论文标题
伽马射线观察大力神群的前景
Prospects for gamma-ray observations of Hercules cluster
论文作者
论文摘要
星系簇（GC）是宇宙大规模结构中最大，最大的重力物体。由于簇内培养基（ICM）和宇宙射线（CRS）的keV温度，GC是热X射线辐射的有效来源和非热的Leptonic（Synchrotron）无线电发射。 GC也是HADRONIC CRS的储藏室，但尚未检测到GCS的非热辐射伽玛射线排放（主要是由于PP碰撞和随后的Pion Decay引起的）。在这项工作中，我们模拟了从Hercules群集的主要部分-GC A2151中的预期非热态伽马射线和中微子排放，并估计了通过现有（Fermi-Lat，Lhass，lhasso，icecube）和计划的（CTA，ICECUBE，ICECUBE-GEN2）地面基于基于基础的Ans Spectors的观察的观点。
Galaxy clusters (GCs) are the largest and most massive gravitationally bound objects in the large-scale structure of the Universe. Due to keV temperatures of virialized gas in the intracluster medium (ICM) and presence of cosmic rays (CRs), GCs are effective sources of thermal X-ray radiation and non-thermal leptonic (synchrotron) radio emission. GCs are also store-rooms for hadronic CRs, but non-thermal hadronic gamma-ray emission (mainly, due to pp collisions and subsequent pion decay) from GCs has not been detected yet. In this work we simulate the expected non-thermal hadronic gamma-ray and neutrino emission from dominant part of Hercules cluster - GC A2151 - and estimate a perspective of detection of this emission by existing (Fermi-LAT, LHASSO, IceCube) and planned (CTA, IceCube-Gen2) ground-based ans space-based detectors.
