Detecting the stochastic gravitational-wave background

書誌事項

Detecting the stochastic gravitational-wave background

Carlo Nicola Colacino

(IOP concise physics)

Morgan & Claypool, c2017

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注記

Includes bibliographical references

内容説明・目次

内容説明

The stochastic gravitational-wave background (SGWB) is by far the most difficult source of gravitational radiation detect. At the same time, it is the most interesting and intriguing one. This book describes the initial detection of the SGWB and describes the underlying mathematics behind one of the most amazing discoveries of the 21st century. On the experimental side it would mean that interferometric gravitational wave detectors work even better than expected. On the observational side, such a detection could give us information about the very early Universe, information that could not be obtained otherwise. Even negative results and improved upper bounds could put constraints on many cosmological and particle physics models.

目次

Preface Acknowledgements Author biography 1. A brief history of gravitational radiation 2. General theoretical considerations about the cosmological SGWB 3. SGWB generation and source detection 4. Astrophysical sources

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詳細情報

  • NII書誌ID(NCID)
    BB26418044
  • ISBN
    • 9781681740188
  • 出版国コード
    us
  • タイトル言語コード
    eng
  • 本文言語コード
    eng
  • 出版地
    San Rafael, C.A.
  • ページ数/冊数
    1 v.
  • 大きさ
    26 cm
  • 分類
  • 件名
  • 親書誌ID
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