/
Article

Does gravity change with time?

JUL 01, 1980
Highly regarded theories hold that the gravitational “constant” should decrease with time. To date no observations have refuted this prediction and some offer positive evidence supporting it.
Paul S. Wesson

The Newtonian gravitational parameter G is a constant in both Newton’s law of gravitation (force = −GM1M2/r122) and Einstein’s general theory of relativity. However, over the last fifty years there have been numerous suggestions that G might in fact change with time. The detailed grounds for these suggestions have differed, but most variable‐G theories account for gravitation on a cosmological basis. As such, they usually involve a time‐dependent G: G = G(t), where t is a parameter that can, loosely speaking, be interpreted as the “age” of the Universe. A value of G that depends on time is a drastic departure from the established physics of gravitation (based on Newton’s and Einstein’s theories). Before looking at G‐variability in detail it is therefore logical to ask first: Why should G vary?

This article is only available in PDF format

References

  1. 1. P. S. Wesson, Cosmology and Geophysics, A. Hilger, Bristol, U K (1978).

  2. 2. P. A. M. Dirac, Proc. Roy. Soc. Lond. A165, 199 (1938).

  3. 3. P. A. M. Dirac, Proc. Roy. Soc. Lond. A333, 403 (1973).

  4. 4. F. Hoyle, J. V. Narlikar, Nature 233, 41 (1971).https://doi.org/NATUAS

  5. 5. V. Canuto, P. J. Adams, S.‐H. Hsieh, E. Tsiang, Phys. Rev. (Ser. 3) D16, 1643 (1977).

  6. 6. P. S. Wesson, Gravity, Particles and Astrophysics, D. Reidel, Dordrecht, Holland; in press (1980).

  7. 7. V. Canuto, S.‐H. Hsieh, Ap. J. 237, 613 (1980).

  8. 8. V. Canuto, S.‐H. Hsieh, Ap. J. Suppl. 41, 243 (1979);
    V. Canuto, S.‐H. Hsieh, J. R. Owen, Ap. J. Suppl. 41, 263 (1979),
    and V. Canuto, J. R. Owen, Ap. J. Suppl. 41, 301 (1979).

  9. 9. J. M. Barnothy, B. M. Tinsley, Ap. J. 182, 343 (1973).

  10. 10. V. Canuto, J. V. Narlikar, Ap. J. 236, 6 (1980).

  11. 11. V. Canuto, S.‐H. Hsieh, J. R. Owen, Mon. Not. Roy. Astr. Soc. 188, 829 (1979).

  12. 12. T. C. Van Flandern, Mon. Not. Roy. Astr. Soc. 170, 333 (1975).

  13. 13. R. C. Ritter, G. T. Gillies, R. T. Rood, J. W. Beams, Nature 271, 228 (1978).https://doi.org/NATUAS

More about the authors

Paul S. Wesson, Department of Geophysics and Astronomy, the University of British Columbia, Vancouver.

Related content
/
Article
/
Article
Cognizant of their role within the scientific community, scientific societies had to weigh how to respond to the actions by the Atomic Energy Commission.
/
Article
Interviews now available to the public bring the famed physicist’s lesser-known early years to life.
/
Article
Graduate students in physics and astronomy struggle with mental health. Support from peers and advisers is critical; so is institutional change.
This Content Appeared In
pt-cover_1980_07.jpeg

Volume 33, Number 7

Get PT newsletters in your inbox

pt_newsletter_card_blue.png
PT The Week in Physics

A collection of PT's content from the previous week delivered every Monday.

pt_newsletter_card_darkblue.png
PT New Issue Alert

Be notified about the new issue with links to highlights and the full TOC.

pt_newsletter_card_pink.png
PT Webinars & White Papers

The latest webinars, white papers and other informational resources.

By signing up you agree to allow AIP to send you email newsletters. You further agree to our privacy policy and terms of service.