Past, present and future of the Resonant-Mass gravitational wave detectors

@article{Aguiar2011PastPA,
  title={Past, present and future of the Resonant-Mass gravitational wave detectors},
  author={Odylio Denys Aguiar},
  journal={Research in Astronomy and Astrophysics},
  year={2011},
  volume={11},
  pages={1-42}
}
  • O. Aguiar
  • Published 6 September 2010
  • Physics
  • Research in Astronomy and Astrophysics
Resonant-mass gravitational wave detectors are reviewed from the concept of gravitational waves and its mathematical derivation, using Einstein's general relativity, to the present status of bars and spherical detectors, and their prospects for the future, which include dual detectors and spheres with non-resonant transducers. The review not only covers technical aspects of detectors and sciences that will be done, but also analyzes the subject in a historical perspective, covering the various… 

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References

SHOWING 1-10 OF 176 REFERENCES

Wideband dual sphere detector of gravitational waves.

TLDR
At cryogenic temperatures, one approaches the standard quantum limit for broadband operation with reasonable choices for the cavity finesses and the intracavity light power.

Do Gravitational Waves Travel at Light Velocity

Abstract We extend the standard Feynman–Deser approach of field theoretical derivation of Einstein's gravitational theory. We show that it is possible to obtain a theory that incorporates a great

Gravitational-wave observations as a tool for testing relativistic gravity

Gravitational-wave observations can be powerful tools in the testing of relativistic theories of gravity--perhaps the only tools for distinguishing between certain extant theories in the foreseeable

Optical gravitational wave detectors on the ground and in space: theory and technology

Major predictions of General Relativity, unforeseen at the beginning of the preceding century, are now under investigation. The existence of black holes of any mass from tens to billions of solar

Numerical analysis of the performance of a resonant gravity-wave detector.

This paper presents the results of a detailed numerical calculation of the performance of a resonant gravitational radiation detector which uses an inductive transducer and a superconducting quantum

Gravitational wave reception by a sphere

The reception of gravitational waves by an elastic self-gravitating spherical detector is studied in detail. The equations of motion of a detector driven by a gravitational wave are presented in the

Gravitational wave astronomy

The first decade of the new millennium should see the first direct detections of gravitational waves. This will be a milestone or fundamental physics and it will open the new observational science of

A Geometric Method for Location of Gravitational Wave Sources

We show that the interaction of a gravitational wave with a spherical resonant-mass antenna changes the antenna's shape to that of an ellipsoid. These changes in shape always determine the direction

Gravitational Radiation and Its Detection

A review is presented of the theoretical and experimental aspects of the field of gravitational radiation. This article, aimed particularly at showing that the problem of gravitational radiation can

What can we learn about gravitational wave physics with an elastic spherical antenna

A general formalism is set up to analyse the response of an arbitrary solid elastic body to an arbitrary metric Gravitational Wave perturbation, which fully displays the details of the interaction
...