Torsion-Bar Antenna for Low-Frequency Gravitational-Wave Observations

DOI 機関リポジトリ (HANDLE) HANDLE HANDLE HANDLE ほか3件をすべて表示 一部だけ表示 被引用文献23件 オープンアクセス

書誌事項

公開日
2010-10
資源種別
journal article
権利情報
  • © 2010 The American Physical Society
DOI
  • 10.1103/physrevlett.105.161101
公開者
The American Physical Society

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説明

We propose a novel type of gravitational-wave antenna, formed by two bar-shaped test masses and laser-interferometric sensors to monitor their differential angular fluctuations. This antenna has a fundamental sensitivity to low-frequency signals below 1 Hz, even with a ground-based configuration. In addition, it is possible to expand the observation band to a lower limit determined by the observation time, by using modulation and up-conversion of gravitational-wave signals by rotation of the antenna. The potential sensitivity of this antenna is superior to those of current detectors in a 1 mHz–10 Hz frequency band and is sufficient for observations of gravitational waves radiated from in-spiral and merger events of intermediate-mass black holes.

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