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Although the low frequency electronic Raman response in the superconductingstate of the cuprates can be largely understood in terms of a d-wave energygap, a long standing problem has been an explanation for the spectra observedin the $A_{1g}$ polarization orientations. We present calculations whichsuggest that the peak position of the observed $A_{1g}$ spectra is due to acollective spin fluctuation mode.Comment: 4 pages, 5 eps figure

Collective spin fluctuation mode and Raman scattering in superconducting cuprates