainly due to the extremely photon-hungry nature of X-ray polarimetry leading to severely limited sensitivity of X-ray polarimeters. The great improvement in sensitivity in spectroscopy and imaging was possible due to focusing X-ray optics which is effective only at the soft X-ray energy range. Similar improvement in sensitivity of polarisation measurement at soft X-ray range is expected in near future with the advent of GEM based photoelectric polarimeters. However, at energies >10 keV, even spectroscopic and imaging sensitivities of X-ray detector are limited due to lack of focusing optics. Thus hard X-ray polarimetry so far has been largely unexplored area. On the other hand, typically the polarisation degree is expected to increase at higher energies as the radiation from non-thermal processes is dominant fraction. So polarisation measurement in hard X-ray can yield significant insights into such processes. With the recent availability of hard X-ray optics (e.g. with upcoming NuSTAR, Astro-H missions) which can focus X-rays from 5 KeV to 80 KeV, sensitivity of X-ray detectors in hard X-ray range is expected to improve significantly. In this context we explore feasibility of a focal plane hard X-ray polarimeter based on Compton scattering having a thin plastic scatterer surrounded by cylindrical array scintillator detectors. We have carried out detailed Geant4 simulation to estimate the modulation factor for 100 % polarized beam as well as polarimetric efficiency of this configuration. We have also validated these results with a semi-analytical approach. Here we present the initial results of polarisation sensitivities of such focal plane Compton polarimeter coupled with the reflection efficiency of present era hard X-ray optics.
机译:X射线极化测定法可能是研究天体X射线源的各种物理过程及其几何形状的重要工具。然而,与光谱,定时和成像相比,X射线偏振测定法进展不大,这主要是由于X射线偏振测定法极度需要光子,从而严重限制了X射线偏振计的灵敏度。由于聚焦X射线光学器件仅在软X射线能量范围内有效,因此光谱和成像灵敏度的极大提高是可能的。随着基于GEM的光电偏振仪的出现,预计在不久的将来在软X射线范围内偏振测量的灵敏度也会有类似的提高。但是,在能量> 10 keV的情况下,由于缺乏聚焦光学器件,X射线探测器的光谱和成像灵敏度也受到限制。因此,到目前为止,硬X射线极化仪一直是未开发的领域。另一方面,由于来自非热过程的辐射占主导地位,通常期望偏振度在更高的能量下增加。因此,在硬X射线中进行偏振测量可以对此类过程产生重要的见解。随着近来可以将X射线从5KeV聚焦到80KeV的硬X射线光学器件(例如即将推出的NuSTAR,Astro-H任务)的可用性,有望提高硬X射线范围内X射线探测器的灵敏度显着。在这种情况下,我们探讨了基于康普顿散射的焦平面硬X射线旋光仪的可行性,康普顿散射具有由圆柱形阵列闪烁体检测器包围的薄塑料散射体。我们已经进行了详细的Geant4仿真,以估计100%偏振光束的调制系数以及该配置的极化效率。我们还使用半分析方法验证了这些结果。在这里,我们介绍了这种焦平面康普顿旋光仪的偏振敏感性的初步结果,并结合了当前时代的硬X射线光学器件的反射效率。

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