Black Holes, Galaxy Clusters and Gravitational Waves

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http://eprints.org/relation/isVolatileVersionOf http://etheses.bham.ac.uk/id/document/3269 http://eprints.org/relation/ispreviewThumbnailVersionOf http://etheses.bham.ac.uk/id/document/3269 http://eprints.org/relation/isVersionOf http://etheses.bham.ac.uk/id/document/3269 archive 4031 disk0/00/00/13/21 2011-02-18 12:41:51 2019-01-17 16:58:15 2011-07-19 16:33:08 thesis show 0 Del Pozzo Walter Raychaudhury Somak University of Birmingham Black Holes, Galaxy Clusters and Gravitational Waves unpub QC 10col_ephy This thesis deals with three aspects of modern astrophysical research. We propose a Bayesian data analysis framework to test alternative theories of gravity using observations of Gravitational Waves (GWs) from the inspiral phase of binary systems. We compare General Relativity predictions to the ones from a Massive Graviton theory. We can discriminate between the two theories and produce posterior probability distribution functions. We also devise a method to combine multiple observations that y increases the amount of information that is possible to extract from GWs. Using current wide-field sky survey s, in concert with the established Luminosity -- Black Hole mass relation, we calculate the mass distribution of supermassive massive black holes (SMBHs) and Active Galactic Nuclei (AGNs) in three different environments. SMBHs and radio-AGNs are concentrated in dense environments. The Black Hole Fundamental Plane predicts X-ray properties for our SMBHs and unifies modes of AGN activity in terms of the rate of accretion. Studying two-body mergers of realistic galaxy clusters, we show that these reproduce the observed metallicity distribution in the Intra Cluster Medium (ICM). We characterise entropy generation and mixing induced by the merger process. 2010-12 2010-05 graduation eng This unpublished thesis/dissertation is copyright of the author and/or third parties. The intellectual property rights of the author or third parties in respect of this work are as defined by The Copyright Designs and Patents Act 1988 or as modified by any successor legislation. Any use made of information contained in this thesis/dissertation must be in accordance with that legislation and must be properly acknowledged. Further distribution or reproduction in any format is prohibited without the permission of the copyright holder. public 221 University of Birmingham School of Physics and Astronomy d_ph na 2010-12 graduation