WIDE-BAND MEASUREMENT OF GRAVITATIONAL-WAVES - THE VIRGO PROJECT

被引：3

作者：

GIAZOTTO, A

机构：

[1] Sezione di Pisa, INFN, Pisa

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS | 1992年 / 15卷 / 06期

关键词：

Experimental tests of general relativity and observations of gravitational radiation;

D O I：

10.1007/BF02506688

中图分类号：

学科分类号：

摘要：

To detect gravitational waves (GW) in a frequency range between 10 Hz and few kHz a ground-bases antenna was designed by the French-Italian collaboration VIRGO. The antenna is a 3 km long interferometer with special suspensions for the optical components, planned to reduce the seismic noise in order to reach the low-frequency region. Results on the seismic isolation devices are given together with some preliminary results on the use of permanent magnets on the VIRGO suspensions.

引用

页码：955 / 971

页数：17

共 18 条

[1]

Pacini F., Nature, 219, (1968)

[2]

Gold T., Nature, 218, (1968)

[3]

Zimmerrmann M., Szedenits E., Gravitational waves from rotating and precessing rigid bodies: Simple models and applications to pulsars, Physical Review D, 20, (1979)

[4]

Zimmerrmann M., Gravitational waves from rotating and precessing rigid bodies. II. General solutions and computationally useful formulas, Physical Review D, 21, (1980)

[5]

Zimmerrmann M., Nature, 271, (1978)

[6]

Pandharipande V.R., Pines D., Smith R.A., Neutron star structure : theory observation, and speculation., The Astrophysical Journal, 208, (1976)

[7]

Taylor J.H., Manchester R.N., Galactic distribution and evolution of pulsars, The Astrophysical Journal, 215, (1977)

[8]

Lyne A.G., Manchester R.N., Taylor J.H., The galactic population of pulsars, Monthly Notices of the Royal Astronomical Society, 213, (1985)

[9]

Manchester R.N., Taylor J.H., Observed and derived parameters for 330 pulsars, The Astronomical Journal, 86, (1981)

[10]

Rawley L.A., J. H. T, Nature, 218, (1968)

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