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The new gravitational radiation detectors

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Lettere al Nuovo Cimento (1969-1970)

An Erratum to this article was published on 01 December 1970

12. - Conclusion.

The room temperature electronics described here solves the problem of detection of the thermal fluetuations of the aluminum cylinder gravitational radiation detectors, with good signal-to-noise ratio and time resolution as small as a few tenths of one second.

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Footnotes

  1. J. Weber:Phys. Rev.,117, 306 (1960).

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  2. J. Weber:Phys. Rev. Lett.,17, 1228 (1966).

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  3. J. Weber:Phys. Rev. Lett.,24, 276 (1970).

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Author notes

  1. J. Weber

    Present address: the University of Maryland, College Park, Md.

Authors and Affiliations

  1. The Institute for Advanced Study, Princeton, N. J.

    J. Weber

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  1. J. Weber
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Supported in part by the National Science Foundation.

An erratum to this article is available at http://dx.doi.org/10.1007/BF02753709.

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Weber, J. The new gravitational radiation detectors. Lettere Nuovo Cimento (1969-1970) 4, 653–658 (1970). https://doi.org/10.1007/BF02755039

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  • DOI: https://doi.org/10.1007/BF02755039

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