Head-on collisions of black holes: The particle limit

We compute gravitational radiation waveforms, spectra, and energies for a point particle of mass $m_0$ falling from rest at radius $r_0$ into a Schwarzschild hole of mass $M$. This radiation is found to lowest order in ${(m}_0/M)$ with the use of a Laplace transform. In contrast with numerical relativity results for head-on collisions of equal-mass holes, the radiated energy is found not to be a monotonically increasing function of initial separation; there is a local radiated-energy maximum at $r_0\approx 4.5M$. The present results, along with results for infall from infinity, provide a complete catalog of waveforms and spectra for particle infall. We give a representative sample from that catalog and an interesting observation: Unlike the simple spectra for other head-on collisions (either of particle and hole, or of equal mass holes) the spectra for $\infty >r_0>\sim 5M$ show a series of evenly spaced bumps. A simple explanation is given for this. Lastly, our energy versus $r_0$ results are compared with approximation methods used elsewhere, for small and for large initial separation.