Radiative E1 decay widths of are calculated through the relativistic Salpeter method, with the assumption that is the (2P) state, which is the radial excited state of (1P). We firstly calculated the E1 decay width of (1P), the result is in agreement with experimental data excellently, then we calculated the case of with the assignment that it is (2P). Results are: keV, ${\Gamma}({\rm X(3872)}\rightarrow \gamma \psi(2S))=146{\Gamma}({\rm X(3872)}\rightarrow \gamma \psi(3770))=7.09{{\rm Br(X(3872)}\rightarrow\gamma\psi(2{\rm S}))}/{{\rm Br(X(3872)}\rightarrow \gamma {\sl J}/\psi)}=4.4$ agrees with experimental data by BaBar, but larger than the new up-bound reported by Belle recently. With the same method, we also predict the decay widths: ${\Gamma}(\chi_{b1}(1\rm P))\rightarrow \gamma \Upsilon(1\rm S))=30.0{\Gamma}(\chi_{b1}(2\rm P))\rightarrow \gamma \Upsilon(1\rm S))=5.65{\Gamma}(\chi_{b1}(2\rm P))\rightarrow \gamma \Upsilon(2S))=15.8{\Gamma}(\chi_{b1}(1\rm P))\sim 85.7{\Gamma}(\chi_{b1}(2\rm P))\sim 66.5$ keV.

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