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I present here the results of the study of the gravitational radiationgenerated by the infall (from rest at radius $r_0$) of a point particle of mass$m_0$ into a Schwarzschild black hole of mass $M$. We use Laplace's transformmethods and find that the spectra of radiation for $\sim5M<r_0<\infty$ presentsa series of evenly spaced bumps. The total radiated energy is not monotonicallydecreasing with $r_0$, but presents a joroba (hunch-back) at around$r_0\approx4.5M$. I finally discuss the detectability of the gravitationalradiation coming from the black hole in the center of our galaxy.Comment: Latex, 4 pages, 3 figures (resume' of the talk at the 18th Texas  Symposium

Model for Gravitational Radiation from the Galactic Center: Infall of a Particle into a Black Hole