检索规则说明:AND代表“并且”;OR代表“或者”;NOT代表“不包含”;(注意必须大写,运算符两边需空一格)
检 索 范 例 :范例一: (K=图书馆学 OR K=情报学) AND A=范并思 范例二:J=计算机应用与软件 AND (U=C++ OR U=Basic) NOT M=Visual
作 者:吴铠岚 林栩凌[1] 郑永超[1] 黎明[3] 边星 王运永[5] 霍红庆 牛家树 贾建军[7] 张晓敏 WU Kailan;LIN Xuling;ZHENG Yongchao;LI Ming;BIAN Xing;WANG Yunyong;HUO Hongqing;NIU Jiashu;JIA Jianjun;ZHANG Xiaomin(Beijing Institute of Space Mechanics and Electricity,Beijing 100094,China;School of Physical Science and Technology,Lanzhou University,Lanzhou 730000,China;DFH Satellite Co.,Ltd.,Beijing 100094,China;Institute of Mechanics,Chinese Academy of Sciences,Beijing 100190,China;Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China;Shanxi University,Taiyuan 237016,China;Shanghai Institute of Technical Physics,Chinese Academy of Sciences,Shanghai 200083,China;Beijing Azspace Technology Co.,Ltd,Beijing 100190,China)
机构地区:[1]北京空间机电研究所,北京100094 [2]兰州大学物理科学与技术学院,兰州730000 [3]航天东方红卫星有限公司,北京100094 [4]中国科学院力学研究所,北京100190 [5]中国科学院高能物理研究所,北京100049 [6]山西大学,太原237016 [7]中国科学院上海技术物理研究所,上海200083 [8]北京紫微宇通科技有限公司,北京100190
出 处:《深空探测学报(中英文)》2023年第3期247-256,共10页Journal Of Deep Space Exploration
基 金:国家重点研发计划(2020YFC2200404,SQ2021YFC220144)。
摘 要:为覆盖月基引力波探测的0.1~5 Hz测量频段,进一步提高引力波探测的灵敏度,月基引力波探测方案被提出。在简要介绍引力波数学描述及特性的基础上,对当前已有的几种主要月基引力波探测方案进行了介绍,重点论述了各方案的探测原理、探测灵敏度以及探测目标;将月基探测方案与地面及空间探测方案进行了对比;讨论分析了月基引力波探测方案实施所需要考虑的关键问题,给出了可能的解决方法;讨论分析了月基引力波探测可能的主要噪声源以及对应的影响量级;对月基引力波探测的未来发展进行了展望。To observe the frequency in the range of 0.1 Hz to 5 Hz in lunar-based gravitational-wave detection and improve the sensitivity of gravitational-wave detection,a method of lunar-based gravitational-wave detection was proposed.Based on a brief introduction to the mathematical description and properties of gravitational waves,this paper gave a brief introduction to existing gravitational-wave detectors and compared the lunar-based observatories with the space and Earth-based detectors.Lunar-based detectors that have been proposed,such as Gravitational-wave Lunar Observatories for Cosmology(GLOC),Lunar Gravitational-Wave Antenna(LGWA),etc.,are briefly introduced.The critical technique is also discussed and alternative solutions are given.The possible main noise sources and corresponding impact magnitudes for lunar-based gravitational wave detection were discussed.Also,the future development of the lunar-based gravitational wave detection is prospected.
关 键 词:引力波探测 月基引力波探测 激光干涉测量 月震仪阵列 引力波天文学
分 类 号:V11[航空宇航科学与技术—人机与环境工程]
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在链接到云南高校图书馆文献保障联盟下载...
云南高校图书馆联盟文献共享服务平台 版权所有©
您的IP:216.73.216.7