General Relativity. Can the strength of gravity reduce for dense masses?

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Is there anything in Einstein’s Field Equations that allows the strength of gravity to reduce for regions of high mass/radius ratio? It could be desirable for two reasons.

Reason 1) From Newtonian considerations. The flatness problem is equivalent to (for each mass m).

mc^2-GMm/R=0 (1)

G=Rc^2/M (2)

Where M and R represent the mass and radius of the rest of the universe up to the Hubble radius. Small numerical constants omitted for simplicity.

For a larger mass, with the self-potential energy term included

mc^2-GMm/R-(Gm^2)/r=0 (3)

r is the radius of mass m , leading to

G_reduced = c^2/(M/R+m/r) = G/(1+Gm/(rc^2 )) (4)

i.e. a reduction in G for masses of high m/r ratio, approaching c^2/G

Reason 2)

It would allow bounces or explosions form galactic centres and avoid a situation of infinite density and pressure. It could account for the ‘foam’ like large scale structure.

It's part of a new cosmology

https://www.researchgate.net/publication/342040580_A_New_Solution_of_the_Friedman_Equations

that predicts an apparent omega(m) of between 0.25 and 0.333 and matches supernovae data without a cosmological constant.

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