本文主要研究内容
作者（2019）在《Gravitational wave standard sirens and cosmological parameter measurement》一文中研究指出：The first detection of gravitational waves (GWs) produced by the binary neutron star (BNS) merger in August 17, 2017[1] is fairly meaningful because it initiated the new era of multi-messenger astronomy. In this BNS merger event, we not only detected the gravitational waves, but also detected the electromagnetic waves in various wave bands [2]. This multi-messenger observation led to a series of important re-
Abstract
The first detection of gravitational waves (GWs) produced by the binary neutron star (BNS) merger in August 17, 2017[1] is fairly meaningful because it initiated the new era of multi-messenger astronomy. In this BNS merger event, we not only detected the gravitational waves, but also detected the electromagnetic waves in various wave bands [2]. This multi-messenger observation led to a series of important re-
论文参考文献
[1].GW170817: The key to the door of multi-messenger astronomy including gravitational waves[J]. He Gao. Science China(Physics,Mechanics & Astronomy).2018(05)[2].The promising dawn of multimessenger astronomy[J]. Mike Guidry. Science Bulletin.2018(01)[3].Propagation effect of gravitational wave on detector response[J]. Zhe Chang,Chao-Guang Huang,Zhi-Chao Zhao. Science China(Physics,Mechanics & Astronomy).2016(10)[4].An exciting time for gravitational wave astronomy[J]. Fan Zhang. Science Bulletin.2016(03)[5].A global analysis searching for neutrinos associated with black hole merger gravitational wave events[J]. Yu-Zi Yang,Jia-Jie Ling,Wei Wang,Zhao-Kan Cheng. Research in Astronomy and Astrophysics.2018(11)[6].National Astronomical Observatories Chinese Academy of Sciences[J]. Bulletin of the Chinese Academy of Sciences.2011(03)[7].Chinese Scientists Hail the Era of Gravitational Wave Astronomy[J]. XIN LING. Bulletin of the Chinese Academy of Sciences.2015(03)[8].THE PROGRAM OF GLOBAL CHARACTER RESEARCH OF SOLAR TERRESTRIAL SYSTEM IN THE 22TH SOLAR CYCLE—Forward of the Proceedings[J]. Wen Rui HUInstitute of Mechanics, Chinese Academy of SciencesBai Rong ZHANG Yunnan Observatoty, Chinese Academy of Sciences. 云南天文台台刊.1989(S1)[9].Development of superconducting mixers for THz astronomy[J]. SHI ShengCai1,2 1Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China;2Key Laboratory of Radio Astronomy,Chinese Academy of Sciences,Nanjing 210008,China. Science China(Information Sciences).2012(01)[10].Space Astronomy in China:2008-2010[J]. Gan Weiqun1 Zhang Shuangnan2 Yan Yihua3 Chang Jin11(Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008) 2(Institute of High Energy Physics,Chinese Academy of Sciences) 3(National Astronomical Observatory,Chinese Academy of Sciences). 空间科学学报.2010(05)
论文详细介绍
论文作者分别是来自Science China(Physics,Mechanics & Astronomy)的，发表于刊物Science China(Physics,Mechanics & Astronomy)2019年11期论文，是一篇关于,Science China(Physics,Mechanics & Astronomy)2019年11期论文的文章。本文可供学术参考使用，各位学者可以免费参考阅读下载，文章观点不代表本站观点，资料来自Science China(Physics,Mechanics & Astronomy)2019年11期论文网站，若本站收录的文献无意侵犯了您的著作版权，请联系我们删除。
标签：Science China(Physics; Mechanics & Astronomy)2019年11期论文;
：Gravitational wave standard sirens and cosmological parameter measurement论文
下载Doc文档