Search for the PN coefficients for the Energy flux through Gravitational
  Waves from Black-Hole Binaries using Markov Chain Monte Carlo
  In this work, the focus is on the improvement of the existing post-Newtonian
approximation for the gravitational flux from Super Massive Black Hole
Binaries. In order to improve the existing templates for LISA, we need more
accurate post-Newtonian expansions for the gravitational flux. Stochastic
search techniques like the Markov Chain Monte Carlo (MCMC) have been used
extensively for searching for sky parameters etc. The idea is to combine the
two and approach the problem of finding post-Newtonian coefficients using MCMC.
It has been shown that matching against a 5.5PN signal, with noise, the last
coefficient can be found by MCMC very easily and displays fast convergence.
Also the space for higher dimensional searches are explored.
