The numerical solution is computed using C, FORTRAN and RNPL and compared to the exact solution. We check for convergence and calculate the truncation error. A plot displaying the topology is also included.
The numerical solution is created using RNPL and a parameter survey in pulse width is conducted. For most pulses some mass falls into the black hole, and by integrating the ``conserved'' mass function over the entire region we can calculate how much mass due to the scalar field is actually there and thus find the absorption coefficient as a function of pulse width.