Salmona 1967
Salmona, A., 1967: Effect of gravitational scalar field on high-density star structure. Phys. Rev., 154, 1218-1223, doi:10.1103/PhysRev.154.1218.
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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Salmona, A.: Effect of gravitational scalar field on high-density star structure, Phys. Rev., 154, 1218-1223, doi:10.1103/PhysRev.154.1218, 1967.
Salmona, A. (1967), Effect of gravitational scalar field on high-density star structure, Phys. Rev., 154, 1218-1223, doi:10.1103/PhysRev.154.1218.
Salmona, A., 1967: Effect of gravitational scalar field on high-density star structure. Phys. Rev., 154, 1218-1223, doi:10.1103/PhysRev.154.1218.
Salmona, A. 1967, Phys. Rev., 154, 1218, doi:10.1103/PhysRev.154.1218.
Salmona A. Effect of gravitational scalar field on high-density star structure, Phys Rev 1967;154:1218-1223. doi:10.1103/PhysRev.154.1218.
A. Salmona, Phys. Rev. 154, 1218-1223, doi:10.1103/PhysRev.154.1218 (1967).
