We study nonnnegative radially symmetric solutions of the parabolic-elliptic
Keller-Segel whole space system \begin{align*}
\left{\begin{array}{c@{,}l@{\quad}l@{,}c} u_{t}&=\Delta
u-\nabla!\cdot(u\nabla v),\ &x\in^n,& t>0,\ 0 &=\Delta v+u+f(x),
&x\in^n,& t>0,\ u(x,0)&=u_{0}(x),\ &x\in^n,&
\end{array}\right. \end{align*} with prototypical external signal production
\begin{align*} f(x):=\begin{cases} f_0\vert x\vert^{-\alpha},&\vert
x\vert \leq R-\rho,\ 0,& \vert x\vert\geq R+\rho,\ \end{cases}
\end{align*} for and , which is
still integrable but not of class
for some .
For corresponding parabolic-parabolic Neumann-type boundary-value problems in
bounded domains , where
for some
and , it is known that the system does not
emit blow-up solutions if the quantities
$|u_0|{^{\frac{n}{2}+\delta_0}(\Omega)},
|f|{^{\frac{n}{2}+\delta_0}(\Omega)}|v_0|_{^{\theta}(\Omega)}\theta>n$, are all bounded by
some small enough.
We will show that whenever and
in , a measure-valued global-in-time weak
solution to the system above can be constructed which blows up immediately.
Since these conditions are independent of and , we will thus
prove the criticality of for the existence of global bounded
solutions under a smallness conditions as described above.

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