4.4 Article Proceedings Paper

The International Pulsar Timing Array project: using pulsars as a gravitational wave detector

期刊

CLASSICAL AND QUANTUM GRAVITY
卷 27, 期 8, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/27/8/084013

关键词

-

资金

  1. Direct For Mathematical & Physical Scien
  2. Division Of Astronomical Sciences [1009580, 0748580] Funding Source: National Science Foundation
  3. Direct For Mathematical & Physical Scien
  4. Division Of Physics [0969857] Funding Source: National Science Foundation
  5. Office Of The Director
  6. Office Of Internatl Science &Engineering [0968296] Funding Source: National Science Foundation
  7. Science and Technology Facilities Council [ST/G002487/1, ST/F002874/1] Funding Source: researchfish
  8. STFC [ST/G002487/1, ST/F002874/1] Funding Source: UKRI

向作者/读者索取更多资源

The International Pulsar Timing Array project combines observations of pulsars from both northern and southern hemisphere observatories with the main aim of detecting ultra-low frequency (similar to 10(-9)-10(-8) Hz) gravitational waves. Here we introduce the project, review the methods used to search for gravitational waves emitted from coalescing supermassive binary black-hole systems in the centres of merging galaxies and discuss the status of the project.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.4
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据