GAMMA-400 项目现状
天体物理仪器与方法
2015-06-03 v1
摘要
本文介绍了新型空间伽马射线望远镜 GAMMA-400 的初步设计，其能量范围为 100 MeV - 3 TeV。该仪器的角分辨率在 MeV 时为 1-2，在 GeV 时约为 0.01；能量分辨率在 GeV 时约为 1%；质子排斥因子约为 。这些指标经过优化，旨在解决广泛的科学课题，例如搜寻暗物质信号、研究银河系及河外伽马射线源、银河系及河外弥漫辐射、伽马射线暴，以及对宇宙射线电子、正电子和原子核能谱进行高精度测量。
引用
@article{arxiv.1201.2490,
title = {Status of the GAMMA-400 Project},
author = {A. M. Galper and O. Adriani and R. L. Aptekar and I. V. Arkhangelskaja and A. I. Arkhangelskiy and M. Boezio and V. Bonvicini and K. A. Boyarchuk and Yu. V. Gusakov and M. O. Farber and M. I. Fradkin and V. A. Kachanov and V. A. Kaplin and M. D. Kheymits and A. A. Leonov and F. Longo and P. Maestro and P. Marrocchesi and E. P. Mazets and E. Mocchiutti and A. A. Moiseev and N. Mori and I. Moskalenko and P. Yu. Naumov and P. Papini and P. Picozza and V. G. Rodin and M. F. Runtso and R. Sparvoli and P. Spillantini and S. I. Suchkov and M. Tavani and N. P. Topchiev and A. Vacchi and E. Vannuccini and Yu. T. Yurkin and N. Zampa and V. G. Zverev},
journal= {arXiv preprint arXiv:1201.2490},
year = {2015}
}
备注
6 pages, 1 figure, 1 table, submitted to Advances in Space Research