Skip to main content
Log in

On the band width of resonant gravitational-wave antennas

  • Published:
Lettere al Nuovo Cimento (1971-1985)

Summary

The band width of a resonant gravitational-wave antenna depends on the ratio Г of the wide-band noise to the narrow-band noise. For Г → 0 the band width becomes infinitely large, even if the coupling parameter between bar and transducer is small.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. J. P. Richard:Phys. Rev. Lett.,52, 165 (1984).

    Article  ADS  MATH  Google Scholar 

  2. J. P. Richard: inProceedings of the Second Marcel Grossman Meeting on General Relativity. Trieste, 1979, edited byR. Ruffini (North-Holland, Amsterdam, 1982).

    Google Scholar 

  3. P. Bonifazi, V. Ferrari, S. Frasca, G. V. Pallottino andG. Pizzella:Nuovo Cimento C,1, 465 (1978);

    Article  ADS  Google Scholar 

  4. G. Pizzella:Nuovo Cimento C,2, 209 (1979);

    Article  ADS  Google Scholar 

  5. G. V. Pallottino andG. Pizzella:Nuovo Cimento C,4, 237 (1981).

    Article  ADS  Google Scholar 

  6. Presented byG. Pizzella at theSecond Workshop on Precision Measurements of Relativistic Effects in Astrophysical Systems held in Rome, 11–13July 1983;

  7. G. V. Pallottino andG. Pizzella:Sensitivity of a Weber-type resonant antenna to monochromatic gravitational waves, Nuovo Cimento C, to be bublislied.

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Pizzella, G. On the band width of resonant gravitational-wave antennas. Lett. Nuovo Cimento 40, 240–242 (1984). https://doi.org/10.1007/BF02751776

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02751776

PACS

PACS

Navigation