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Test of Possible Variations of the Gravitational Constant by the Observation of White Dwarfs within Galactic Clusters

Arrigo Finzi*

  • Istituto di Fisica, Università di Roma, Roma, Italia

  • *On leave from the Israeli Institute of Technology, Haifa, Israel.

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 k varies throughout space-time according to the law k=k0(1+aVc2), where a is a dimensionless constant of the order of unity and V is the gravitational potential. If k 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.

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