  Recently it was shown that classical electromagnetism admits new asymptotic
conservation laws \cite{2007.03627}. In this paper we derive the analogue of
the first of these asymptotic conservation laws upon imposing Feynman boundary
condition on the radiative field. We also show that the Feynman solution at
$\mathcal{O}(e^3)$ contains purely imaginary modes falling off as $\lbrace
\frac{\log u}{u^nr}, n\geq 0\rbrace$ which are absent in the classical
radiative solution. The $\log u$ mode has also appeared in
\cite{1903.09133,1912.10229} and violates the Ashtekar-Struebel fall offs for
the radiative field\cite{AS}. We expect that new $\frac{(\log
u)^m}{u^mr}$-modes would appear in the Feynman solution at order
$\mathcal{O}(e^{2m+1})$. Thus, all the other modes are expected to preserve the
Ashtekar-Struebel fall offs.
