Dilation Theory by Roy D Herbert suggests it does.
Abstract;
Conservational geometric symmetries apply to all emergent phenomena independently of scale, providing geometric unity and a greater temporal hydrodynamic environment by the conservation of emergent entropic time.
Therefore spacetime holds more than the four dimensions but also a temporal dimension a fluid like symmetry as such, time is more than a quantum moment of change but also a fluid symmetry.
A fifth hydrodynamic temporal environment as such the domain of temporal fluid mechanics, considering the hydrodynamic environment of the fifth dimension as a temporal hydrodynamic environment now allows us to explore the tensor calculus involved.
In a 5-dimensional space-time, the gravitational field can be described by a metric tensor ( g_{ij} ), which represents the geometry of the space-time.
The stress-energy tensor ( T_{ij} ), which describes the distribution of matter and energy, is related to the metric tensor by Einstein's field equations:
R_{ij} - \frac{1}{2} R g_{ij} = 8 \pi G T_{ij} ] where ( R_{ij} ) is the Ricci tensor, ( R ) is the Ricci scalar, and ( G ) is the gravitational constant.
In the context of a temporal hydrodynamic environment, the stress-energy tensor ( T_{ij} ) can be decomposed into a fluid-like component, which represents the energy density and pressure, and a momentum density component.
The fluid-like component can be expressed in terms of the fluid velocity ( u^i ) and the energy density ( \epsilon ) and pressure ( p ) as:
T_{ij} = (\epsilon + p) u_i u_j - p g_{ij} ] The fluid velocity ( u^i ) represents the flow of time in the fifth dimension, and the energy density ( \epsilon ) and pressure ( p ) represent the temporal hydrodynamic properties.
The fluid velocity ( u^i ) is related to the metric tensor ( g_{ij} ) and the time coordinate ( t ) in the fifth dimension by:
u^i = \frac{1}{\sqrt{-g_{00}}} \delta^i_0 ] where ( g_{00} ) is the time-time component of the metric tensor, and ( \delta^i_0 ) is the Kronecker delta.
The temporal hydrodynamic properties ( \epsilon ) and ( p ) can be related to the metric tensor ( g_{ij} ) and the fluid velocity ( u^i ) by:
[ \epsilon = - \frac{T_{00}}{u^0 u^0} ] [ p = \frac{T_{11} + T_{22} + T_{33}}{3} ] where ( T_{00} ) is the time-time component of the stress-energy tensor, and ( T_{11}, T_{22}, T_{33} ) are the space-space components of the stress-energy tensor.
There is however a fundamental flaw inherited from Einstein's field equations, they do not take into consideration that temporal hydrodynamic environment of the fifth dimension, which will ultimate reveal itself no doubt.
To revise Einstein's field equations considering the hydrodynamic environment of the fifth dimension, we need to extend the equations to five dimensions.
The resulting five-dimensional Einstein field equations would be:
$$R_{AB} - \frac{1}{2}Rg_{AB} + \Lambda g_{AB} = \frac{8\pi G}{c^4}T_{AB}$$
where the indices A and B now run from 0 to 4, and the metric tensor g_{AB} is a five-dimensional tensor.
All is conserved in time as is time, with my regards to all.