We present an explanation of the unusual peak/dip/hump features observed in photoemission experiments on Bi2212 at . We argue that these features arise from the interaction of the fermionic quasi-particles with overdamped spin fluctuations. We show that the strong spin-fermion interaction combined with the feedback effect on the spin damping due to superconductivity yields a Fermi-liquid form of the fermionic spectral function for $\omega < 2 \Delta\Delta$ is the maximum value of the superconducting gap, and a non-Fermi-liquid form for . In the Fermi-liquid regime, the spectral function displays a quasiparticle peak at ; in the non-Fermi-liquid regime it possesses a broad maximum (hump) at . In between the two regimes, the spectral function has a dip at . We argue that our theory also explains the tunneling data for the superconducting density of states.

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