We study nonnnegative radially symmetric solutions of the parabolic–elliptic Keller–Segel whole space system0, \\\\ 0=\\Delta v+u+f(x),~ & x\\in {{\\mathbb{R}}^{n}},t>0, \\\\ u(x,0)={{u}_{0}}(x),~ & x\\in {{\\mathbb{R}}^{n}}, \\end{array}\\right. \\end{eqnarray} ?>{ut=Δu−∇⋅(u∇v), x∈Rn,t>0,0=Δv+u+f(x), x∈Rn,t>0,u(x,0)=u0(x), x∈Rn,with prototypical external signal productionf(x):={f0|x|−α,if |x|⩽R−ρ,0,if |x|⩾R+ρ,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 and , for some , 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 c0 > 0, we obtain a strong indication that in fact is critical for the existence of global bounded solutions under a smallness conditions as described above.
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