Just to tidy this up. One way to do this formally is to write the position ##x(t)## at any time ##t## then write expressions for the position at specific times 1 and 2 and subtract. It is implicitly understood that time ##t=0## is when motions starts, i.e. the clock starts when the object starts moving. Also, numerical subscripts denote values of quantities at specific times, e.g. ##v_0## is the velocity when the motion (and the clock) starts, ##v_1## is the velocity when the clock reads ##t_1##, etc. Then,
##x(t)=x_0+v_0t+\frac{1}{2}at^2##
##x_1=x_0+v_0t_1+\frac{1}{2}at_1^2##
##x_2=x_0+v_0t_2+\frac{1}{2}at_2^2##
Thus, the displacement from clock time ##t_1## to clock time ##t_2## is $$\Delta x=x_2-x_1=v_0(t_2-t_1)+\frac{1}{2}a\left(t_2^2-t_1^2\right).$$ A second way to do this formally is to start a second clock when the object is at position ##x_1## and has velocity ##v_1##. This clock reads time ##\tau.## The position is, of course, relative to the same origin and is written as
##x(\tau)=x_1+v_1\tau+\frac{1}{2}a\tau^2.## Clearly, the second clock runs behind the first and the times displayed by the clocks are related by ##\tau=t-t_1##. The object reaches ##x_2## at time ##\tau_2=t_2-t_1## so that
$$\begin{align} & x(\tau_2)=x_2=x_1+v_1\tau_2+\frac{1}{2}a\tau_2^2 \nonumber \\
&\implies x_2-x_1=\Delta x=v_1(t_2-t_1)+\frac{1}{2}a\left(t_2-t_1\right)^2.
\end{align}$$ The expressions for the displacement derived by the two methods are the same. This can be verified by substituting ##v_1=v_0+at_1## in equation (1).