How Inflationary Gravitons Affect the Force of Gravity

We employ an unregulated computation of the graviton self-energy from gravitons on de Sitter background to infer renormalized result. This is used quantum-correct linearized Einstein equation. solve this equation for potentials that represent gravitational response a static, point mass. find large spatial and temporal logarithmic corrections Newtonian potential shift. Although suppressed by minuscule loop-counting parameter, these cause perturbation theory break down at distances late times. Another interesting fact induce up three logarithms, whereas loop massless, minimally coupled scalars produces only single logarithm. in line with mode function: induces two scalar gives none.