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From modern observations of gravitational interactions, it can be inferredthat there is much left to discover about the fundamental gravitational field.Since the advent of the General Theory of Relativity over a century ago, wehave come to make exotic assumptions pertaining to the inner workings of anassociated field theory. One of which is an elastic nature to spacetime and thebehavior of gravity for strong and weak fields. In this work we investigate amore \textit{physical} nature, expanding upon general relativity led byobservations of strong sources. We introduce a candidate Lorentz-invariantfield theory that employs an \textit{elastic} and \textit{pseudoscalar} natureto the field interpretation and it's properties. A unique generation of theEuler-Lagrange equations of motion is presented; resulting in a longitudinalwave equation for the \textit{Dilation} gravitational field. This provides amodern advancement of a relativistic gravitational field theory, supported byobservation.

Scalar-Tensor Gravitational Strain Field Equations and the Longitudinal Wave Form