• 主题
高级搜索  >
历史搜索 清空历史
首页> 外文会议>International astronautical congress >ASTROPHYSICAL DATA ANALYSIS FOR THE DETECTION OF GRAVITATIONAL WAVES FROM INSPIRAL COMPACT BINARIES INJECTED IN LIGO'S FIFTH AND SIXTH SCIENCE RUNS
【24h】

ASTROPHYSICAL DATA ANALYSIS FOR THE DETECTION OF GRAVITATIONAL WAVES FROM INSPIRAL COMPACT BINARIES INJECTED IN LIGO'S FIFTH AND SIXTH SCIENCE RUNS

机译：从Ligo第五和第六科学中注射的载体紧凑型二进制文件中检测引力波的天体物理数据分析

获取原文
页面导航
  • 摘要
  • 著录项
  • 相似文献
  • 相关主题

摘要

Gravitational Waves (GW), the ripples in the fabric of the space-time predicted one hundred years ago in the Einstein's General Theory of Relativity, have been finally detected. These gravity waves are emitted by massive astrophysical objects moving with violent accelerations and propagates at the speed of light. The tremendous effort of a great number of scientists has ended with the detection of a GW emitted 1.3 billion years ago by a binary system composed of two merging black holes of masses 36 and 29 the sun's mass possibly located in the Magellanic cloud. Detection of GW required the construction and calibration of a network of very sensible instruments designed to measure distance changes in the order of 1/1000th the diameter of a proton. These instruments are based on the L-shape laser Michelson interferometer. The most representative of these GW detectors is the two 4km-long-arms interferometers named Laser Interferometer Gravitational-wave Observatory (LIGO). This work presents an introduction to the fundamental theory of GW, the nature and characteristics of the different astrophysical sources of GW and describes the scientific and technological efforts developed to detect GWs using LIGO. Subsequently, the work focuses on the mathematical model of GW generated by inspiral compact binaries, a system composed of a pair of neutron stars and/or black holes in their late stage of evolution, and presents a comprehensive data analysis methodology developed to perform detection of the GW emitted by these astrophysical sources that are induced in intcrfcromctcr-bascd detector such as LIGO. Results of experiments performed to test and evaluate the detection of GW from inspiral compact binaries injected in LIGO's fifth and sixth science runs are presented and discussed.
机译：引力波（GW），在一百年前在爱因斯坦一般的相对论中预测的空间时间纹体的涟漪已经终于检测到。这些重力波被大规模的天体物理物体发出，其具有剧烈加速度，并以光速传播。大量科学家的巨大努力已经通过一个由两种合并的黑洞36和29可能位于Magellanic云中的Sun的群体组成的二进制系统，以13亿多年来的巨额系统的努力。 GW的检测需要施工和校准设计，该网络设计用于测量距离变化的距离为1/1000的直径。这些仪器基于L形激光迈克尔逊干涉仪。这些GW探测器的最代表性是名为激光干涉仪重力波天文台（Ligo）的两个4km长臂干涉仪。这项工作介绍了GW的基本理论，不同天体物理来源的基本理论，并描述了使用Ligo检测GWS的科学和技术努力。随后，该工作侧重于由Inspiral Compact二进制文件产生的GW的数学模型，该系统由进化后期的一对中子恒星和/或黑洞组成，并提出了一种开发用于执行检测的综合数据分析方法这些天体物理源发出的GW，其在IntcromctCr-Bascd检测器中诱导如Ligo。提出并讨论了对Rigo第五和第六次科学运行中注射的施肥紧凑型副术中的测试和评估GW检测的实验结果。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱：kefu@zhangqiaokeyan.com

京公网安备：11010802029741号 ICP备案号：京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有

  • 客服微信

  • 服务号