We present an explanation of the unusual peak/dip/hump features observed in
photoemission experiments on Bi2212 at T much less than T-c. We argue that
the strong spin-fermion interaction combined with the feedback effect on t
he spin damping due to superconductivity yields a Fermi liquid form of the
fermionic spectral function for omega < 2 Delta where Delta is the maximum
value of the superconducting gap, and a nonFermi liquid form for omega > 2
Delta. In the Fermi liquid regime, the spectral function A(k(F), omega) dis
plays a quasiparticle peak at omega = Delta; in the nonFermi liquid regime
it possesses a bread maximum at omega much greater than Delta. In between t
he two regimes, the spectral function has a dip at omega similar to 2 Delta
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