Gas-based time projection chambers (TPCs) have been shown to be highly sensitive X-ray polarimeters having excellent quantum efficiency while at the same time achieving large modulation factors. To observe polarization of the prompt X-ray emission of a Gamma-ray burst (GRB), a large area detector is needed. Diffusion of the electron cloud in a standard TPC could be prohibitive to measuring good modulation when the drift distance is large. Therefore, we propose using a negative ion TPC (NITPC) with Nitromethane (CH3NO2) as the electron capture agent. The diffusion of negative ions is reduced over that of electrons due to the thermal coupling of the negative ions to the surrounding gas. This allows for larger area detectors as the drift distance can be increased without degrading polarimeter modulation. Negative ions also travel ~200 times slower than electrons, allowing the readout electronics to operate slower, resulting in a reduction of instrument power. To optimize the NITPC design, we have measured gas gain with SciEnergy gas electron multipliers (GEMs) in single and double GEM configurations. Each setup was tested with different gas combinations, concentrations and pressures: P10 700 Torr, Ne+CO2 700 Torr at varying concentrations of CO2 and Ne+CO2+CH3NO2 700 Torr. We report gain as a function of total voltage, measured from top to bottom of the GEM stack, and as a function of drift field strength for the gas concentrations listed above. Examples of photoelectron tracks at 5.9 keV are also presented.
Performance measurement of HARPO: a Time Projection Chamber as a gamma-ray telescope and polarimeter
我们分析了气体时间投影室(TPC)作为高性能的伽马射线望远镜和偏振仪在e $^+$ e $^-$对创建制度的性能。我们使用在已知偏振的伽马射线束收集的数据。TPC提供由气体体积中的每次转换引起的轨迹的两个正交投影$(x,z)$和$(y,z)$。我们使用一个简单的顶点查找程序,其中顶点和伪轨迹退出他们被确定。我们用蒙特卡罗模拟研究了单光子角分辨率的各种贡献,并将它们与实验数据进行了比较,发现它们非常吻合。由于探测器的非圆柱对称结构,对转换的方位角分布显示出偏差。这种偏差将在太空任务的长时间曝光中达到平均值,但对于这种双光束表征,我们通过双系统控制方案确保了其准确模拟,数据采集采用相对于光束偏振方向旋转几个角度的探测器,并采用非偏振光束进行系统控制。我们测量,第一次,在低能量对创建制度的线性偏振伽马射线束的偏振不对称性。这个亚GeV的能量范围对于宇宙源来说是至关重要的,因为它们的光谱是幂律的,随着能量的增加而迅速下降。这项工作可以为将极化伽马射线天文学扩展到MeV能量范围之外铺平道路。