TY - JOUR
T1 - Development of a detector pair for very high frequency gravitational waves
AU - Akutsu, T.
AU - Kawamura, S.
AU - Arai, K.
AU - Tatsumi, D.
AU - Nagano, S.
AU - Sugiyama, N.
AU - Chiba, T.
AU - Takahashi, R.
AU - Yamamoto, K.
AU - Nishizawa, A.
AU - Nishida, E.
AU - Fukushima, Mitsuhiro
AU - Yamazaki, T.
AU - Fujimoto, M. K.
PY - 2008
Y1 - 2008
N2 - We are developing a detector with two laser interferometers for gravitational waves at 100 MHz. Each interferometer is a Sagnac interferometer with a 75-cm baseline synchronous recycling (or resonant recycling) cavity. Two such interferometers are constructed to perform cross-correlation analysis. The original signals at around 100 MHz are converted into electrical signals at lower frequencies before we collect the data. The output noise of each interferometer is measured to correspond to less than 1×10-16 Hz-1/2 in strain amplitude at around 100 MHz.
AB - We are developing a detector with two laser interferometers for gravitational waves at 100 MHz. Each interferometer is a Sagnac interferometer with a 75-cm baseline synchronous recycling (or resonant recycling) cavity. Two such interferometers are constructed to perform cross-correlation analysis. The original signals at around 100 MHz are converted into electrical signals at lower frequencies before we collect the data. The output noise of each interferometer is measured to correspond to less than 1×10-16 Hz-1/2 in strain amplitude at around 100 MHz.
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U2 - 10.1088/1742-6596/122/1/012007
DO - 10.1088/1742-6596/122/1/012007
M3 - Article
AN - SCOPUS:65649119318
SN - 1742-6588
VL - 122
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
M1 - 012007
ER -