Theory of the Detection of Continuous Gravitational Radiation
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概要
- 論文の詳細を見る
The sensitivity of resonant antennas for continuous gravitational radiationemitted from a coherent source is discussed. Fourier integration of the antennaoutput over an extended period results in a signal-to-noise ratio proportional tothe quality factor of the antenna. This holds true even for an antenna withan extremely large quality factor which has an antenna decay time longer thanthe available observation time. The method of cold damping is useful in thisconnection, increasing the bandwidth of the antenna without losing its sensitivity.
- 一般社団法人日本物理学会の論文
- 1979-03-15
著者
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Hirakawa Hiromasa
Department of Nuclear Engineering, Faculty of Engineernig, Kyushu University
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Fujimoto Masakatsu
Tokyo Astronomical Observatory
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