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Gravitational waves from binary black hole pairs have emerged as an importantobservational tool in current times. The energy of the BH - BH binary pair isradiated in the form of gravitational waves and to compensate for that energy,kinetic energy of the system decreases gradually. Consequently the mutualseparation of the objects decreases with time and tends to merge. The wholeprocess may require a very long time comparable or longer than the age of theuniverse, specially in the case of low mass mergers. We have examined the casein which a massive object compared to the individual masses comprising thebinary pair is present nearby such a system. We have found that in this casethe merging process takes place much rapidly than that of the conventionalBH-BH merging process. Scenarios with both an Intermediate Mass Black Hole(IBMH) ($10^{5}\:M_{\odot}$) as well as a Super Massive Black Hole (SMBH) havebeen studied and the latter has been found to provide a much higher overallrate for the BH-BH merger process.

Speeding up of Binary Merger Due to "Apparent" Gravitational Wave Emissions