- Access by Xinjiang University
Test of Possible Variations of the Gravitational Constant by the Observation of White Dwarfs within Galactic Clusters
Phys. Rev. 128, 2012 – Published 1 December, 1962
DOI: https://doi.org/10.1103/PhysRev.128.2012
Abstract
An astronomical test is suggested for the hypothesis that the gravitational constant varies throughout space-time according to the law , where is a dimensionless constant of the order of unity and is the gravitational potential. If varies, the gravitational self-energy of a body also varies. This brings about a correction in the gravitational force which, in the case of a very dense and massive body like a white dwarf, is not completely negligible. In the gravitational field of the Galaxy, the path of a white dwarf will be slightly different from that of a normal star. In consequence, a white dwarf in a very weakly bound cluster will escape; a white dwarf in a more strongly bound cluster will occupy an anomalous position. Testing these predictions seems to be within the limits of present-day possibilities.
References (19)
- A. Einstein, The Meaning of Relativity (Princeton University Press, Princeton, New Jersey, 1950), p. 102
- D. W. Sciama, Monthly Notices Roy. Astron. Soc. 113, 34 (1953)
- P. Jordan, Schwerkraft und Weltall (Friedrich Viewig und Sohn, Braunschweig, Germany, 1955)
- R. H. Dicke, Revs. Modern Phys. 29, 363 (1957)
- P. Jordan, Z. Physik 157, 112 (1959)
- C. H. Brans, Ph.D. thesis, Princeton University, 1961 (unpublished)
- C. Brans and R. H. Dicke, Phys. Rev. 124, 925 (1961)
- C. Brans, Phys. Rev. 125, 2194 (1962)
- R. H. Dicke, Phys. Rev. 125, 2163 (1962)
- A. Finzi, Nuovo cimento 20, 1079 (1961)
- W. J. Luyten, Harvard College Observatory Annual Card No. 1202
- W. J. Luyten, Astrophys. J. 59, 224 (1954)
Omitted endnote
- J. Peebles (private communication)
- J. H. Oort, Astrophys. J. 116, 233 (1952)
Omitted endnote
- W. J. Luyten (private communication)
- A. R. Sandage, Astrophys. J. 125, 422 (1957)
- B. J. Bock, Sky and Telescope 10, 239 (1951)