Skeldon, K.D. et al. (2000) Performance of the Glasgow 10 m prototype gravitational wave detector operating at lambda=1064 nm. Physics Letters A, 273(5-6), 277 -284. (doi:10.1016/S0375-9601(00)00511-9)
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Publisher's URL: http://dx.doi.org/10.1016/S0375-9601(00)00511-9
We report on measurements performed with the Glasgow prototype gravitational wave detector which has recently been converted to operate with a Nd:YAG laser at 1064 nm. The differential displacement amplitude spectral density above a few hundred Hz is similar to 5 x 10(-19) m/root Hz which is consistent with the limitations imposed by shot noise in this frequency range. We also present sensitivity spectra over a lower frequency regime to highlight the impact of improved suspension designs.
|Glasgow Author(s) Enlighten ID:||Casey, Dr Morag and Hough, Professor James and Barr, Dr Bryan and Ward, Dr Henry and Newton, Dr Gavin and Skeldon, Dr Kenneth and Strain, Professor Kenneth and Plissi, Dr Michael|
|Authors:||Skeldon, K.D., Clubley, D.A., Barr, B.W., Casey, M.M., Hough, J., Killbourn, S.D., McNamara, P.W., Newton, G.P., Plissi, M.V., Robertson, D.I., Robertson, N.A., Strain, K.A., and Ward, H.|
|Subjects:||Q Science > QC Physics|
|College/School:||College of Science and Engineering > School of Physics and Astronomy|
|Journal Name:||Physics Letters A|