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First retain the question's units $c=1$. Insert the retarded time Dirac delta:For a point charge, the spatial delta sets $x^{\prime }=x_0(t^{\prime })$. Put $R(t^{\prime })=|x-x_0(t^{\prime })|$, $\hat{R}=(x-x_0)/R$ and $v={\dot{x}}_0(t^{\prime })$. The retarded root $t_{\ast }$ satisfies $t-t_{\ast }=R(t_{\ast })$. The derivative of the delta's argument is $-1+\hat{R}\cdot v$, so for a subluminal trajectory its absolute value is $1-\hat{R}\cdot v$. Performing the time integral givesAll quantities in the denominator are evaluated at the retarded time. The retarded vector potential uses current $j=qv{\delta }^{(3)}(x^{\prime }-x_0)$ and the same Jacobian determinant, givingRestoring physical $c$, the root is $t-t_{\ast }=R_{\ast }/c$, both denominators become $R_{\ast }-v_{\ast }\cdot {\mathbf{R}}_{\ast }/c$, and ${\mu }_0=1/({ϵ}_0{c}^2)$. Thus $\mathbf{A}=v_{\ast }\varphi /c^2$. This is the Liénard–Wiechert potential; the Jacobian determinant, rather than merely substituting retarded position into a static Coulomb formula, accounts for the velocity factor.

The retarded potential represents causal propagation: each source element contributes according to its charge density at the earlier time needed for a signal to reach the observer, with inverse-distance weighting. The printed formula uses units with the speed of light equal to one.

Insert a Dirac delta function in time to writeFor the moving point charge, spatial integration leaves $q/(4\pi {ϵ}_0)$ times $\int R(\tau {)}^{-1}\delta (t-\tau -R(\tau ))d\tau$, with $R(\tau )=|x-x_0(\tau )|$. The retarded time ${\tau }_r$ solves $t-{\tau }_r=R({\tau }_r)$. Since $R^{\prime }(\tau )=-v(\tau )\cdot n(\tau )$, the delta-function Jacobian is $1-v\cdot n$, positive for subluminal motion. Therefore the Liénard–Wiechert potential iswhere $R=x-x_0({\tau }_r)$ and $v={\dot{x}}_0({\tau }_r)$. Replacing charge density by the current density $qv{\delta }^{(3)}(x-x_0)$ gives $\boxed{A=v\varphi }$ in these $c=1$ units. Restoring SI units gives denominator $R-v\cdot R/c$ and $A=v\varphi /c^2$, with all source quantities still evaluated at retarded time.

The past light cone of a spacetime event $O$ is the past-directed part of its light cone. In Minkowski spacetime, its spacetime events satisfy $|\Delta \mathbf{x}|=-c\Delta t$ with $\Delta t<0$. They are the possible emission events of light rays arriving at $O$. The interior also contains events that can send slower signals to $O$. The retarded potential of a moving point electric charge, given by the Liénard–Wiechert potential, uses the emission event where the source's world line intersects this boundary.