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Simulation of a Xe-based X-ray Polarimeter at 10-30 keV

  • J. Zhang
  • , X. Cai
  • , Y. Huang*
  • , Q. Liu
  • , F. Xie
  • , J. Li
  • , H. Liu*
  • *此作品的通讯作者
  • Guangxi Key Laboratory for Relativistic Astrophysics
  • Guangxi University
  • School of Physical Sciences
  • University of Chinese Academy of Sciences
  • Key Laboratory of Particle Astrophysics
  • CAS - Institute of High Energy Physics

科研成果: 期刊稿件 › 文章 › 同行评审

摘要

Polarization detection of X-rays is a non-negligible topic to astrophysical observation. Many polarization detection methods have been well developed for X-rays in the energy range below 10 keV, while the detection at 10-30 keV is rarely discussed. This paper presents a simulation study of a Xe-based gas pixel detector, which can achieve the polarization detection of X-rays at 10-30 keV. To verify the emission angle distribution of photoelectrons, different electromagnetic models in Geant4 were investigated. After a necessary modification by considering the missing factor when sampling the emission angle, a good agreement can be achieved. Moreover, the detection capability of 20 keV polarized photons was discussed and the modulation factor of 43% could be obtained.

源语言英语
期刊论文编号P04003
期刊Journal of Instrumentation
卷17
期4
DOI
出版状态已出版 - 1 4月 2022
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