Linearized Theory of Gravity (Temporal Physics)
Linearized Theory of Gravity In light of the temporal dependence of the metric tensor and the need for a dynamic approach, the metric perturbation in a weak field might be updated to: ημν(t) = [ 1 + α₀ · t² 0 0 0 1 + α₁ · t² 0 0 0 1 + α₂ · t² ] g_μν = η_μν + h_μν Where: h_μν = Perturbation influenced by τ(t) The perturbation h_μν should reflect the time-dependent scaling. For a more accurate representation, the perturbation might be: h_00 = -2 * (k * q1 * q2) / (r * (1 + α * t²)) Modified Potential The Coulomb potential in the context of time-dependence is: V(r, t) = (k * q1 * q2) / (r * (1 + α * t²)) The Newtonian gravitational potential ϕ is then: ϕ(r, t) = (k * q1 * q2) / (r * (1 + α * t²)) Metric Perturbation With the modified potential, the perturbation in the metric tensor due to the gravitational field is: h_00 = -2 * (k * q1 * q2) / (r * (1 + α * t²)) Wave Propagation and Polarization The linearized Einstein field equations for the perturbation now include the time-depende...