Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2000-06-22
Phys.Rev.D63:082001,2001
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
20 pages, 7 figures
Scientific paper
10.1103/PhysRevD.63.082001
We rigorously analyze the frequency response functions and antenna sensitivity patterns of three types of interferometric detectors to scalar mode of gravitational waves which is predicted to exist in the scalar-tensor theory of gravity. By a straightforward treatment, we show that the antenna sensitivity pattern of the simple Michelson interferometric detector depends strongly on the wave length $\lambda_{\rm SGW}$ of the scalar mode of gravitational waves if $\lambda_{\rm SGW}$ is comparable to the arm length of the interferometric detector. For the Delay-Line and Fabry-Perot interferometric detectors with arm length much shorter than $\lambda_{\rm SGW}$, however, the antenna sensitivity patterns depend weakly on $\lambda_{\rm SGW}$ even though $\lambda_{\rm SGW}$ is comparable to the effective path length of those interferometers. This agrees with the result obtained by Maggiore and Nicolis.
Harada Tomohiro
Kawamura Seiji
Nakamura Takashi
nakao Ken-ichi
Shibata Masaru
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