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Gravitational Radiation and the Validity of General Relativity

OCT 01, 1999
Observing the speed, polarization, and back influence of gravitational waves would subject Einstein’s theory to new tests.
Clifford M. Will

While the detection of gravitational radiation may usher in a new era of “gravitational wave” astronomy (see the accompanying article by Barry Barish and Rainer Weiss, on page 44), it should also yield new and interesting tests of Einstein’s general theory of relativity, especially in the radiative and strong‐field regimes. Consequently, we are in an unusual situation. After all, we rarely think of electromagnetic astronomy as providing tests of Maxwell’s theory. Neutrino astronomy may be a closer cousin: We can observe neutrinos to learn about the solar interior or about supernovae, while also checking such fundamental phenomena as neutrino oscillations. To some extent, the usefulness of astronomical observations in testing fundamental theory depends upon how well tested the theory is already. At the same time, since general relativity is the basis for virtually all discussion of gravitational‐wave detectors and sources, the extent of its “upfront” validity is of some concern to us.

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References

  1. 1. For reviews, see J.‐A. Marck, J.‐P. Lasota, eds., Relativistic Gravitation and Gravitational Radiation, Cambridge U. P., Cambridge, England (1997).

  2. 2. For reviews, see C. M. Will, Theory and Experiment in Gravitational Physics, Cambridge U. P., Cambridge, England (1993).
    See also C. M. Will, in Gravity from the Hubble Length to the Planck Length: XXVI SLAC Summer Institute on Particle Physics, L. Dixon, ed., Stanford Linear Accelerator Center, Stanford, Calif, in press, available on the Web at http://www.slac.stanford.edu/gen/meeting/ssi/1998/manu_list.html. For a popular accounting, see C. M. Will, Was Einstein Right? Basic Books, New York (1993, reprinted 1998).

  3. 3. T. Damour, in Marck and Lasota, p. 3.

  4. 4. Y. Suet et al., Phys. Rev. D 50, 3614 (1994).https://doi.org/PRVDAQ

  5. 5. R. A. Hulse, Rev. Mod. Phys. 66, 699 (1994).
    J. H. Taylor, Rev. Mod. Phys. 66, 711 (1994).https://doi.org/RMPHAT

  6. 6. A. Wolszczan, in Marck and Lasota, p. 113.

  7. 7. See articles by C. W. F. Everitt, G. M. Reiser, and others, in Proc. Eighth Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation, and Relativistic Field Theories, T. Piran, ed., World Scientific, Singapore (1999), pp. 259, 1135, 1139.

  8. 8. C. M. Will, Phys. Rev. D 57, 2061 (1998).https://doi.org/PRVDAQ

  9. 9. L. Blanchet, in Marck and Lasota, p. 33.

  10. 10. See the following articles in Marck and Lasota: E. Müller, p. 273;
    K. Oohara, T. Nakamura, p. 309;
    E. Seidel, W.‐M. Suen, p. 335;
    S. Bonazzola, E. Gourgoulhon, J.‐A. Marck, p. 257.

More about the authors

Clifford M. Will, McDonnell Center for the Space Sciences, Washington University.

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Volume 52, Number 10

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