I cannot see the link between time uniformity and conservation of energy the way it is tackled in this excerpt...
It is very difficult to understand what the author means in detail based solely on the posted excerpt. The author is trying to explain something in everyday language that really only can be explained in equations.
Conservation of energy can be seen to hold in a variety of systems ranging from classical mechanical systems, to relativistic systems, to quantum mechanical systems. The requirement for conservation of energy turns out to be that there is no explicit time-dependence in the Hamiltonian (e.g., no time dependent constraints, no time dependent potential, etc.).
To see how this comes about, consider a simple example of a single particle (with mass $m$, position $x$ and velocity $v=dx/dt$) in one dimension in a constant conservative potential (U). The Hamiltonian for this systems is:
$$
H = \frac{m}{2}v^2 + U(x)
$$
The time derivative is:
$$
\frac{dH}{dt} = \frac{m}{2}2v\frac{dv}{dt} + \frac{dU}{dx}v
$$
$$
=mva-Fv,
$$
since $\frac{dU}{dx} = -F$, for a conservative potential.
But, we know that $F = ma$, from Newton's second law, so the RHS is actually zero:
$$
\frac{dH}{dt} = mva - mav = mva - mva = 0
$$
This property of the Hamiltonian turns out to hold much more generally[1] such that:
$$
\frac{dH}{dt} = \frac{\partial H}{\partial t}\;,
$$
which means that if there is no explicit time dependence in the Hamiltonian H (i.e., $\frac{\partial H}{\partial t}=0$) then $\frac{dH}{dt}=0$. This latter equation is what we mean when we say that energy is conserved.
To restate again in words: If there is no explicit time dependence in the Hamiltonian then energy is conserved. This is really "all" that can be understood from the quoted flowery excerpt.
[1]: For the Classical case, see, for example, Whittaker's "A Treatise of The Analytical Dynamics of Particles and Rigid Bodies" (2nd Edition) at page 62.