Effect of Gravitational Scalar Field on High-Density Star Structure

Details Effect of Gravitational Scalar Field on High-Density Star Structure Effect of Gravitational Scalar Field on High-Density Star Structure

Feb 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967phrv..154.1218s&link_type=abstract

Physical Review, vol. 154, Issue 5, pp. 1218-1223

Physics

35

Scientific paper

The theory of gravitation allowing variation of the gravitational constant G by means of a scalar field introduced by Brans and Dicke is applied in the case of a fluid sphere in gravitational equilibrium. The departure of the mass-radius relation in this theory from the Einstein theory is investigated for different values of the constant ω and for high central-energy densities in completely degenerate stars (neutron stars).

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