Merging phase of double black hole binaries and modelling their gravitational waves
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Abstract (EN)
In this thesis, gravitational waves that are produced by double black holes have been investigated. The amplitude of gravitational waves in case of a binary system has been determined by using the Einstein field equations. Gravitational wave modells of double black hole binaries that have different orbital parameters and mass ratio rates have been compared. The merging processes of them have been also discussed.
Author
Hakan Eser
How to Cite
Hakan Eser (Master Thesis). Merging phase of double black hole binaries and modelling their gravitational waves, 2015, Ege University.
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